aads

Friday Cephalopod: Baby done growed up [Pharyngula]

Don’t you just love those photo series of the young’uns at different ages?

Developmental staging of Octopus bimaculoides. a Whole egg photomicrograph illustrates the egg stalk and the animal pole (asterisk) where the embryonic body forms. Extent of epiboly in this stage (st) 8 embryo is marked with arrowheads. b End on view of a stage 8 embryo with the egg capsule and yolk removed. In dark field illumination, the organ primordia are visible as ectodermal and mesodermal thickenings. The mantle anlage (m) is central, the prospective mouth (mo) at the top of the panel is anterior, and the arm bud pairs (1–4) are arrayed peripherally. The folds of the collar (co) and the prospective funnel (fo, ff) fall at intermediate positions. c–f The growth of the organ systems by stage 10 is illustrated in end on (c), anterior (d), posterior (e) and left side (f) views. g–m The shape of the adult octopus emerges at middle (g–l) and late (m) embryonic stages. Illustrated are anterior (g and j), posterior (h and k) and left side (i and l) views of stage 13 (g–i) and stage 18 (j–l) embryos, and an anterior view of a stage 19 embryo (m). n and o Anterior views of O. bimaculoides (n) and its brain (o) at hatching (stage 20). A, anterior view; ey, eye; fun, funnel; gil, gill; L, lateral view; olf, olfactory organ; opt, optic lobe; P, posterior view; pf, funnel pouch; st, statocyst; supes, supraesophageal mass. Scale bars: 1mm (a), 500 μm (b–o)

Developmental staging of Octopus bimaculoides. a Whole egg photomicrograph illustrates the egg stalk and the animal pole (asterisk) where the embryonic body forms. Extent of epiboly in this stage (st) 8 embryo is marked with arrowheads. b End on view of a stage 8 embryo with the egg capsule and yolk removed. In dark field illumination, the organ primordia are visible as ectodermal and mesodermal thickenings. The mantle anlage (m) is central, the prospective mouth (mo) at the top of the panel is anterior, and the arm bud pairs (1–4) are arrayed peripherally. The folds of the collar (co) and the prospective funnel (fo, ff) fall at intermediate positions. c–f The growth of the organ systems by stage 10 is illustrated in end on (c), anterior (d), posterior (e) and left side (f) views. g–m The shape of the adult octopus emerges at middle (g–l) and late (m) embryonic stages. Illustrated are anterior (g and j), posterior (h and k) and left side (i and l) views of stage 13 (g–i) and stage 18 (j–l) embryos, and an anterior view of a stage 19 embryo (m). n and o Anterior views of O. bimaculoides (n) and its brain (o) at hatching (stage 20). A, anterior view; ey, eye; fun, funnel; gil, gill; L, lateral view; olf, olfactory organ; opt, optic lobe; P, posterior view; pf, funnel pouch; st, statocyst; supes, supraesophageal mass. Scale bars: 1mm (a), 500 μm (b–o)

Shigeno et al. Zoological Letters (2015) 1:26



from ScienceBlogs http://ift.tt/1K2VIga

Don’t you just love those photo series of the young’uns at different ages?

Developmental staging of Octopus bimaculoides. a Whole egg photomicrograph illustrates the egg stalk and the animal pole (asterisk) where the embryonic body forms. Extent of epiboly in this stage (st) 8 embryo is marked with arrowheads. b End on view of a stage 8 embryo with the egg capsule and yolk removed. In dark field illumination, the organ primordia are visible as ectodermal and mesodermal thickenings. The mantle anlage (m) is central, the prospective mouth (mo) at the top of the panel is anterior, and the arm bud pairs (1–4) are arrayed peripherally. The folds of the collar (co) and the prospective funnel (fo, ff) fall at intermediate positions. c–f The growth of the organ systems by stage 10 is illustrated in end on (c), anterior (d), posterior (e) and left side (f) views. g–m The shape of the adult octopus emerges at middle (g–l) and late (m) embryonic stages. Illustrated are anterior (g and j), posterior (h and k) and left side (i and l) views of stage 13 (g–i) and stage 18 (j–l) embryos, and an anterior view of a stage 19 embryo (m). n and o Anterior views of O. bimaculoides (n) and its brain (o) at hatching (stage 20). A, anterior view; ey, eye; fun, funnel; gil, gill; L, lateral view; olf, olfactory organ; opt, optic lobe; P, posterior view; pf, funnel pouch; st, statocyst; supes, supraesophageal mass. Scale bars: 1mm (a), 500 μm (b–o)

Developmental staging of Octopus bimaculoides. a Whole egg photomicrograph illustrates the egg stalk and the animal pole (asterisk) where the embryonic body forms. Extent of epiboly in this stage (st) 8 embryo is marked with arrowheads. b End on view of a stage 8 embryo with the egg capsule and yolk removed. In dark field illumination, the organ primordia are visible as ectodermal and mesodermal thickenings. The mantle anlage (m) is central, the prospective mouth (mo) at the top of the panel is anterior, and the arm bud pairs (1–4) are arrayed peripherally. The folds of the collar (co) and the prospective funnel (fo, ff) fall at intermediate positions. c–f The growth of the organ systems by stage 10 is illustrated in end on (c), anterior (d), posterior (e) and left side (f) views. g–m The shape of the adult octopus emerges at middle (g–l) and late (m) embryonic stages. Illustrated are anterior (g and j), posterior (h and k) and left side (i and l) views of stage 13 (g–i) and stage 18 (j–l) embryos, and an anterior view of a stage 19 embryo (m). n and o Anterior views of O. bimaculoides (n) and its brain (o) at hatching (stage 20). A, anterior view; ey, eye; fun, funnel; gil, gill; L, lateral view; olf, olfactory organ; opt, optic lobe; P, posterior view; pf, funnel pouch; st, statocyst; supes, supraesophageal mass. Scale bars: 1mm (a), 500 μm (b–o)

Shigeno et al. Zoological Letters (2015) 1:26



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Winter Circle: Brightest winter stars

Photo credit: Computer Science Geek

The Winter Circle – sometimes called the Winter Hexagon – is a big circle of bright stars on the dark dome of a winter night. At the center of the Winter Circle, you’ll find center Orion’s bright red star Betelgeuse. Rigel, Aldebaran, Capella, Procyon, Sirius, Castor and Pollux are the bright stars that make up the large, circular pattern.

Follow these links to learn more about this easy-to-find star pattern.

The Winter Circle is an asterism, not a constellation

How to spot the Winter Circle

Best months for viewing the Winter Circle

The Winter Circle is an asterism. The International Astronomical Union (IAU) decided on the 88 official constellations in the 1930s, but anyone is free to make an asterism.

An asterism is just a recognizable star pattern. It’s a bit like picking out a pattern in a cloud, although, if the name for the pattern is used often enough by enough people, it could become part of the stargazers’ lexicon – as has the name Winter Circle. The Winter Circle may well be the largest famous asterism in the heavens.

View larger. | There are many bright stars near Jupiter in 2014. The planet lies in the midst of what we stargazers in the Northern Hemisphere know as the Winter Circle. This beautiful photo captured January 11, 2014 by EarthSky Facebook friend Duke Marsh in Indiana. Thank you, Duke.

View larger. | In 2014, planet Jupiter lay in the midst of what we stargazers in the Northern Hemisphere know as the Winter Circle. EarthSky Facebook friend Duke Marsh in Indiana captured this beautiful photo on January 11, 2014. Thank you, Duke.

How to spot the Winter Circle. If you’re familiar with the winter constellation Orion, note that Rigel, the brilliant star at the lower right of Orion’s Belt, resides at the southwest corner of the Winter Circle.

Now draw an imaginary line going leftward through the three stars of Orion’s Belt to find the southernmost and brightest star of the Winter Circle, Sirius.

The opposite direction through Orion’s Belt points to Aldebaran, the star that depicts the ruddy eye in the constellation Taurus the Bull.

Castor and Pollux, the brightest stars in the constellation Gemini the Twins, are also found by way of Orion’s Belt. A line from the northwest (upper right) star of Orion’s Belt and through Betelgeuse escorts you to these two bright Gemini stars.

Look for Procyon above Sirius and below Castor and Pollux. Procyon, Sirius and Betelgeuse by themselves make up another star pattern – another asterism – often called as the Winter Triangle.

Bright Capella, the northernmost star of the Winter Circle, is found to the upper right of Castor and Pollux and the upper left of Aldebaran.

For some idea of the Winter Circle’s humongous size, an imaginary arc drawn from Sirius to Capella stretches out about one-third the way across the dome of sky.

When to see the Winter Circle When the winter solstice arrives on or near December 21, the Winter Circle rises high enough to be seen in your southeast sky at about 9 p.m. After rising, the Winter Circle swings westward across the sky, and is highest up in the south around 1 a.m. It appears in the southwest sky around 5 a.m. The western (right) half of the Winter Circle sets in the west before the onset of a winter solstice dawn.

The Winter Circle stars rise and set some 4 minutes earlier with each passing night. Therefore, on January 21, the Winter Circle is found in the same place in the sky about 2 hours earlier than it was on the winter solstice one month before. On January 21, the Winter Circle appears in the southeast around 7 p.m., highest up in the south around 11 p.m. and in the southwest at 3 a.m. In late February and early March, the Winter Circle is found in your southern sky at nightfall and early evening.

On a dark and clear moonless night, look for the soft-glowing river of stars that we call the Milky Way to meander right through the Winter Circle.

Enjoying EarthSky? Sign up for our free daily newsletter today!

Bottom line: The Winter Circle is a large circular pattern on the sky’s dome, consisting of the bright stars Rigel, Aldebaran, Capella, Procyon, Sirius, Castor and Pollux.



from EarthSky http://ift.tt/1DyYKJy

Photo credit: Computer Science Geek

The Winter Circle – sometimes called the Winter Hexagon – is a big circle of bright stars on the dark dome of a winter night. At the center of the Winter Circle, you’ll find center Orion’s bright red star Betelgeuse. Rigel, Aldebaran, Capella, Procyon, Sirius, Castor and Pollux are the bright stars that make up the large, circular pattern.

Follow these links to learn more about this easy-to-find star pattern.

The Winter Circle is an asterism, not a constellation

How to spot the Winter Circle

Best months for viewing the Winter Circle

The Winter Circle is an asterism. The International Astronomical Union (IAU) decided on the 88 official constellations in the 1930s, but anyone is free to make an asterism.

An asterism is just a recognizable star pattern. It’s a bit like picking out a pattern in a cloud, although, if the name for the pattern is used often enough by enough people, it could become part of the stargazers’ lexicon – as has the name Winter Circle. The Winter Circle may well be the largest famous asterism in the heavens.

View larger. | There are many bright stars near Jupiter in 2014. The planet lies in the midst of what we stargazers in the Northern Hemisphere know as the Winter Circle. This beautiful photo captured January 11, 2014 by EarthSky Facebook friend Duke Marsh in Indiana. Thank you, Duke.

View larger. | In 2014, planet Jupiter lay in the midst of what we stargazers in the Northern Hemisphere know as the Winter Circle. EarthSky Facebook friend Duke Marsh in Indiana captured this beautiful photo on January 11, 2014. Thank you, Duke.

How to spot the Winter Circle. If you’re familiar with the winter constellation Orion, note that Rigel, the brilliant star at the lower right of Orion’s Belt, resides at the southwest corner of the Winter Circle.

Now draw an imaginary line going leftward through the three stars of Orion’s Belt to find the southernmost and brightest star of the Winter Circle, Sirius.

The opposite direction through Orion’s Belt points to Aldebaran, the star that depicts the ruddy eye in the constellation Taurus the Bull.

Castor and Pollux, the brightest stars in the constellation Gemini the Twins, are also found by way of Orion’s Belt. A line from the northwest (upper right) star of Orion’s Belt and through Betelgeuse escorts you to these two bright Gemini stars.

Look for Procyon above Sirius and below Castor and Pollux. Procyon, Sirius and Betelgeuse by themselves make up another star pattern – another asterism – often called as the Winter Triangle.

Bright Capella, the northernmost star of the Winter Circle, is found to the upper right of Castor and Pollux and the upper left of Aldebaran.

For some idea of the Winter Circle’s humongous size, an imaginary arc drawn from Sirius to Capella stretches out about one-third the way across the dome of sky.

When to see the Winter Circle When the winter solstice arrives on or near December 21, the Winter Circle rises high enough to be seen in your southeast sky at about 9 p.m. After rising, the Winter Circle swings westward across the sky, and is highest up in the south around 1 a.m. It appears in the southwest sky around 5 a.m. The western (right) half of the Winter Circle sets in the west before the onset of a winter solstice dawn.

The Winter Circle stars rise and set some 4 minutes earlier with each passing night. Therefore, on January 21, the Winter Circle is found in the same place in the sky about 2 hours earlier than it was on the winter solstice one month before. On January 21, the Winter Circle appears in the southeast around 7 p.m., highest up in the south around 11 p.m. and in the southwest at 3 a.m. In late February and early March, the Winter Circle is found in your southern sky at nightfall and early evening.

On a dark and clear moonless night, look for the soft-glowing river of stars that we call the Milky Way to meander right through the Winter Circle.

Enjoying EarthSky? Sign up for our free daily newsletter today!

Bottom line: The Winter Circle is a large circular pattern on the sky’s dome, consisting of the bright stars Rigel, Aldebaran, Capella, Procyon, Sirius, Castor and Pollux.



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Global Warming Over The Next Decade: Candidates take note. [Greg Laden's Blog]

The Time Scales of Political and Climate Change Matter

The US is engaged in the laborious process of electing a new leader, who will likely be President for 8 years. Climate change has finally become an issue in US electoral politics. The climate policies of the next US President, and the Congress, will have a direct impact on the climate, because those policies will affect how much fossil carbon is put into the atmosphere over coming decades. So it is vital to consider what the climate may do during the next administration and the longer period that will include that administration’s effective legacy period, more or less the next decade starting now.

There is evidence that the ongoing warming of the planet’s surface is likely accelerate to in the near future. Recent decades have seen the Earth’s surface temperatures go up at a relatively slower than average rate compared to earlier decades. The best available science suggests that this rate is about to increase. We can expect a series of mostly record breaking months and years that will add up to an alarmingly warm planet.

(The graphic showing continued global warming through 2015 at the top of the post is from here.)

The Rate Of Global Warming Is About To Increase

I wrote about this last February, in discussing a paper by Steinmann, Mann, and Miller, that said:

The recent slowdown in global warming has brought into question the reliability of climate model projections of future temperature change and has led to a vigorous debate over whether this slowdown is the result of naturally occurring, internal variability or forcing external to Earth’s climate system. … we applied a semi-empirical approach that combines climate observations and model simulations to estimate Atlantic- and Pacific-based internal multidecadal variability (termed “AMO” and “PMO,” respectively). Using this method [we show that] competition between a modest positive peak in the AMO and a substantially negative-trending PMO … produce a slowdown or “false pause” in warming of the past decade.

That research was also discussed by Chris Mooney and John Upton. John Upton updated this discussion earlier this week, noting,

Cyclical changes in the Pacific Ocean have thrown earth’s surface into what may be an unprecedented warming spurt, following a global warming slowdown that lasted about 15 years.

While El Niño is being blamed for an outbreak of floods, storms and unseasonable temperatures across the planet, a much slower-moving cycle of the Pacific Ocean has also been playing a role in record-breaking warmth. The recent effects of both ocean cycles are being amplified by climate change.

Why Does The Rate of Global Warming Vary?

This is pretty complicated, and even those who are on the cutting edge of this research are cautious in making links between their models and the on the ground reality of warming in the near future. The long term rise in surface temperature, which is what we usually refer to when using the term “Global Warming,” is not steady and smooth, but instead, it is rather squiggly. But the ups and downs that accompany the general upward trend are mostly caused by things that are known.

The sun provides the energy to warm the Earth’s surface, and this contribution changes over time, but the sun varies very little in its output, and thus has less influence than other factors. The sun’s energy warms the Earth mainly because our atmosphere contains some greenhouse gasses. The more greenhouse gas the more surface warmth. As humans add greenhouse gas (mainly CO2 released by burning fossil fuel) the surface temperature eventually rises to a higher equilibrium. But the variation in the sun’s strength is hardly observable.

Aerosols, also known as dust or in some cases pollution (or airborne particles) can reduce the surface temperature by intercepting some of the Sun’s energy on its way to the surface (I oversimplify). These aerosols come mainly from industrial pollution and volcanoes. The addition of a large amount of aerosol into the atmosphere by a major volcanic eruption can have a relative cooling effect but one that lasts for a short duration, because the dust eventually settles.

Screen Shot 2016-01-07 at 11.09.08 AM

There are many other important factors. Changes in land use patterns that cause changes in effectiveness of carbon sinks – places where atmospheric carbon (mainly CO2) is trapped in solid form by biological systems – increase atmospheric CO2. Melting glacial ice takes up heat and influences surface temperatures. And so on.

The biggest single factor that imposes a squiggle on the upward trending line of surface temperature is the interaction between the atmosphere and the ocean. Close to 100% of the extra heat added to the Earth’s system by global warming ends up in the world’s oceans. The heat is moved into the ocean because the surface warms up (from the sun) but surface water is constantly being mixed into lower levels of the ocean, and visa versa. When it comes to the Earth’s surface temperature, the ocean is the dog and the surface is the tail.

A famous, and now perhaps infamous, example of this interaction between ocean and air is the El Niño Southern Oscillation (ENSO). Here’s the simple version (see here for more detail). The equatorial Pacific’s surface is constantly being warmed by the sun. The surface waters are usually blown towards the west by trade winds. (Those trade winds are caused in part by the rotation of the Earth, and in part by the ongoing redistribution of excess tropical heat towards the poles). This causes warm water to move west, where it is potentially subducted into the ocean, moving heat into the sea. That heat eventually may work its way out of the ocean through various currents.

During many years, the ins and the outs are similar. During some years, La Niña years, the amount of heat moving into the ocean is larger, which can cause a small cooling influence on the planet. Every now and then, the reverse happens. This involves complicated changes in trade winds and ocean currents. A good chunk of the heat that has been stored in the Pacific now emerges and is added very abruptly, over a period of several months, to the atmosphere. This is an El Niño event. We are at this moment experiencing one of the strongest El Niño events ever recorded, possibly the strongest (we won’t know until it has been going a while longer.)

ENSO is one, in fact the biggest, example of atmosphere-ocean interaction that influences surface temperatures. But, ENSO is only one part of the interaction between the Pacific and the atmosphere. There is also a phenomenon known as the Pacific Multidecadal Oscillation (PMO). For its part, the Atlantic has the AMO, a similar system. These phenomena are characterized by a general transfer of heat either into or out of the ocean, with several years in a row seeing more heat move into the ocean, followed by several years in a row of more heat moving out of the ocean.

Though ENSO and the PMO are distinct processes, they may be related. I asked climate scientist Michael Mann if he views El Nino as part of the larger scale system of PMO, or if El Niño essentially rides on top of, or acts independently from PMO. He told me, “I would say the latter. At some level, the PMO really describes the long-term changes in the frequency and magnitude of El Niño and La Niña events, i.e. change in the behavior of ENSO on multidecadal timescales, and it will appear as multidecadal oscillation with an ENSO-like signature with some modifications due to the fact that certain processes, like gyre-advection and subduction of water masses, act on longer timescales and do they are seen with the PMO bot not El Niño or La Niña.”

The influence of ENSO on global surface temperatures is well illustrated in this graphic from Skeptical Science.

AllENSOwtrends

Here, the surface temperature anomaly is shown from the late 1960s to recent (does not include the last few years). The annual values are classified into years during which ENSO was neutral, or neutral with volcanic influences, La Nina years, and El Niño years with or without volcanoes. A separate trend line is shown for years that should be relatively warm (El Niño), relatively cool (La Niña), and years that should be about average.

The influence of the PMO is also apparent.

Screen Shot 2016-01-07 at 12.18.44 PM

This graphic shows the measurement of the Pacific Decadal Oscillation and the surface temperature anomalies. The data are averaged out over a two year cycle (otherwise the PDO would be way too squiggly to be useful visually). Notice that during periods when the PDO is positive (adding heat to the atmosphere) there tends to be a stronger upward trend of surface temperature, and when the PDO is negative, the surface temperature rises more slowly. Remember, a lot of other factors, such as aerosols, are influencing the temperature line, so this relationship is quite imperfect.

Also notice that both lines trend dramatically upward near the end of the graph. This reflects the last couple of years (including right now) of dramatically increasing surface temperatures, and an apparent positive shift in the PDO. Just as interesting is the negative PDO associated with a reduced upward trend in the surface temperatures, fondly known by many as the “Hiatus” or “Pause” in global warming, during the first part of the 20th century. Indeed, it is likely that this slowdown (not really a pause) in warming is largely a result of a higher rate of excess heat being plowed into the oceans, and less coming back out. This is also a period during which the ENSO system produced no strong El Niños.

But the PDO is, as noted, part of a larger phenomenon of ocean-atmosphere interaction. The study noted above by Steinman, Mann, and Miller takes a broad view of these oscillations and their impact on climate. In RealClimate, Mann writes,

We focused on the Northern Hemisphere and the role played by two climate oscillations known as the Atlantic Multidecadal Oscillation or “AMO” … and the … Pacific Multidecadal Oscillation or “PMO”… The oscillation in Northern Hemisphere average temperatures (which we term the Northern Hemisphere Multidecadal Oscillation or “NMO”) is found to result from a combination of the AMO and PMO.

…Our conclusion that natural cooling in the Pacific is a principal contributor to the recent slowdown in large-scale warming is consistent with some other recent studies…

…the state-of-the-art climate model simulations analyzed in our current study suggest that this phenomenon is a manifestation of purely random, internal oscillations in the climate system.

This finding has potential ramifications for the climate changes we will see in the decades ahead. As we note in the last line of our article,

Given the pattern of past historical variation, this trend will likely reverse with internal variability, instead adding to anthropogenic warming in the coming decades.

That is perhaps the most worrying implication of our study, for it implies that the “false pause” may simply have been a cause for false complacency, when it comes to averting dangerous climate change.

What Will Global Warming Do During The Next Decade?

Have political leaders and representatives been lukewarm on climate change over recent years in part because the climate change itself has been less dramatic than it could be? And, conversely, is it the case that the next couple of decades will see a reverse in both? I asked Michael Mann if his research indicated that the indicators such as the PMO, AMO, or the derived NMO, show that the oceans are about to contribute to a speedup in warming. He told me, “…both PMO and AMO contribute to NMO, but in recent decades PMO has been the dominant player, and yes, I would expect to see the recent turn toward El Nino-like conditions and enhanced hemispheric/global warming as an apparent upturn in the NMO, though it is always difficult if not impossible to diagnose true change in the low-frequency signal right at the end of a time series.”

Let’s have a closer look at the influence of the PDO on global surface temperatures. Since the human influence on the atmosphere has grown over time, we want to focus on more recent decades when the input of additional greenhouse gases had already risen to a high level. This graphic shows the NASA GISS surface temperature anomaly values (the dots) from 1980 to the present, but with some trend lines added in.

Screen Shot 2016-01-08 at 10.19.19 AM

The black dots and the curvy trend line to the left represent a period of time when the PDO was positive, but also includes a depression in surface temperature because of the eruption of Mount Pinatubo. I made the trend line a “second order polynomial” instead of a regular straight line. A polynomial equation can capture internal curviness of a series of data.

(A polynomial equation that is of the same “order” as the number of points in the data set would, theoretically, zig and zag back and forth to account for each data point’s position which would be absurd. One must be careful with poylnomials. But a second order polynomial can honestly reflect a modest curviness in a series of data, and in this case, helps the line do its job at visually presenting a short term pattern.)

The second series of data, in blue, shows a period of mostly negative PMO, again, with a second order polynomial line drawn on it. This is the period of time that includes the so-called “hiatus” in global warming, when the upward trend of increasing surface temperature was somewhat attenuated. That attenuation was probably caused by a number of factors, and in fact, at least one of those factors had to do with inadequacies of the data itself, in that the measurements fail to account for extreme warming in the Arctic and parts of Africa. But the negative PMO, and likely, according to Steinmann, Mann and Miller, a larger scale relationship between atmosphere and ocean, seem to have somewhat flattened out the line.

But then we come to the third part of the data, in red. The ocean-atmosphere relationship has switched the other way. The PMO has been positive since the last part of 2013, and over a smaller and more recent time frame, we have been experiencing a strong El Niño.

This graphic does a nice job showing how short and medium term upward and downward trends eventually cancel out to produce a single upward trend in global surface temperature. Very short term shifts such as a given El Niño event or a given Volcanic eruption cause the most obvious squiggles. Somewhat longer term, multi-decade trends such as the PDO cause longer parts of the series of measurements to rise more or less quickly. But over nearly 40 years shown here, and longer periods, all the ups and downs average out to a single trend that can be reliably projected for a reasonable period of time.

Will More Rapid Global Warming Spur A More Effective Policy Response?

These ups and downs in the rate of warming are not important to the long term trend, but they are important because of their immediate effects on weather. And that is all that should matter. But these short and medium term trends, as well as even more immediate events such as individual storms, take on a greater importance that has nothing to do with the science of climate change itself. These changes affect the way politicians, advocates, and the general public, regard climate change, and serve to motivate or attenuate action on one side of the false debate or another.

We have known enough about climate change and its causes to have started the shift from fossil fuels to alternative strategies for producing energy long before 1980, but have in fact done very little to solve this problem. Initially, climate change seemed more like a thing of the future, and in fact, had relatively little impact on the most influential and powerful nations and people. Disruptions of weather patterns started to become more apparent around or just before 1980, but for the next few decades anti-science forces were well organized, and their efforts were enhanced, at the beginning of the 21st century, by the unthinking and unknowing process of air-sea interactions that reduced the rate of surface temperature increase even while weather patterns continued to become more and more chaotic.

But the truth is, a widespread flood in the American bottomlands defeats a snowball in the hands of a contrarian Senator. Eventually, more and more people in the US have been affected by inclement weather, and the frequency with which destructive storms of various kinds hammer the same subpopulation again and again has gone up. The symbolic snowball melts under the cold hard stare of voters who wonder how they are going to rebuild their lives after floods, severe storms, and droughts have taken away their property, in some cases their loved ones, and raised their insurance rates.

So the question emerges, will the next decade or so be a period of increased, or of attenuated, motivation from Mother Nature to act on climate change? The rational actor will act now, because we know that the greenhouse gas we pump into the atmosphere today changes the climate for decades to come. The reactionary actor with little capability or interest in thinking long term (i.e. most people) will be mollified by a decade with few severe storms, not much flooding, a seemingly secure food supply, and a snowball or two.

I left the projection of the future as a single estimate based on the past several decades (all the data shown on the graph). I could have imposed a more upward trending line, maybe a nice curve like these polynomials show, as an extension to the blue line. But since the graphic is going out a couple more decades, and the ups and downs average out over several decades, I think it is fair enough to use the linear projection shown by the red dotted line.

I’m not actually making a prediction of future global surface temperatures here. What I’m showing instead is that two things seem to be true. First, long term (over decades) global warming has happened and will likely to continue at about the same pace for a while. This has been going on long enough that by now we should viscerally understand that the squiggles are misleading. Second, the last couple of decades have been a period of reduced warming, but that period is likely over, and we are likely to experience an increased rate of warming.

Will surface temperatures during the term of the next POTUS squiggle about mostly above that red dotted line on this graph, or will those temperatures squiggle up and down above and below the line, or even below it? Based on the best available science, that first choice is most likely. Whomever ends up being POTUS, and the corresponding Congress, will be enacting (or failing to enact) policy during a period of surface temperature increasing at a rate higher than we have in recent years.

A vitally important known unknown, is what will the effects of such a rise in surface temperature be. We have various levels of confidence that storminess, changes in the distribution of rainfall, drought, and through the melting of glacial ice, sea level rise, are all important forms of climate disruption we are currently experiencing, and we should expect more of the same. The unknown is whether or not we should expect a dramatic acceleration of these changes in the short term future.

How will the insurance industry address an increase in widespread catastrophic damage caused by storms and floods? Will the government have to underwrite future losses, or will disaster insurance simply become something we can’t have? Will there be damage to our food production system that ultimately results in less certainly in the food supply, and how will we deal with that? The well known “reugee crisis” is a climate refugee crisis. But it may be a small one compared to what could happen in the future. Will we need to restrict development in mountain areas more subject to fires, and withdraw settlement from low lying areas along major rivers? How will we address more widespread and more severe killer heat waves?

The battle to preserve the use of fossil fuels exists at the state level in the US. Should we have a national effort to stop the legislatures in red states from putting the kibosh on local development of clean energy sources, either by energy utilities or individual home owners?

Sea level rise has already had several negative effects, but it is also is a longer term issue, and is perhaps among the most serious consequences of human greenhouse gas pollution. At some point, American politicians in some areas will be faced not with the question, “Will this or that Congressional district be represented by a Democrat or a Republican,” but rather, “Where the people who lived in this district go now that the sea is taking it?”

Over time, I think the social and political will to address climate change has grown, though very slowly. It might seem that the effects of climate change right now are fairly severe, with floods and fires and all that being more common. But while these effects are real and important, they have been minor compared to what the future is likely to bring. The anemic but positive growth of willingness to act has occurred in a political and physical climate that is less than nurturing of dramatic and effective action.

Whoever is elected president this time around, and the Congress, will serve during a period when the people’s will to act will transform from that inspired by activists pushing for change, to outcries of a larger number of desperate and suffering newcomers to the rational side of the climate change discussion.

Expect a sea change in the politics of science policy.



from ScienceBlogs http://ift.tt/1n8eTjM

The Time Scales of Political and Climate Change Matter

The US is engaged in the laborious process of electing a new leader, who will likely be President for 8 years. Climate change has finally become an issue in US electoral politics. The climate policies of the next US President, and the Congress, will have a direct impact on the climate, because those policies will affect how much fossil carbon is put into the atmosphere over coming decades. So it is vital to consider what the climate may do during the next administration and the longer period that will include that administration’s effective legacy period, more or less the next decade starting now.

There is evidence that the ongoing warming of the planet’s surface is likely accelerate to in the near future. Recent decades have seen the Earth’s surface temperatures go up at a relatively slower than average rate compared to earlier decades. The best available science suggests that this rate is about to increase. We can expect a series of mostly record breaking months and years that will add up to an alarmingly warm planet.

(The graphic showing continued global warming through 2015 at the top of the post is from here.)

The Rate Of Global Warming Is About To Increase

I wrote about this last February, in discussing a paper by Steinmann, Mann, and Miller, that said:

The recent slowdown in global warming has brought into question the reliability of climate model projections of future temperature change and has led to a vigorous debate over whether this slowdown is the result of naturally occurring, internal variability or forcing external to Earth’s climate system. … we applied a semi-empirical approach that combines climate observations and model simulations to estimate Atlantic- and Pacific-based internal multidecadal variability (termed “AMO” and “PMO,” respectively). Using this method [we show that] competition between a modest positive peak in the AMO and a substantially negative-trending PMO … produce a slowdown or “false pause” in warming of the past decade.

That research was also discussed by Chris Mooney and John Upton. John Upton updated this discussion earlier this week, noting,

Cyclical changes in the Pacific Ocean have thrown earth’s surface into what may be an unprecedented warming spurt, following a global warming slowdown that lasted about 15 years.

While El Niño is being blamed for an outbreak of floods, storms and unseasonable temperatures across the planet, a much slower-moving cycle of the Pacific Ocean has also been playing a role in record-breaking warmth. The recent effects of both ocean cycles are being amplified by climate change.

Why Does The Rate of Global Warming Vary?

This is pretty complicated, and even those who are on the cutting edge of this research are cautious in making links between their models and the on the ground reality of warming in the near future. The long term rise in surface temperature, which is what we usually refer to when using the term “Global Warming,” is not steady and smooth, but instead, it is rather squiggly. But the ups and downs that accompany the general upward trend are mostly caused by things that are known.

The sun provides the energy to warm the Earth’s surface, and this contribution changes over time, but the sun varies very little in its output, and thus has less influence than other factors. The sun’s energy warms the Earth mainly because our atmosphere contains some greenhouse gasses. The more greenhouse gas the more surface warmth. As humans add greenhouse gas (mainly CO2 released by burning fossil fuel) the surface temperature eventually rises to a higher equilibrium. But the variation in the sun’s strength is hardly observable.

Aerosols, also known as dust or in some cases pollution (or airborne particles) can reduce the surface temperature by intercepting some of the Sun’s energy on its way to the surface (I oversimplify). These aerosols come mainly from industrial pollution and volcanoes. The addition of a large amount of aerosol into the atmosphere by a major volcanic eruption can have a relative cooling effect but one that lasts for a short duration, because the dust eventually settles.

Screen Shot 2016-01-07 at 11.09.08 AM

There are many other important factors. Changes in land use patterns that cause changes in effectiveness of carbon sinks – places where atmospheric carbon (mainly CO2) is trapped in solid form by biological systems – increase atmospheric CO2. Melting glacial ice takes up heat and influences surface temperatures. And so on.

The biggest single factor that imposes a squiggle on the upward trending line of surface temperature is the interaction between the atmosphere and the ocean. Close to 100% of the extra heat added to the Earth’s system by global warming ends up in the world’s oceans. The heat is moved into the ocean because the surface warms up (from the sun) but surface water is constantly being mixed into lower levels of the ocean, and visa versa. When it comes to the Earth’s surface temperature, the ocean is the dog and the surface is the tail.

A famous, and now perhaps infamous, example of this interaction between ocean and air is the El Niño Southern Oscillation (ENSO). Here’s the simple version (see here for more detail). The equatorial Pacific’s surface is constantly being warmed by the sun. The surface waters are usually blown towards the west by trade winds. (Those trade winds are caused in part by the rotation of the Earth, and in part by the ongoing redistribution of excess tropical heat towards the poles). This causes warm water to move west, where it is potentially subducted into the ocean, moving heat into the sea. That heat eventually may work its way out of the ocean through various currents.

During many years, the ins and the outs are similar. During some years, La Niña years, the amount of heat moving into the ocean is larger, which can cause a small cooling influence on the planet. Every now and then, the reverse happens. This involves complicated changes in trade winds and ocean currents. A good chunk of the heat that has been stored in the Pacific now emerges and is added very abruptly, over a period of several months, to the atmosphere. This is an El Niño event. We are at this moment experiencing one of the strongest El Niño events ever recorded, possibly the strongest (we won’t know until it has been going a while longer.)

ENSO is one, in fact the biggest, example of atmosphere-ocean interaction that influences surface temperatures. But, ENSO is only one part of the interaction between the Pacific and the atmosphere. There is also a phenomenon known as the Pacific Multidecadal Oscillation (PMO). For its part, the Atlantic has the AMO, a similar system. These phenomena are characterized by a general transfer of heat either into or out of the ocean, with several years in a row seeing more heat move into the ocean, followed by several years in a row of more heat moving out of the ocean.

Though ENSO and the PMO are distinct processes, they may be related. I asked climate scientist Michael Mann if he views El Nino as part of the larger scale system of PMO, or if El Niño essentially rides on top of, or acts independently from PMO. He told me, “I would say the latter. At some level, the PMO really describes the long-term changes in the frequency and magnitude of El Niño and La Niña events, i.e. change in the behavior of ENSO on multidecadal timescales, and it will appear as multidecadal oscillation with an ENSO-like signature with some modifications due to the fact that certain processes, like gyre-advection and subduction of water masses, act on longer timescales and do they are seen with the PMO bot not El Niño or La Niña.”

The influence of ENSO on global surface temperatures is well illustrated in this graphic from Skeptical Science.

AllENSOwtrends

Here, the surface temperature anomaly is shown from the late 1960s to recent (does not include the last few years). The annual values are classified into years during which ENSO was neutral, or neutral with volcanic influences, La Nina years, and El Niño years with or without volcanoes. A separate trend line is shown for years that should be relatively warm (El Niño), relatively cool (La Niña), and years that should be about average.

The influence of the PMO is also apparent.

Screen Shot 2016-01-07 at 12.18.44 PM

This graphic shows the measurement of the Pacific Decadal Oscillation and the surface temperature anomalies. The data are averaged out over a two year cycle (otherwise the PDO would be way too squiggly to be useful visually). Notice that during periods when the PDO is positive (adding heat to the atmosphere) there tends to be a stronger upward trend of surface temperature, and when the PDO is negative, the surface temperature rises more slowly. Remember, a lot of other factors, such as aerosols, are influencing the temperature line, so this relationship is quite imperfect.

Also notice that both lines trend dramatically upward near the end of the graph. This reflects the last couple of years (including right now) of dramatically increasing surface temperatures, and an apparent positive shift in the PDO. Just as interesting is the negative PDO associated with a reduced upward trend in the surface temperatures, fondly known by many as the “Hiatus” or “Pause” in global warming, during the first part of the 20th century. Indeed, it is likely that this slowdown (not really a pause) in warming is largely a result of a higher rate of excess heat being plowed into the oceans, and less coming back out. This is also a period during which the ENSO system produced no strong El Niños.

But the PDO is, as noted, part of a larger phenomenon of ocean-atmosphere interaction. The study noted above by Steinman, Mann, and Miller takes a broad view of these oscillations and their impact on climate. In RealClimate, Mann writes,

We focused on the Northern Hemisphere and the role played by two climate oscillations known as the Atlantic Multidecadal Oscillation or “AMO” … and the … Pacific Multidecadal Oscillation or “PMO”… The oscillation in Northern Hemisphere average temperatures (which we term the Northern Hemisphere Multidecadal Oscillation or “NMO”) is found to result from a combination of the AMO and PMO.

…Our conclusion that natural cooling in the Pacific is a principal contributor to the recent slowdown in large-scale warming is consistent with some other recent studies…

…the state-of-the-art climate model simulations analyzed in our current study suggest that this phenomenon is a manifestation of purely random, internal oscillations in the climate system.

This finding has potential ramifications for the climate changes we will see in the decades ahead. As we note in the last line of our article,

Given the pattern of past historical variation, this trend will likely reverse with internal variability, instead adding to anthropogenic warming in the coming decades.

That is perhaps the most worrying implication of our study, for it implies that the “false pause” may simply have been a cause for false complacency, when it comes to averting dangerous climate change.

What Will Global Warming Do During The Next Decade?

Have political leaders and representatives been lukewarm on climate change over recent years in part because the climate change itself has been less dramatic than it could be? And, conversely, is it the case that the next couple of decades will see a reverse in both? I asked Michael Mann if his research indicated that the indicators such as the PMO, AMO, or the derived NMO, show that the oceans are about to contribute to a speedup in warming. He told me, “…both PMO and AMO contribute to NMO, but in recent decades PMO has been the dominant player, and yes, I would expect to see the recent turn toward El Nino-like conditions and enhanced hemispheric/global warming as an apparent upturn in the NMO, though it is always difficult if not impossible to diagnose true change in the low-frequency signal right at the end of a time series.”

Let’s have a closer look at the influence of the PDO on global surface temperatures. Since the human influence on the atmosphere has grown over time, we want to focus on more recent decades when the input of additional greenhouse gases had already risen to a high level. This graphic shows the NASA GISS surface temperature anomaly values (the dots) from 1980 to the present, but with some trend lines added in.

Screen Shot 2016-01-08 at 10.19.19 AM

The black dots and the curvy trend line to the left represent a period of time when the PDO was positive, but also includes a depression in surface temperature because of the eruption of Mount Pinatubo. I made the trend line a “second order polynomial” instead of a regular straight line. A polynomial equation can capture internal curviness of a series of data.

(A polynomial equation that is of the same “order” as the number of points in the data set would, theoretically, zig and zag back and forth to account for each data point’s position which would be absurd. One must be careful with poylnomials. But a second order polynomial can honestly reflect a modest curviness in a series of data, and in this case, helps the line do its job at visually presenting a short term pattern.)

The second series of data, in blue, shows a period of mostly negative PMO, again, with a second order polynomial line drawn on it. This is the period of time that includes the so-called “hiatus” in global warming, when the upward trend of increasing surface temperature was somewhat attenuated. That attenuation was probably caused by a number of factors, and in fact, at least one of those factors had to do with inadequacies of the data itself, in that the measurements fail to account for extreme warming in the Arctic and parts of Africa. But the negative PMO, and likely, according to Steinmann, Mann and Miller, a larger scale relationship between atmosphere and ocean, seem to have somewhat flattened out the line.

But then we come to the third part of the data, in red. The ocean-atmosphere relationship has switched the other way. The PMO has been positive since the last part of 2013, and over a smaller and more recent time frame, we have been experiencing a strong El Niño.

This graphic does a nice job showing how short and medium term upward and downward trends eventually cancel out to produce a single upward trend in global surface temperature. Very short term shifts such as a given El Niño event or a given Volcanic eruption cause the most obvious squiggles. Somewhat longer term, multi-decade trends such as the PDO cause longer parts of the series of measurements to rise more or less quickly. But over nearly 40 years shown here, and longer periods, all the ups and downs average out to a single trend that can be reliably projected for a reasonable period of time.

Will More Rapid Global Warming Spur A More Effective Policy Response?

These ups and downs in the rate of warming are not important to the long term trend, but they are important because of their immediate effects on weather. And that is all that should matter. But these short and medium term trends, as well as even more immediate events such as individual storms, take on a greater importance that has nothing to do with the science of climate change itself. These changes affect the way politicians, advocates, and the general public, regard climate change, and serve to motivate or attenuate action on one side of the false debate or another.

We have known enough about climate change and its causes to have started the shift from fossil fuels to alternative strategies for producing energy long before 1980, but have in fact done very little to solve this problem. Initially, climate change seemed more like a thing of the future, and in fact, had relatively little impact on the most influential and powerful nations and people. Disruptions of weather patterns started to become more apparent around or just before 1980, but for the next few decades anti-science forces were well organized, and their efforts were enhanced, at the beginning of the 21st century, by the unthinking and unknowing process of air-sea interactions that reduced the rate of surface temperature increase even while weather patterns continued to become more and more chaotic.

But the truth is, a widespread flood in the American bottomlands defeats a snowball in the hands of a contrarian Senator. Eventually, more and more people in the US have been affected by inclement weather, and the frequency with which destructive storms of various kinds hammer the same subpopulation again and again has gone up. The symbolic snowball melts under the cold hard stare of voters who wonder how they are going to rebuild their lives after floods, severe storms, and droughts have taken away their property, in some cases their loved ones, and raised their insurance rates.

So the question emerges, will the next decade or so be a period of increased, or of attenuated, motivation from Mother Nature to act on climate change? The rational actor will act now, because we know that the greenhouse gas we pump into the atmosphere today changes the climate for decades to come. The reactionary actor with little capability or interest in thinking long term (i.e. most people) will be mollified by a decade with few severe storms, not much flooding, a seemingly secure food supply, and a snowball or two.

I left the projection of the future as a single estimate based on the past several decades (all the data shown on the graph). I could have imposed a more upward trending line, maybe a nice curve like these polynomials show, as an extension to the blue line. But since the graphic is going out a couple more decades, and the ups and downs average out over several decades, I think it is fair enough to use the linear projection shown by the red dotted line.

I’m not actually making a prediction of future global surface temperatures here. What I’m showing instead is that two things seem to be true. First, long term (over decades) global warming has happened and will likely to continue at about the same pace for a while. This has been going on long enough that by now we should viscerally understand that the squiggles are misleading. Second, the last couple of decades have been a period of reduced warming, but that period is likely over, and we are likely to experience an increased rate of warming.

Will surface temperatures during the term of the next POTUS squiggle about mostly above that red dotted line on this graph, or will those temperatures squiggle up and down above and below the line, or even below it? Based on the best available science, that first choice is most likely. Whomever ends up being POTUS, and the corresponding Congress, will be enacting (or failing to enact) policy during a period of surface temperature increasing at a rate higher than we have in recent years.

A vitally important known unknown, is what will the effects of such a rise in surface temperature be. We have various levels of confidence that storminess, changes in the distribution of rainfall, drought, and through the melting of glacial ice, sea level rise, are all important forms of climate disruption we are currently experiencing, and we should expect more of the same. The unknown is whether or not we should expect a dramatic acceleration of these changes in the short term future.

How will the insurance industry address an increase in widespread catastrophic damage caused by storms and floods? Will the government have to underwrite future losses, or will disaster insurance simply become something we can’t have? Will there be damage to our food production system that ultimately results in less certainly in the food supply, and how will we deal with that? The well known “reugee crisis” is a climate refugee crisis. But it may be a small one compared to what could happen in the future. Will we need to restrict development in mountain areas more subject to fires, and withdraw settlement from low lying areas along major rivers? How will we address more widespread and more severe killer heat waves?

The battle to preserve the use of fossil fuels exists at the state level in the US. Should we have a national effort to stop the legislatures in red states from putting the kibosh on local development of clean energy sources, either by energy utilities or individual home owners?

Sea level rise has already had several negative effects, but it is also is a longer term issue, and is perhaps among the most serious consequences of human greenhouse gas pollution. At some point, American politicians in some areas will be faced not with the question, “Will this or that Congressional district be represented by a Democrat or a Republican,” but rather, “Where the people who lived in this district go now that the sea is taking it?”

Over time, I think the social and political will to address climate change has grown, though very slowly. It might seem that the effects of climate change right now are fairly severe, with floods and fires and all that being more common. But while these effects are real and important, they have been minor compared to what the future is likely to bring. The anemic but positive growth of willingness to act has occurred in a political and physical climate that is less than nurturing of dramatic and effective action.

Whoever is elected president this time around, and the Congress, will serve during a period when the people’s will to act will transform from that inspired by activists pushing for change, to outcries of a larger number of desperate and suffering newcomers to the rational side of the climate change discussion.

Expect a sea change in the politics of science policy.



from ScienceBlogs http://ift.tt/1n8eTjM

Wonder Endlessly timelapse of California skies

This gorgeous timelapse was created by our friend Jack Fusco. He calls it Wonder Endlessly. Jack said:

The title is a reflection of the desire to always seek new adventures. There are few things that can match the overwhelming sense of wonder felt when you’re looking up at a sky full of stars. Keeping that strong sense of wonder is what makes me want to head in to the middle of nowhere in the dark, to climb across wet rocks and dodge waves to capture something new. That feeling is something that I hoped to capture with this timelapse.

How did he create it? Jack said:

Hours of scouting and planning went in to each of the 26 different sequences in the video. Some were planned months in advance to coordinate the tide with right moon phase.

Here’s his technical info:

Equipment –
Cameras: Sony A7R2 , Nikon D800E
Lenses: Sigma 24mm f/1.4 ART, Sigma 50mm f/1.4 ART, Nikon 14-24 f/2.8
Motion Control: Rhino EVO & Motion Timelapse slider
Tripod: Feisol CT- 3442
Music: Dan Phillipson – Ascend

Some locations include: La Jolla, Solana Beach, Malibu (Leo Carillo, El Matador), Anza-Borrego Desert (Clark Dry Lake Bed, Wind Caves), Julian, Carlsbad

You can see more of Jack’s work at his website, or follow him on Facebook or Instagram

Enjoying EarthSky? Sign up for our free daily newsletter today!



from EarthSky http://ift.tt/1mKZmG1

This gorgeous timelapse was created by our friend Jack Fusco. He calls it Wonder Endlessly. Jack said:

The title is a reflection of the desire to always seek new adventures. There are few things that can match the overwhelming sense of wonder felt when you’re looking up at a sky full of stars. Keeping that strong sense of wonder is what makes me want to head in to the middle of nowhere in the dark, to climb across wet rocks and dodge waves to capture something new. That feeling is something that I hoped to capture with this timelapse.

How did he create it? Jack said:

Hours of scouting and planning went in to each of the 26 different sequences in the video. Some were planned months in advance to coordinate the tide with right moon phase.

Here’s his technical info:

Equipment –
Cameras: Sony A7R2 , Nikon D800E
Lenses: Sigma 24mm f/1.4 ART, Sigma 50mm f/1.4 ART, Nikon 14-24 f/2.8
Motion Control: Rhino EVO & Motion Timelapse slider
Tripod: Feisol CT- 3442
Music: Dan Phillipson – Ascend

Some locations include: La Jolla, Solana Beach, Malibu (Leo Carillo, El Matador), Anza-Borrego Desert (Clark Dry Lake Bed, Wind Caves), Julian, Carlsbad

You can see more of Jack’s work at his website, or follow him on Facebook or Instagram

Enjoying EarthSky? Sign up for our free daily newsletter today!



from EarthSky http://ift.tt/1mKZmG1

128/366: Shiny! [Uncertain Principles]

It seems appropriate to use a power-of-two day for a new digital device, so here’s a photo of my new phone:

My new phone on the wireless charger.

My new phone on the wireless charger.

Getting and setting this up took up much of yesterday. It’s a Droid Turbo, which is basically the Verizon-branded version of the 2015 equivalent of the Moto X I had previously. Yes, I know, Verizon is kind of unpleasant, but I do just enough travel that the better coverage they offer matters to me. And one of the regularly-cited grievances against them, that they don’t push out Android OS updates as often as other carriers, actually verges on a positive feature for me– I really hate it when I get a decent workflow established, and then a software update moves all the buttons around and eliminates or changes features I use all the time.

Anyway, it’s new, it’s shiny, the wi-fi works (one of the reasons I needed a new phone is that the wi-fi crapped out on the old one ages ago, and updates that were big enough that the phone would only download them over wi-fi have been piling up. And I’ve been overrunning my data plan because everything went via that rather than using the home wi-fi network. I’ve had it for less than 24 hours, so I’ve still got a bunch of playing to do to discover new features, but right now, I need to get back to doing useful work.



from ScienceBlogs http://ift.tt/1UBZp1Q

It seems appropriate to use a power-of-two day for a new digital device, so here’s a photo of my new phone:

My new phone on the wireless charger.

My new phone on the wireless charger.

Getting and setting this up took up much of yesterday. It’s a Droid Turbo, which is basically the Verizon-branded version of the 2015 equivalent of the Moto X I had previously. Yes, I know, Verizon is kind of unpleasant, but I do just enough travel that the better coverage they offer matters to me. And one of the regularly-cited grievances against them, that they don’t push out Android OS updates as often as other carriers, actually verges on a positive feature for me– I really hate it when I get a decent workflow established, and then a software update moves all the buttons around and eliminates or changes features I use all the time.

Anyway, it’s new, it’s shiny, the wi-fi works (one of the reasons I needed a new phone is that the wi-fi crapped out on the old one ages ago, and updates that were big enough that the phone would only download them over wi-fi have been piling up. And I’ve been overrunning my data plan because everything went via that rather than using the home wi-fi network. I’ve had it for less than 24 hours, so I’ve still got a bunch of playing to do to discover new features, but right now, I need to get back to doing useful work.



from ScienceBlogs http://ift.tt/1UBZp1Q

What causes the aurora borealis or northern lights?

Photo by Ruslan Merzlyakov. Visit him on Facebook.

Photo by Ruslan Merzlyakov. Visit him on Facebook.

Those who live at or visit high latitudes might at times experience colored lights shimmering across the night sky. Some Inuit believed that the spirits of their ancestors could be seen dancing in the flickering aurora. In Norse mythology, the aurora was a fire bridge to the sky built by the gods. This ethereal display – the aurora borealis or aurora australis, the northern or southern lights – is beautiful. What causes these lights to appear?

Our sun is 93 million miles away. But its effects extend far beyond its visible surface. Great storms on the sun send gusts of charged solar particles hurtling across space. If Earth is in the path of the particle stream, our planet’s magnetic field and atmosphere react.

When the charged particles from the sun strike atoms and molecules in Earth’s atmosphere, they excite those atoms, causing them to light up.

What does it mean for an atom to be excited? Atoms consist of a central nucleus and a surrounding cloud of electrons encircling the nucleus in an orbit. When charged particles from the sun strike atoms in Earth’s atmosphere, electrons move to higher-energy orbits, further away from the nucleus. Then when an electron moves back to a lower-energy orbit, it releases a particle of light or photon.

What happens in an aurora is similar to what happens in the neon lights we see on many business signs. Electricity is used to excite the atoms in the neon gas within the glass tubes of a neon sign. That’s why these signs give off their brilliant colors. The aurora works on the same principle – but at a far more vast scale.

When charged particles from the sun strike air molecules in Earth's magnetic field, they cause those molecules' atoms to become excited. The molecules give off light as they calm down. Image Credit: NASA

The aurora often appears as curtains of lights, but they can also be arcs or spirals, often following lines of force in Earth’s magnetic field. Most are green in color but sometimes you’ll see a hint of pink, and strong displays might also have red, violet and white colors. The lights typically are seen in the far north – the nations bordering the Arctic Ocean – Canada and Alaska, Scandinavian countries, Iceland, Greenland and Russia. But strong displays of the lights can extend down into more southerly latitudes in the United States. And of course, the lights have a counterpart at Earth’s south polar regions.

The colors in the aurora were also a source of mystery throughout human history. But science says that different gases in Earth’s atmosphere give off different colors when they are excited. Oxygen gives off the green color of the aurora, for example. Nitrogen causes blue or red colors.

So today the mystery of the aurora is not so mysterious as it used to be. Yet people still travel thousands of miles to see the brilliant natural light shows in Earth’s atmosphere. And even though we know the scientific reason for the aurora, the dazzling natural light show can still fire our imaginations to visualize fire bridges, gods or dancing ghosts.

Jennifer Khordi captured this aurora last night (September 7) over the Catskills of New York state.

Jennifer Khordi captured this aurora on September 7, 2015 over the Catskills of New York state. Visit Jennifer Khordi on Facebook.

Aurora just west of Saskatoon, by Colin Chatfield. He said,

Aurora just west of Saskatoon, by Colin Chatfield. He said, “We were just about to leave as the Aurora was just a dull band, then it came alive for about an hour or so. This was taken at 2:02am on January 27, 201] … It is not very visible, but I caught Comet Lovejoy at centre left of this photo.”

“This photo was captured a couple of hours ago in Nordreisa, Norway. I was dressed in my very best winter clothes and I can easily admit that I was freezing most of the time anyways, 22 below (-7.6 fahrenheit) kinda has that effect.” January, 2015. © 2015 Tor-Ivar Næss

Aurora in Vesterlålen, Norway, January 2015 by Stig Hansen

Aurora in Vesterlålen, Norway by Stig Hansen

Mike Taylor in Maine caught this photo of last night's aurora. More about Mike and this photo.

Mike Taylor in Maine caught this photo in September, 2014. More about Mike and this photo.

Photo © 2014 Tor-Ivar Næss

Photo © Tor-Ivar Næss

Photo credit: Hallvor Hobbyfotograf Lillebo

Aurora borealis over Norway’s Steinvikholmen Castle by Hallvor Hobbyfotograf Lillebo.View larger. | Photo credit: Hallvor Hobbyfotograf Lillebo

Reisafjorden, Norway bathing in auroras on January 2, 2014. Copyright 2014 Tor-Ivar Næss.

Reisafjorden, Norway bathing in auroras on January 2, 2014. When charged particles from the sun strike atoms in Earth’s atmosphere, they cause electrons in the atoms to move to a higher-energy state. When the electrons drop back to a lower energy state, they release a photon: light. This process creates the beautiful aurora, or northern lights. Image copyright 2014 Tor-Ivar Næss. Via WaitForIt on Facebook.

View larger. | Mike Taylor calls this photo Moonlight Aurora II. He captured it on February 19, 2014.

View larger. | Mike Taylor calls this photo Moonlight Aurora II. He captured it on February 19, 2014. Visit Taylor Photography

View larger. | Aurora over Mount Hood in Oregon as captured by Ben Coffman Photography during the night of May 31-June 1, 2013.

View larger. | Aurora over Mt. Hood in Oregon as captured by Ben Coffman Photography during the night of May 31-June 1, 2013. Visit Ben’s photography page on G+ or visit Ben on Facebook.

Aurora on January 1, 2014 by Geir-Inge Bushmann. See more photos from Geir-Inge Bushmann

Aurora on January 1, 2014 by Geir-Inge Bushmann. The lights typically are seen in the far north – the nations bordering the Arctic Ocean – Canada and Alaska, Scandinavian countries, Iceland, Greenland and Russia. See more photos from Geir-Inge Bushmann

View larger. | Aurora seen by EarthSky Facebook friend Colin Chatfield in Saskatchewan, Canada on May 19, 2012.

View larger. | Spectacular aurora, or northern lights, seen by EarthSky Facebook friend Colin Chatfield in Saskatchewan, Canada on October 24, 2011.

Bottom line: When charged particles from the sun strike atoms in Earth’s atmosphere, they cause electrons in the atoms to move to a higher-energy state. When the electrons drop back to a lower energy state, they release a photon: light. This process creates the beautiful aurora, or northern lights.



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Photo by Ruslan Merzlyakov. Visit him on Facebook.

Photo by Ruslan Merzlyakov. Visit him on Facebook.

Those who live at or visit high latitudes might at times experience colored lights shimmering across the night sky. Some Inuit believed that the spirits of their ancestors could be seen dancing in the flickering aurora. In Norse mythology, the aurora was a fire bridge to the sky built by the gods. This ethereal display – the aurora borealis or aurora australis, the northern or southern lights – is beautiful. What causes these lights to appear?

Our sun is 93 million miles away. But its effects extend far beyond its visible surface. Great storms on the sun send gusts of charged solar particles hurtling across space. If Earth is in the path of the particle stream, our planet’s magnetic field and atmosphere react.

When the charged particles from the sun strike atoms and molecules in Earth’s atmosphere, they excite those atoms, causing them to light up.

What does it mean for an atom to be excited? Atoms consist of a central nucleus and a surrounding cloud of electrons encircling the nucleus in an orbit. When charged particles from the sun strike atoms in Earth’s atmosphere, electrons move to higher-energy orbits, further away from the nucleus. Then when an electron moves back to a lower-energy orbit, it releases a particle of light or photon.

What happens in an aurora is similar to what happens in the neon lights we see on many business signs. Electricity is used to excite the atoms in the neon gas within the glass tubes of a neon sign. That’s why these signs give off their brilliant colors. The aurora works on the same principle – but at a far more vast scale.

When charged particles from the sun strike air molecules in Earth's magnetic field, they cause those molecules' atoms to become excited. The molecules give off light as they calm down. Image Credit: NASA

The aurora often appears as curtains of lights, but they can also be arcs or spirals, often following lines of force in Earth’s magnetic field. Most are green in color but sometimes you’ll see a hint of pink, and strong displays might also have red, violet and white colors. The lights typically are seen in the far north – the nations bordering the Arctic Ocean – Canada and Alaska, Scandinavian countries, Iceland, Greenland and Russia. But strong displays of the lights can extend down into more southerly latitudes in the United States. And of course, the lights have a counterpart at Earth’s south polar regions.

The colors in the aurora were also a source of mystery throughout human history. But science says that different gases in Earth’s atmosphere give off different colors when they are excited. Oxygen gives off the green color of the aurora, for example. Nitrogen causes blue or red colors.

So today the mystery of the aurora is not so mysterious as it used to be. Yet people still travel thousands of miles to see the brilliant natural light shows in Earth’s atmosphere. And even though we know the scientific reason for the aurora, the dazzling natural light show can still fire our imaginations to visualize fire bridges, gods or dancing ghosts.

Jennifer Khordi captured this aurora last night (September 7) over the Catskills of New York state.

Jennifer Khordi captured this aurora on September 7, 2015 over the Catskills of New York state. Visit Jennifer Khordi on Facebook.

Aurora just west of Saskatoon, by Colin Chatfield. He said,

Aurora just west of Saskatoon, by Colin Chatfield. He said, “We were just about to leave as the Aurora was just a dull band, then it came alive for about an hour or so. This was taken at 2:02am on January 27, 201] … It is not very visible, but I caught Comet Lovejoy at centre left of this photo.”

“This photo was captured a couple of hours ago in Nordreisa, Norway. I was dressed in my very best winter clothes and I can easily admit that I was freezing most of the time anyways, 22 below (-7.6 fahrenheit) kinda has that effect.” January, 2015. © 2015 Tor-Ivar Næss

Aurora in Vesterlålen, Norway, January 2015 by Stig Hansen

Aurora in Vesterlålen, Norway by Stig Hansen

Mike Taylor in Maine caught this photo of last night's aurora. More about Mike and this photo.

Mike Taylor in Maine caught this photo in September, 2014. More about Mike and this photo.

Photo © 2014 Tor-Ivar Næss

Photo © Tor-Ivar Næss

Photo credit: Hallvor Hobbyfotograf Lillebo

Aurora borealis over Norway’s Steinvikholmen Castle by Hallvor Hobbyfotograf Lillebo.View larger. | Photo credit: Hallvor Hobbyfotograf Lillebo

Reisafjorden, Norway bathing in auroras on January 2, 2014. Copyright 2014 Tor-Ivar Næss.

Reisafjorden, Norway bathing in auroras on January 2, 2014. When charged particles from the sun strike atoms in Earth’s atmosphere, they cause electrons in the atoms to move to a higher-energy state. When the electrons drop back to a lower energy state, they release a photon: light. This process creates the beautiful aurora, or northern lights. Image copyright 2014 Tor-Ivar Næss. Via WaitForIt on Facebook.

View larger. | Mike Taylor calls this photo Moonlight Aurora II. He captured it on February 19, 2014.

View larger. | Mike Taylor calls this photo Moonlight Aurora II. He captured it on February 19, 2014. Visit Taylor Photography

View larger. | Aurora over Mount Hood in Oregon as captured by Ben Coffman Photography during the night of May 31-June 1, 2013.

View larger. | Aurora over Mt. Hood in Oregon as captured by Ben Coffman Photography during the night of May 31-June 1, 2013. Visit Ben’s photography page on G+ or visit Ben on Facebook.

Aurora on January 1, 2014 by Geir-Inge Bushmann. See more photos from Geir-Inge Bushmann

Aurora on January 1, 2014 by Geir-Inge Bushmann. The lights typically are seen in the far north – the nations bordering the Arctic Ocean – Canada and Alaska, Scandinavian countries, Iceland, Greenland and Russia. See more photos from Geir-Inge Bushmann

View larger. | Aurora seen by EarthSky Facebook friend Colin Chatfield in Saskatchewan, Canada on May 19, 2012.

View larger. | Spectacular aurora, or northern lights, seen by EarthSky Facebook friend Colin Chatfield in Saskatchewan, Canada on October 24, 2011.

Bottom line: When charged particles from the sun strike atoms in Earth’s atmosphere, they cause electrons in the atoms to move to a higher-energy state. When the electrons drop back to a lower energy state, they release a photon: light. This process creates the beautiful aurora, or northern lights.



from EarthSky http://ift.tt/1tDXph8

New alcohol guidelines to help cut cancer risk

alcohol_hero

After much media build-up, Professor Dame Sally Davies, the Government’s Chief Medical Officer, has announced updated guidelines on low-risk drinking for the UK.

Today’s announcement has been in the pipeline since the previous government announced in 2012 it intended to have them reviewed. And over the last year there’s been growing speculation as to just what the new guidelines might look like.

This update is welcome – the guidelines were last reviewed back in 1995 – and thorough, drawing on three different expert groups and multiple reviews of a wide-range of evidence. It aims to prevent a broad range of diseases, as well as injuries and accidents. But it’s also influenced by the considerable evidence that has emerged showing that even low level drinking can increase the risk of some cancers, and that this risk increases the more alcohol people drink.

The changes are also down to a weakening of the evidence that there are health benefits to drinking alcohol – so the new version is about minimising harms, rather than considering them in addition to benefits.

So what’s changed?  What do the new recommendations mean for you? And how has the evidence changed since the last update? We’ll discuss this below. But first, one thing that hasn’t changed is that the guideline amount is measured in ‘units’ of alcohol. And you aren’t alone in wondering…

…what on earth is a ‘unit’ of alcohol?

One unit is defined as 10ml (or 8g) of pure alcohol. But that probably hasn’t helped you know how many you’re drinking.

The difficulty with communicating about alcohol consumption is that it’s very difficult for people to measure and track what they’re drinking. Chiefly this is because people (thankfully) don’t drink pure alcohol, and different drinks contain different concentrations of alcohol (hence ‘ABV – alcohol by volume – the % figure on many drinks which is the proportion of pure alcohol it contains).

And that’s before you factor in pub measures versus what people might pour themselves at home.

So using units is a way of trying to standardise advice on alcohol. But it’s far from ideal, and there’s lots of evidence (e.g. this study) that people struggle to understand what units mean, and that they aren’t the same as ‘drinks’. The committee that drew up the guidelines was aware of these limitations, but despite searching for a different solution, they say “If there is a better alternative to the UK unit, we have yet to hear of it.”

As the graphic below shows, almost any drink you might order at the bar contains more than one unit:

What’s new? And what’s changed?

The main change is that the recommendation for men and women is now the same – to keep health risks to a minimum, people should drink no more than 14 units of alcohol a week. This is because the evidence now suggests men’s and women’s risks from drinking a given amount of alcohol are about the same – although  men have a higher risk than women of immediate harms such as accidents and injuries, and women’s risk of long term illness (and premature death) is higher.

And the focus has switched back to weekly, rather than daily, limits. The previous (1995) guidelines introduced daily limits. And while these didn’t entirely replace the weekly recommendations, confusingly the two didn’t match up – people drinking up to the maximum every day would exceed the weekly limit by 7 units.

The daily limits have come in for other criticisms too – for example research published this summer, found that people who don’t drink every day (which is the majority of the population) tended to ignore the guidelines, because the advice didn’t seem relevant to them. The move away from daily limits has partly been motivated by research like this on how people understand and use guidelines.

And as we said above, the new guidelines also largely do away with the notion that alcohol is beneficial for our health.

The committee also wanted to help people reduce the risks from drinking large amounts on one occasion, and they’ve addressed this in a number of ways. Firstly, the weekly guidance also says if people drink as much as 14 units in a week, they should spread it out evenly over at least 3 days, cautioning that heavy drinking sessions increase the risk of accidents and injuries as well as long-term illnesses. As well as suggesting people limit the amount they drink in one session, there is also advice for people to help cut the immediate risks – such as drinking more slowly.

And it also suggests people have drink-free days to help cut down on the amount they drink.

The way the guidelines are now presented also makes it clear that 14 units per week is a limit, not a target. And they highlight that the risk for some diseases, such as mouth, throat and breast cancers, is increased at any level of regular drinking – so the guidelines don’t represent an absolutely safe amount to drink; they’re intended to keep a person’s health risks from alcohol to a minimum.

Finally, the committee has decided on a minimum risk level in context of other risks we expose ourselves to. So the 14 unit limit is the level of drinking that would be expected to lead to a lifetime risk of dying from an alcohol-related condition which is similar to the harms of other routine activities, such as driving a car (to be precise, about one per cent).

Cancer and the new guidelines

So that’s the new guidelines, and units, explained. But as we said above, one reason for these changes is the strengthening evidence of the link between alcohol and cancer.  So what’s changed here?

We’ve blogged about alcohol and cancer many times – especially the link with breast cancer – but here’s a quick recap.

It’s been established for decades that alcohol can cause cancer, but the impact that lighter drinking has on risk has taken longer to tease apart. That’s because the effect on risk is smaller, more difficult for scientists to demonstrate  conclusively, and also prove it’s not down to other things (such as smoking or poor diet) muddying the waters.

But more recently, it’s become clear that low level drinking (meaning around a drink a day on average) increases the risk of breast, mouth, throat and oesophageal cancers. And the more you drink, the higher the risk of these and other cancers. Altogether, alcohol is linked to seven types of cancer with bowel, liver and laryngeal cancers making up the total.

The extra risk for drinking at low levels is fairly small, so it probably won’t make much difference to an individual’s absolute risk of developing cancer – but over a population the size of the UK, where many people drink at low levels, it adds up to a big impact.

To try to show how even light drinking can increase the risk of cancer, and how the risk rises with heavier drinking, we’ve done some calculations using the latest evidence on how different levels of drinking affect the risk of mouth cancer:

These figures are worked out using the same method as we’ve previously used for breast cancer and alcohol drinking – but show the risk for mouth cancer which affects both men and women. There’s more detail about how we calculated them below*.

What next?

These updated guidelines are welcome – but by themselves they’re not going to solve the UK’s problems with alcohol and health.  The amount we drink in the UK is almost double what it was in 1960, so it’s also vital that the government invests in national health campaigns to provide people with clear information about the health risks of drinking alcohol, particularly at levels above these new guidelines.

But even if people know and understand the risks, they need to be in an environment that supports them to make changes. So as well as clear guidelines and public campaigns, we also want to see the government introduce measures to tackle the price, promotion and availability of alcohol, such as minimum unit pricing, as outlined in the independent alcohol strategy Health First.

What can I do?

These guidelines are an important step in helping people understand – and reduce – the risks from drinking alcohol. When it comes to cancer, our advice hasn’t changed – the less alcohol you drink, the lower your risk.

There are lots of simple ways to start cutting down. For many people, simply tracking how much you drink can be an eye opener – there are lots of free apps and tools available, such as this one from Change4Life.

Some quick ways to cut out units are to choose lower strength beers and wines, opt for smaller servings – or you could try a shandy or spritzer. Or just replace every other alcoholic drink with a soft drink on a night out.

And if you’re drinking in a group, staying out of large rounds means you don’t have to match anyone else’s pace, and you can more easily avoid being cajoled into having a drink that you didn’t really want.

And there’s something else you can do too – the CMO has also announced a public consultation to check that the guidelines are clear, easy to understand and, perhaps most importantly, useful. And they’d like you to take part.

Everyone has their own priorities and their own approach to risk, but along with the CMO we believe people have a right to clear information to help them make decisions about their lives. We hope these new guidelines will help people understand and manage the risks of drinking alcohol.

– Sarah

*Footnote: how we calculated the mouth cancer risk stats

We’ve started off by estimating the underlying risk of a non-drinker in the UK being diagnosed with mouth cancer – we have to estimate this because risk of being diagnosed with mouth cancer at some stage in your life (1 in 84 for men, 1 in 157 for women) includes the whole population – from tee-totallers to very heavy drinkers. Because mouth cancer risk rises with alcohol drinking, we can assume the lifetime risk for non-drinkers is lower than these population averages.

Using these estimated risks for non-drinkers, we’ve then modelled the impact of drinking at different levels using risks for men and women from a recent review of the evidence. Of course these figures are estimates – but they give a good indication of the impact of alcohol drinking at a population level.

And why the funny numbers of units?  Research, including the paper our calculations are based on, often uses grams of alcohol per day as a standard measure of drinking. The amounts in the paper we’ve based our calculations on translate to 12, 25 and 50 grams of alcohol per day, which look like a much more sensible set of numbers to pick, but we wanted to present this in units to match with the guidelines. The drinking levels we’ve picked represent people drinking within the guidelines, at around the previous weekly limit for men, and well above the recommended limits.



from Cancer Research UK - Science blog http://ift.tt/1Za96Wz
alcohol_hero

After much media build-up, Professor Dame Sally Davies, the Government’s Chief Medical Officer, has announced updated guidelines on low-risk drinking for the UK.

Today’s announcement has been in the pipeline since the previous government announced in 2012 it intended to have them reviewed. And over the last year there’s been growing speculation as to just what the new guidelines might look like.

This update is welcome – the guidelines were last reviewed back in 1995 – and thorough, drawing on three different expert groups and multiple reviews of a wide-range of evidence. It aims to prevent a broad range of diseases, as well as injuries and accidents. But it’s also influenced by the considerable evidence that has emerged showing that even low level drinking can increase the risk of some cancers, and that this risk increases the more alcohol people drink.

The changes are also down to a weakening of the evidence that there are health benefits to drinking alcohol – so the new version is about minimising harms, rather than considering them in addition to benefits.

So what’s changed?  What do the new recommendations mean for you? And how has the evidence changed since the last update? We’ll discuss this below. But first, one thing that hasn’t changed is that the guideline amount is measured in ‘units’ of alcohol. And you aren’t alone in wondering…

…what on earth is a ‘unit’ of alcohol?

One unit is defined as 10ml (or 8g) of pure alcohol. But that probably hasn’t helped you know how many you’re drinking.

The difficulty with communicating about alcohol consumption is that it’s very difficult for people to measure and track what they’re drinking. Chiefly this is because people (thankfully) don’t drink pure alcohol, and different drinks contain different concentrations of alcohol (hence ‘ABV – alcohol by volume – the % figure on many drinks which is the proportion of pure alcohol it contains).

And that’s before you factor in pub measures versus what people might pour themselves at home.

So using units is a way of trying to standardise advice on alcohol. But it’s far from ideal, and there’s lots of evidence (e.g. this study) that people struggle to understand what units mean, and that they aren’t the same as ‘drinks’. The committee that drew up the guidelines was aware of these limitations, but despite searching for a different solution, they say “If there is a better alternative to the UK unit, we have yet to hear of it.”

As the graphic below shows, almost any drink you might order at the bar contains more than one unit:

What’s new? And what’s changed?

The main change is that the recommendation for men and women is now the same – to keep health risks to a minimum, people should drink no more than 14 units of alcohol a week. This is because the evidence now suggests men’s and women’s risks from drinking a given amount of alcohol are about the same – although  men have a higher risk than women of immediate harms such as accidents and injuries, and women’s risk of long term illness (and premature death) is higher.

And the focus has switched back to weekly, rather than daily, limits. The previous (1995) guidelines introduced daily limits. And while these didn’t entirely replace the weekly recommendations, confusingly the two didn’t match up – people drinking up to the maximum every day would exceed the weekly limit by 7 units.

The daily limits have come in for other criticisms too – for example research published this summer, found that people who don’t drink every day (which is the majority of the population) tended to ignore the guidelines, because the advice didn’t seem relevant to them. The move away from daily limits has partly been motivated by research like this on how people understand and use guidelines.

And as we said above, the new guidelines also largely do away with the notion that alcohol is beneficial for our health.

The committee also wanted to help people reduce the risks from drinking large amounts on one occasion, and they’ve addressed this in a number of ways. Firstly, the weekly guidance also says if people drink as much as 14 units in a week, they should spread it out evenly over at least 3 days, cautioning that heavy drinking sessions increase the risk of accidents and injuries as well as long-term illnesses. As well as suggesting people limit the amount they drink in one session, there is also advice for people to help cut the immediate risks – such as drinking more slowly.

And it also suggests people have drink-free days to help cut down on the amount they drink.

The way the guidelines are now presented also makes it clear that 14 units per week is a limit, not a target. And they highlight that the risk for some diseases, such as mouth, throat and breast cancers, is increased at any level of regular drinking – so the guidelines don’t represent an absolutely safe amount to drink; they’re intended to keep a person’s health risks from alcohol to a minimum.

Finally, the committee has decided on a minimum risk level in context of other risks we expose ourselves to. So the 14 unit limit is the level of drinking that would be expected to lead to a lifetime risk of dying from an alcohol-related condition which is similar to the harms of other routine activities, such as driving a car (to be precise, about one per cent).

Cancer and the new guidelines

So that’s the new guidelines, and units, explained. But as we said above, one reason for these changes is the strengthening evidence of the link between alcohol and cancer.  So what’s changed here?

We’ve blogged about alcohol and cancer many times – especially the link with breast cancer – but here’s a quick recap.

It’s been established for decades that alcohol can cause cancer, but the impact that lighter drinking has on risk has taken longer to tease apart. That’s because the effect on risk is smaller, more difficult for scientists to demonstrate  conclusively, and also prove it’s not down to other things (such as smoking or poor diet) muddying the waters.

But more recently, it’s become clear that low level drinking (meaning around a drink a day on average) increases the risk of breast, mouth, throat and oesophageal cancers. And the more you drink, the higher the risk of these and other cancers. Altogether, alcohol is linked to seven types of cancer with bowel, liver and laryngeal cancers making up the total.

The extra risk for drinking at low levels is fairly small, so it probably won’t make much difference to an individual’s absolute risk of developing cancer – but over a population the size of the UK, where many people drink at low levels, it adds up to a big impact.

To try to show how even light drinking can increase the risk of cancer, and how the risk rises with heavier drinking, we’ve done some calculations using the latest evidence on how different levels of drinking affect the risk of mouth cancer:

These figures are worked out using the same method as we’ve previously used for breast cancer and alcohol drinking – but show the risk for mouth cancer which affects both men and women. There’s more detail about how we calculated them below*.

What next?

These updated guidelines are welcome – but by themselves they’re not going to solve the UK’s problems with alcohol and health.  The amount we drink in the UK is almost double what it was in 1960, so it’s also vital that the government invests in national health campaigns to provide people with clear information about the health risks of drinking alcohol, particularly at levels above these new guidelines.

But even if people know and understand the risks, they need to be in an environment that supports them to make changes. So as well as clear guidelines and public campaigns, we also want to see the government introduce measures to tackle the price, promotion and availability of alcohol, such as minimum unit pricing, as outlined in the independent alcohol strategy Health First.

What can I do?

These guidelines are an important step in helping people understand – and reduce – the risks from drinking alcohol. When it comes to cancer, our advice hasn’t changed – the less alcohol you drink, the lower your risk.

There are lots of simple ways to start cutting down. For many people, simply tracking how much you drink can be an eye opener – there are lots of free apps and tools available, such as this one from Change4Life.

Some quick ways to cut out units are to choose lower strength beers and wines, opt for smaller servings – or you could try a shandy or spritzer. Or just replace every other alcoholic drink with a soft drink on a night out.

And if you’re drinking in a group, staying out of large rounds means you don’t have to match anyone else’s pace, and you can more easily avoid being cajoled into having a drink that you didn’t really want.

And there’s something else you can do too – the CMO has also announced a public consultation to check that the guidelines are clear, easy to understand and, perhaps most importantly, useful. And they’d like you to take part.

Everyone has their own priorities and their own approach to risk, but along with the CMO we believe people have a right to clear information to help them make decisions about their lives. We hope these new guidelines will help people understand and manage the risks of drinking alcohol.

– Sarah

*Footnote: how we calculated the mouth cancer risk stats

We’ve started off by estimating the underlying risk of a non-drinker in the UK being diagnosed with mouth cancer – we have to estimate this because risk of being diagnosed with mouth cancer at some stage in your life (1 in 84 for men, 1 in 157 for women) includes the whole population – from tee-totallers to very heavy drinkers. Because mouth cancer risk rises with alcohol drinking, we can assume the lifetime risk for non-drinkers is lower than these population averages.

Using these estimated risks for non-drinkers, we’ve then modelled the impact of drinking at different levels using risks for men and women from a recent review of the evidence. Of course these figures are estimates – but they give a good indication of the impact of alcohol drinking at a population level.

And why the funny numbers of units?  Research, including the paper our calculations are based on, often uses grams of alcohol per day as a standard measure of drinking. The amounts in the paper we’ve based our calculations on translate to 12, 25 and 50 grams of alcohol per day, which look like a much more sensible set of numbers to pick, but we wanted to present this in units to match with the guidelines. The drinking levels we’ve picked represent people drinking within the guidelines, at around the previous weekly limit for men, and well above the recommended limits.



from Cancer Research UK - Science blog http://ift.tt/1Za96Wz

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