aads

Moyhu: climate feedbacks and circuits [Stoat]

There’s a vair nice post at Moyhu called climate feedbacks and circuits.

I think it is particaulrly nice that someone competent has finally taken and shaken the gibberish about feedbacks that the EE’s fling about so thoughtlessly and actually made some sense of it.



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There’s a vair nice post at Moyhu called climate feedbacks and circuits.

I think it is particaulrly nice that someone competent has finally taken and shaken the gibberish about feedbacks that the EE’s fling about so thoughtlessly and actually made some sense of it.



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EPA and the new TSCA – Stakeholders push agency in divergent directions   [The Pump Handle]

As the U.S Environmental Protection Agency (EPA) begins work under the Lautenberg Chemical Safety Act for the 21st Century (LCSA) – the updated Toxic Substances Control Act – more striking divisions are emerging between what environmental health advocates and what chemical manufacturing and industry groups want from the law.

These go beyond what was voiced during the public meetings the EPA held in early August to gather input on the rules it will use to prioritize chemicals for review and evaluate those chemicals’ risks. A look at the written comments now submitted to the agency underscores how important these decisions will be. Depending on what the EPA decides, the LCSA could either usher in a new era of public health protections – or it could reinforce and perhaps further entrench the status quo.

Altogether, more than 100 written comments have now been submitted to the EPA on both rules. In raw number of comments submitted, the industrial interest groups and environmental health advocates are currently nearly equally divided. [This could change as more comments are posted to the EPA online docket for the risk evaluation rule.] There are very few comments from apparently unaffiliated citizens, all submitted anonymously. But this is where the parity ends.

Will EPA limit or expand how exposures are considered?

Among the most striking differences between environmental health advocates and industry groups is how they would like EPA to assess chemical exposures. The American Academy of Pediatrics weighed in on the information needed to adequately protect children, reminding the EPA that “Children are not little adults.” In comments to which more than three dozen environmental, health and labor advocacy groups signed on, the EPA was urged to protect fence-line communities. In its comments, Alaska Community Action on Toxics highlighted the importance of how EPA will consider Arctic and other disproportionately exposed communities.

Meanwhile, various industry groups, including the Consumer Specialty Product Association (CSPA) expressed concern about a broad interpretation of the law’s direction to specially consider those who may be most vulnerable to chemical exposures. In its comments, the CSPA asks the EPA to clarify what the law’s means by describing these groups “potentially exposed” and how that differs from “an actual exposure.” Similarly, the International Fragrance Association North America asked that EPA find “some reasonable potential for greater risk” when considering susceptible populations, rather than simply considering those who are more exposed than others. This slicing and dicing could create obstacles for the EPA’s consideration of communities with heavy toxic exposures if it means having to prove individuals’ personal risk factors and specific exposure levels – rather than looking at a community as a whole.

Another point of divergence concerns the scope of the science that stakeholders want the agency to use in prioritizing and evaluating chemicals. The balance of industry and academic science appears to be shaping up as an area of contention, as noted in comments from the Endocrine Society. So does the potential confidentiality of information industry submits to EPA. The American Chemistry Council wants to EPA to explain how it will “protect confidential information during the prioritization process.”

Yet another is various industry groups’ focus on individual chemicals they would like to see designated low priority. This contrasts with the request from numerous environmental health advocates that EPA evaluate groups of similar chemicals together to avoid the single chemical approach that has facilitated so-called “regrettable substitutions” – as has happened with flame retardants.

How will EPA consider highly hazardous chemicals used in manufacturing?

For example, when it comes to worker exposure, the Vinyl Institute has written to the EPA explaining that the primary chemicals used to make vinyl – ethylene chloride, a neurotoxin and potential carcinogen and vinyl chloride monomer, a known human carcinogen – “should be considered as industrial intermediates, with little to no widespread public exposure.” The implication is that given existing regulation of these substances, these chemicals shouldn’t rise to the level of high priority under the Lautenberg Act.

On the other hand, the University of Massachusetts Lowell’s Toxic Use Reduction Institute (TURI) in its comments says:

“In considering chemical intermediates, it is important to consider the potential for occupational or public exposure during accidents or process malfunctions. Experience has shown that it is important not to assume an absence of exposure potential. For example, methyl isocyanate, a source of severe toxic exposures in the Bhopal disaster, is used as a chemical intermediate for the production of carbamate insecticides and herbicides.”

And the AFL-CIO points out that workers

“often are exposed to chemicals earlier in the supply chain” and are “are known for experiencing sentinel exposures because they often are the first to be exposed to a chemical, to higher levels of a chemical and throughout the duration of their working lives.”

The EPA, wrote the union, must

“consider occupational factors that make working populations susceptible to toxicity” throughout its chemical prioritization and evaluation process, “not simply consider occupational uses after chemicals are selected based only on non-occupational factors.”

Occupational diseases caused by chemical exposures, notes the AFL-CIO, “are responsible for more than 50,000 deaths and 190,000 illnesses each year.”

The public will have another chance to weigh in after the EPA releases these proposed rules, which Congress directed EPA to issue by mid-December.

 

 



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As the U.S Environmental Protection Agency (EPA) begins work under the Lautenberg Chemical Safety Act for the 21st Century (LCSA) – the updated Toxic Substances Control Act – more striking divisions are emerging between what environmental health advocates and what chemical manufacturing and industry groups want from the law.

These go beyond what was voiced during the public meetings the EPA held in early August to gather input on the rules it will use to prioritize chemicals for review and evaluate those chemicals’ risks. A look at the written comments now submitted to the agency underscores how important these decisions will be. Depending on what the EPA decides, the LCSA could either usher in a new era of public health protections – or it could reinforce and perhaps further entrench the status quo.

Altogether, more than 100 written comments have now been submitted to the EPA on both rules. In raw number of comments submitted, the industrial interest groups and environmental health advocates are currently nearly equally divided. [This could change as more comments are posted to the EPA online docket for the risk evaluation rule.] There are very few comments from apparently unaffiliated citizens, all submitted anonymously. But this is where the parity ends.

Will EPA limit or expand how exposures are considered?

Among the most striking differences between environmental health advocates and industry groups is how they would like EPA to assess chemical exposures. The American Academy of Pediatrics weighed in on the information needed to adequately protect children, reminding the EPA that “Children are not little adults.” In comments to which more than three dozen environmental, health and labor advocacy groups signed on, the EPA was urged to protect fence-line communities. In its comments, Alaska Community Action on Toxics highlighted the importance of how EPA will consider Arctic and other disproportionately exposed communities.

Meanwhile, various industry groups, including the Consumer Specialty Product Association (CSPA) expressed concern about a broad interpretation of the law’s direction to specially consider those who may be most vulnerable to chemical exposures. In its comments, the CSPA asks the EPA to clarify what the law’s means by describing these groups “potentially exposed” and how that differs from “an actual exposure.” Similarly, the International Fragrance Association North America asked that EPA find “some reasonable potential for greater risk” when considering susceptible populations, rather than simply considering those who are more exposed than others. This slicing and dicing could create obstacles for the EPA’s consideration of communities with heavy toxic exposures if it means having to prove individuals’ personal risk factors and specific exposure levels – rather than looking at a community as a whole.

Another point of divergence concerns the scope of the science that stakeholders want the agency to use in prioritizing and evaluating chemicals. The balance of industry and academic science appears to be shaping up as an area of contention, as noted in comments from the Endocrine Society. So does the potential confidentiality of information industry submits to EPA. The American Chemistry Council wants to EPA to explain how it will “protect confidential information during the prioritization process.”

Yet another is various industry groups’ focus on individual chemicals they would like to see designated low priority. This contrasts with the request from numerous environmental health advocates that EPA evaluate groups of similar chemicals together to avoid the single chemical approach that has facilitated so-called “regrettable substitutions” – as has happened with flame retardants.

How will EPA consider highly hazardous chemicals used in manufacturing?

For example, when it comes to worker exposure, the Vinyl Institute has written to the EPA explaining that the primary chemicals used to make vinyl – ethylene chloride, a neurotoxin and potential carcinogen and vinyl chloride monomer, a known human carcinogen – “should be considered as industrial intermediates, with little to no widespread public exposure.” The implication is that given existing regulation of these substances, these chemicals shouldn’t rise to the level of high priority under the Lautenberg Act.

On the other hand, the University of Massachusetts Lowell’s Toxic Use Reduction Institute (TURI) in its comments says:

“In considering chemical intermediates, it is important to consider the potential for occupational or public exposure during accidents or process malfunctions. Experience has shown that it is important not to assume an absence of exposure potential. For example, methyl isocyanate, a source of severe toxic exposures in the Bhopal disaster, is used as a chemical intermediate for the production of carbamate insecticides and herbicides.”

And the AFL-CIO points out that workers

“often are exposed to chemicals earlier in the supply chain” and are “are known for experiencing sentinel exposures because they often are the first to be exposed to a chemical, to higher levels of a chemical and throughout the duration of their working lives.”

The EPA, wrote the union, must

“consider occupational factors that make working populations susceptible to toxicity” throughout its chemical prioritization and evaluation process, “not simply consider occupational uses after chemicals are selected based only on non-occupational factors.”

Occupational diseases caused by chemical exposures, notes the AFL-CIO, “are responsible for more than 50,000 deaths and 190,000 illnesses each year.”

The public will have another chance to weigh in after the EPA releases these proposed rules, which Congress directed EPA to issue by mid-December.

 

 



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Watch spacewalk live September 1

NASA astronaut Barry Wilmore works outside the International Space Station on the first of three spacewalks preparing the station for future arrivals by U.S. commercial crew spacecraft, Saturday, February 21, 2015. Fellow spacewalker Terry Virts, seen reflected in the visor, shared this photograph on social media. View larger. \ Image credit; NASA

NASA astronaut Barry Wilmore outside the International Space Station during February 2015 spacewalk. Fellow spacewalker Terry Virts, seen reflected in the visor, shared this photograph on social media. Image via NASA

On Thursday, September 1, 2016, two NASA astronauts – Jeff Williams and Kate Rubins – will spacewalk outside the International Space Station (ISS) for the second time in less than two weeks. NASA TV will provide complete coverage beginning at 6:30 a.m. EDT (1030 UTC). The spacewalk is scheduled to begin about 8 a.m. EDT (1200 UTC) and last six and half hours. Translate to your timezone.

Watch here.

Here is what the astronauts will be doing during the spacewalk, according to a NASA statement:

Working on the port side of the orbiting complex’s backbone, or truss, Expedition 48 Commander Jeff Williams and Flight Engineer Kate Rubins of NASA will retract a thermal radiator that is part of the station’s cooling system. The radiator is a backup that had been deployed previously as part of an effort to fix an ammonia coolant leak. They’ll also tighten struts on a solar array joint, and install the first of several enhanced high-definition television cameras that will be used to monitor activities outside the station, including the comings and goings of visiting cargo and crew vehicles.

The Thursday spacewalk will be the fifth of Williams’ career and the second for Rubins. Williams will be designated as extravehicular crew member 1 (EV1), wearing a spacesuit with a red stripe. Rubins will be EV2, wearing a suit with no stripes.

Bottom line: Two ISS astronauts will perform a 6.5 hour spacewalk beginning at about 8:00 a.m. ET (12:00 UTC) Thursday, September 1, 2016. NASA TV will broadcast live coverage.

Read more from NASA



from EarthSky http://ift.tt/2bJGG6b
NASA astronaut Barry Wilmore works outside the International Space Station on the first of three spacewalks preparing the station for future arrivals by U.S. commercial crew spacecraft, Saturday, February 21, 2015. Fellow spacewalker Terry Virts, seen reflected in the visor, shared this photograph on social media. View larger. \ Image credit; NASA

NASA astronaut Barry Wilmore outside the International Space Station during February 2015 spacewalk. Fellow spacewalker Terry Virts, seen reflected in the visor, shared this photograph on social media. Image via NASA

On Thursday, September 1, 2016, two NASA astronauts – Jeff Williams and Kate Rubins – will spacewalk outside the International Space Station (ISS) for the second time in less than two weeks. NASA TV will provide complete coverage beginning at 6:30 a.m. EDT (1030 UTC). The spacewalk is scheduled to begin about 8 a.m. EDT (1200 UTC) and last six and half hours. Translate to your timezone.

Watch here.

Here is what the astronauts will be doing during the spacewalk, according to a NASA statement:

Working on the port side of the orbiting complex’s backbone, or truss, Expedition 48 Commander Jeff Williams and Flight Engineer Kate Rubins of NASA will retract a thermal radiator that is part of the station’s cooling system. The radiator is a backup that had been deployed previously as part of an effort to fix an ammonia coolant leak. They’ll also tighten struts on a solar array joint, and install the first of several enhanced high-definition television cameras that will be used to monitor activities outside the station, including the comings and goings of visiting cargo and crew vehicles.

The Thursday spacewalk will be the fifth of Williams’ career and the second for Rubins. Williams will be designated as extravehicular crew member 1 (EV1), wearing a spacesuit with a red stripe. Rubins will be EV2, wearing a suit with no stripes.

Bottom line: Two ISS astronauts will perform a 6.5 hour spacewalk beginning at about 8:00 a.m. ET (12:00 UTC) Thursday, September 1, 2016. NASA TV will broadcast live coverage.

Read more from NASA



from EarthSky http://ift.tt/2bJGG6b

A closer look at climate change. And denial. LOL. [Greg Laden's Blog]

Seth Myers:



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Seth Myers:



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Cancer resistance developing in Tasmanian devils [Life Lines]

Physics Blogging Round-Up: Fast Cars and Spherical Cows [Uncertain Principles]

It’s been a while since the last Forbes links dump, but since it’s the last day of the month, I figure I might as well sum up a bit. Only two posts, but they have a connection that I’ll expound on a bit to make up for the lack of material…

Can A Tesla Model S Really Accelerate Faster Than Gravity?: I got pointed to a story about the 0-60mph time for a Tesla, and said “That seems fishy…” After climbing back out of the Google rabbit hole, I tried to explain why that seemed unlikely to me, and the funny timing thing that might explain the result.

The Hardest Thing To Grasp In Physics? Thinking Like A Physicist: Some musings about how the trickiest part of learning to be a physicist is getting the mindset, particularly the highly reductionist use of “spherical cow” sorts of approximations.

So, the first of these really pissed off a lot of Car Guys, who left tons of comments, and some angry emails and tweets, pointing to a variety of other cars that supposedly accelerate at large multiples of the acceleration of gravity. I wasn’t especially moved by most of this, in part because they’re not particularly relevant to the question of whether the Tesla result is surprising. It’s true that I didn’t discuss the possibility of aerodynamic down forces that would allow for a larger frictional force, but those aren’t actually important for a normal-ish car like a Tesla. A top fuel dragster is a completely different animal, and I’m not especially surprised that they work differently than an ordinary car.

The other issue I have with the angry reaction is that it really misses the point of the post (which, admittedly, I probably should’ve made more explicit). That is, I don’t actually care whether the Tesla accelerates at 0.98g or 1.1g. My purpose in writing that piece, like most of what I write, really had more to do with the physics mindset than the specific numerical values. I was explaining my reaction and reasoning: when I read the original piece, I was immediately skeptical for reasons that have to do with physics, which sent me off looking for more information that might explain the faster-than-expected time in a way that didn’t require surprising physics, and learned about a timing thing that’s in the right ballpark to account for the apparent discrepancy.

I thought that was an interesting process (obviously, or I wouldn’t’ve been sucked into Googling stuff about car testing), and worth laying out. I’m really not remotely invested in the specific numerical results– if the tires they use turn out to be much stickier than the usual run of things so the acceleration is a little higher than I would expect, well, that’s a nice bit of trivia. It doesn’t really change my thinking about why that was a piece worth writing, which is largely that it illustrates the toy-model-building described in the second post. Thinking like a physicist means that the 0-60mph time isn’t just a random factoid that could take on absolutely any value, it’s something with a physical origin that you can model in a simple way, which leads to an expectation about what the time should be for a relatively ordinary car. And thinking “that’s funny…” does, in fact, lead to something that’s a little funny in the timing, which is also interesting.

But, yeah, I should’ve made that clearer, because, wow, are there people who are deeply invested in the accuracy of those numbers…

Anyway, that’s the story of my recent blogging. Which may become sparse for the next several months, as I’ve gotten myself stuck on a grand jury that sits two days a week, and classes start next Wednesday, so my time is going to be very tight for the immediate future.



from ScienceBlogs http://ift.tt/2bR9vMS

It’s been a while since the last Forbes links dump, but since it’s the last day of the month, I figure I might as well sum up a bit. Only two posts, but they have a connection that I’ll expound on a bit to make up for the lack of material…

Can A Tesla Model S Really Accelerate Faster Than Gravity?: I got pointed to a story about the 0-60mph time for a Tesla, and said “That seems fishy…” After climbing back out of the Google rabbit hole, I tried to explain why that seemed unlikely to me, and the funny timing thing that might explain the result.

The Hardest Thing To Grasp In Physics? Thinking Like A Physicist: Some musings about how the trickiest part of learning to be a physicist is getting the mindset, particularly the highly reductionist use of “spherical cow” sorts of approximations.

So, the first of these really pissed off a lot of Car Guys, who left tons of comments, and some angry emails and tweets, pointing to a variety of other cars that supposedly accelerate at large multiples of the acceleration of gravity. I wasn’t especially moved by most of this, in part because they’re not particularly relevant to the question of whether the Tesla result is surprising. It’s true that I didn’t discuss the possibility of aerodynamic down forces that would allow for a larger frictional force, but those aren’t actually important for a normal-ish car like a Tesla. A top fuel dragster is a completely different animal, and I’m not especially surprised that they work differently than an ordinary car.

The other issue I have with the angry reaction is that it really misses the point of the post (which, admittedly, I probably should’ve made more explicit). That is, I don’t actually care whether the Tesla accelerates at 0.98g or 1.1g. My purpose in writing that piece, like most of what I write, really had more to do with the physics mindset than the specific numerical values. I was explaining my reaction and reasoning: when I read the original piece, I was immediately skeptical for reasons that have to do with physics, which sent me off looking for more information that might explain the faster-than-expected time in a way that didn’t require surprising physics, and learned about a timing thing that’s in the right ballpark to account for the apparent discrepancy.

I thought that was an interesting process (obviously, or I wouldn’t’ve been sucked into Googling stuff about car testing), and worth laying out. I’m really not remotely invested in the specific numerical results– if the tires they use turn out to be much stickier than the usual run of things so the acceleration is a little higher than I would expect, well, that’s a nice bit of trivia. It doesn’t really change my thinking about why that was a piece worth writing, which is largely that it illustrates the toy-model-building described in the second post. Thinking like a physicist means that the 0-60mph time isn’t just a random factoid that could take on absolutely any value, it’s something with a physical origin that you can model in a simple way, which leads to an expectation about what the time should be for a relatively ordinary car. And thinking “that’s funny…” does, in fact, lead to something that’s a little funny in the timing, which is also interesting.

But, yeah, I should’ve made that clearer, because, wow, are there people who are deeply invested in the accuracy of those numbers…

Anyway, that’s the story of my recent blogging. Which may become sparse for the next several months, as I’ve gotten myself stuck on a grand jury that sits two days a week, and classes start next Wednesday, so my time is going to be very tight for the immediate future.



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A Young, Dusty, Disk-Bearing Star Debunks ‘Alien Megastructures’ Theory (Synopsis) [Starts With A Bang]

“Otherwise we are trying to communicate with someone who doesn’t exist with a system which doesn’t work.” -Philip K. Dick

When it comes to the now famous “Alien Megastructures” star, the observations didn’t add up. There were huge, irregular flux dips, but not a hint of infrared radiation that would indicate a circumstellar disk. Infrared radiation was the marker for a whole slew of indicators — planetary collision debris, warped, thick disks, cometary swarms — that could be the cause of such spectacular dips.

Image credit: Tabby Boyajian and her team of PlanetHunters, via http://ift.tt/1Pjgrmk.

Image credit: Tabby Boyajian and her team of PlanetHunters, via http://ift.tt/1Pjgrmk.

Yet there are increasingly more and more stars that show these huge, irregular flux dips, and they all have a few things in common. They’re all young stars, they all emit infrared radiation, they all have circumstellar disks and they all show a variety of disk orientations with respect to our line-of-sight. Is it possible, just as we can’t see Saturn’s rings when they’re edge-on, that this mysterious star’s disk is edge-on, and that’s why we can’t see its infrared flux?

Artist’s conception of the extrasolar ring system circling the young giant planet or brown dwarf J1407b. Image credit: Ron Miller.

Artist’s conception of the extrasolar ring system circling the young giant planet or brown dwarf J1407b. Image credit: Ron Miller.

Go get the whole story on why alien megastructures are out, and a circumstellar disk, with either a warped inner disk or eccentric, cometary-like debris, is in!



from ScienceBlogs http://ift.tt/2c8zEHr

“Otherwise we are trying to communicate with someone who doesn’t exist with a system which doesn’t work.” -Philip K. Dick

When it comes to the now famous “Alien Megastructures” star, the observations didn’t add up. There were huge, irregular flux dips, but not a hint of infrared radiation that would indicate a circumstellar disk. Infrared radiation was the marker for a whole slew of indicators — planetary collision debris, warped, thick disks, cometary swarms — that could be the cause of such spectacular dips.

Image credit: Tabby Boyajian and her team of PlanetHunters, via http://ift.tt/1Pjgrmk.

Image credit: Tabby Boyajian and her team of PlanetHunters, via http://ift.tt/1Pjgrmk.

Yet there are increasingly more and more stars that show these huge, irregular flux dips, and they all have a few things in common. They’re all young stars, they all emit infrared radiation, they all have circumstellar disks and they all show a variety of disk orientations with respect to our line-of-sight. Is it possible, just as we can’t see Saturn’s rings when they’re edge-on, that this mysterious star’s disk is edge-on, and that’s why we can’t see its infrared flux?

Artist’s conception of the extrasolar ring system circling the young giant planet or brown dwarf J1407b. Image credit: Ron Miller.

Artist’s conception of the extrasolar ring system circling the young giant planet or brown dwarf J1407b. Image credit: Ron Miller.

Go get the whole story on why alien megastructures are out, and a circumstellar disk, with either a warped inner disk or eccentric, cometary-like debris, is in!



from ScienceBlogs http://ift.tt/2c8zEHr

adds 2