View at EarthSky Community Photos. | Aurelian Neacsu in Visina, Dambovita, Romania, captured giant sunspot AR2786 on November 24, 2020. In this image, the sunspot is the large dark region in about the 8 o’clock position on the sun, near the edge or “limb” of the sun. A small dark spot – called AR2785 – is immediately to its right. Thank you, Aurelian.
Solar Cycle 25 has now begun, and we’re beginning to see more spots on the sun. Did you know these spots can be predicted in advance? Last week, on November 18, 2020, scientists at the National Solar Observatory (NSO) – whose headquarters are in Boulder, Colorado – predicted a large new sunspot group would emerge this week, just in time for the annual celebration of Thanksgiving in the U.S. The image above shows the spot as predicted, now coming into view. It’s called AR2786.
How did the NSO scientists know this spot would appear? Their prediction came via a technique developed at NSO in the 1990s, known as helioseismology. It’s a way of “listening” to changing sound waves from the sun’s interior. These scientists’ statement explained:
Seismology here on Earth measures sound waves traveling through Earth’s interior to reveal what we cannot see beneath the Earth’s surface. Similarly, helioseismology can highlight structures on the sun that cannot yet be seen from Earth. Millions of sound frequencies bounce freely throughout the sun’s interior, like a bell. Regions of strong magnetic fields perturb with these sound waves, thus a change in wave signal measurements indicates that sunspots may be present.
The 2021 lunar calendars are here! Order yours before they’re gone. Makes a great gift!
View at EarthSky Community Photos. | Radu Anghel in Bacau, Romania, caught AR2786 on November 24, 2020. He wrote: “It’s been a long time with no sunspot activity and now is comeback time. With the new sun cycle, we have an increased sunspot activity including, today, no less the three active regions: 2783, 2785 and 2786. The last one is a giant sunspot, several times bigger than Earth.” Thank you, Radu!
As seen from around the world, giant sunspot AR2786 will come into even better view in the days ahead, as the sun spins. It’ll be possible to glimpse with optical aid, using safe solar filters, or by using an indirect viewing method. Here are 7 tips for observing the sun safely.
Kiran Jain, the scientist who is leading the efforts at NSO to predict coming sunspots via helioseismology, said that the large sunspot AR2786 produced:
… the strongest far-side signal we have had this solar cycle. We first noticed the signal in our far-side images on November 14, 2020. It was inconspicuous at first but grew quickly, breaking detection thresholds just one day later. Since we are in the very early phase of the new solar cycle, the signal from this large spot stands out clearly.
View at EarthSky Community Photos. | Victor C. Rogus in Sedona, Arizona, captured AR 2786 on November 24, too. See how the spot is farther from the edge or “limb” of the sun now? The sun’s rotation is bringing it into better view. Thank you, Victor!
Solar storms are disturbances on the sun whose effects move through our solar system, sometimes striking Earth. They’re often seen to originate in the same region of the sun as sunspots, especially large, complicated sunspots like AR2786. Earth’s atmosphere protects earthly life from the effects of solar storms, but solar activity does affect our human technologies. The NSO statement explained:
The more tangled the magnetic field, the more likely it will result in large solar flares and coronal mass ejections that, in turn, can result in … effects at Earth. These include impacts on communications, GPS and possibly electrical grid systems.
So, when a sunspot like AR2786 occurs, solar scientists and other sun-watchers start watching for solar storms, and the sudden, bright solar flares that go with them. This activity on the sun creates what is called space weather, which NASA describes as:
… conditions on the sun, in the solar wind, and within Earth’s magnetosphere, ionosphere and thermosphere that can influence the performance and reliability of space-borne and ground-based technological systems and can endanger human life or health.
According to the website SpaceWeather.com, the smaller sunspot AR2785, which is near AR2786 on the sun, has already produced a C4-class solar flare, late in the day on November 23. SpaceWeather reported:
The explosion hurled a plume of plasma more than 350,000 km [217,000 miles] across the sun. NASA’s Solar Dynamics Observatory recorded the splashdown [see the animated image below].
SpaceWeather reported that a pulse of ultraviolet radiation from AR2785:
… hit Earth, briefly ionizing the top of our atmosphere. This, in turn, caused a shortwave radio blackout over the South Pacific, including eastern Australia and all of New Zealand: blackout map here. Frequencies affected were mainly below 10 MHz.
More solar flares are in the offing. Three of the biggest sunspots of young Solar Cycle 25 (AR2783, AR2785, AR2786) are either facing Earth or turning in our direction. They all pose a threat for C-class flares (like the one shown below) with a slight chance of even stronger M-flares.
On November 23, 2020, a solar flare from the smaller sunspot near AR2786 – AR2785 – hurled a plume of plasma across the sun that ultimately affected Earth. This sort of event is why scientists study activity on the sun. Image via NASA SDO/ SpaceWeather.com.
The National Solar Observatory helps track these events on the sun, via its GONG network, which consists of six monitoring stations positioned across the globe. The six stations give the GONG network 24-hour coverage of the sun.
Valentin Martinez Pillet, director of the National Solar Observatory, commented:
The GONG network is providing an essential service to United States space weather preparedness. But GONG is close to three decades old and is in need of an upgrade. The original system was not created with space weather in mind, so we are exploring options for the Next Generation GONG network, with modern instrumentation specially attuned with space weather as a priority.
NSF-funded GONG network uses sound waves to measure changes inside the sun, indicative of sunspots on the side pointing away from Earth. These diagrams of the sun’s internal acoustic waves with no sunspots (top panel) and with sunspots (bottom panel) show how the sunspot’s magnetic field perturbs the acoustic waves, changing their signature. Measuring this change allows scientists to predict sunspots on the far side of the sun. Image via NSO/ AURA/ NSF.
Giant sunspot AR2786 as seen from Australia on the morning of November 24, 2020. The sunspot is on the very edge, or “limb” of the sun, in nearly the 9 o’clock position; the image shows AR2786 just as it rotated into view. Image via NSO.
Bottom line: On November 18, scientists at the National Solar Observatory used the technique of helioseismology to predict a large sunspot would emerge from behind the sun. Now that sunspot – AR2786 – is visible. Here’s how they made the prediction.
from EarthSky https://ift.tt/2V3hlLk
View at EarthSky Community Photos. | Aurelian Neacsu in Visina, Dambovita, Romania, captured giant sunspot AR2786 on November 24, 2020. In this image, the sunspot is the large dark region in about the 8 o’clock position on the sun, near the edge or “limb” of the sun. A small dark spot – called AR2785 – is immediately to its right. Thank you, Aurelian.
Solar Cycle 25 has now begun, and we’re beginning to see more spots on the sun. Did you know these spots can be predicted in advance? Last week, on November 18, 2020, scientists at the National Solar Observatory (NSO) – whose headquarters are in Boulder, Colorado – predicted a large new sunspot group would emerge this week, just in time for the annual celebration of Thanksgiving in the U.S. The image above shows the spot as predicted, now coming into view. It’s called AR2786.
How did the NSO scientists know this spot would appear? Their prediction came via a technique developed at NSO in the 1990s, known as helioseismology. It’s a way of “listening” to changing sound waves from the sun’s interior. These scientists’ statement explained:
Seismology here on Earth measures sound waves traveling through Earth’s interior to reveal what we cannot see beneath the Earth’s surface. Similarly, helioseismology can highlight structures on the sun that cannot yet be seen from Earth. Millions of sound frequencies bounce freely throughout the sun’s interior, like a bell. Regions of strong magnetic fields perturb with these sound waves, thus a change in wave signal measurements indicates that sunspots may be present.
The 2021 lunar calendars are here! Order yours before they’re gone. Makes a great gift!
View at EarthSky Community Photos. | Radu Anghel in Bacau, Romania, caught AR2786 on November 24, 2020. He wrote: “It’s been a long time with no sunspot activity and now is comeback time. With the new sun cycle, we have an increased sunspot activity including, today, no less the three active regions: 2783, 2785 and 2786. The last one is a giant sunspot, several times bigger than Earth.” Thank you, Radu!
As seen from around the world, giant sunspot AR2786 will come into even better view in the days ahead, as the sun spins. It’ll be possible to glimpse with optical aid, using safe solar filters, or by using an indirect viewing method. Here are 7 tips for observing the sun safely.
Kiran Jain, the scientist who is leading the efforts at NSO to predict coming sunspots via helioseismology, said that the large sunspot AR2786 produced:
… the strongest far-side signal we have had this solar cycle. We first noticed the signal in our far-side images on November 14, 2020. It was inconspicuous at first but grew quickly, breaking detection thresholds just one day later. Since we are in the very early phase of the new solar cycle, the signal from this large spot stands out clearly.
View at EarthSky Community Photos. | Victor C. Rogus in Sedona, Arizona, captured AR 2786 on November 24, too. See how the spot is farther from the edge or “limb” of the sun now? The sun’s rotation is bringing it into better view. Thank you, Victor!
Solar storms are disturbances on the sun whose effects move through our solar system, sometimes striking Earth. They’re often seen to originate in the same region of the sun as sunspots, especially large, complicated sunspots like AR2786. Earth’s atmosphere protects earthly life from the effects of solar storms, but solar activity does affect our human technologies. The NSO statement explained:
The more tangled the magnetic field, the more likely it will result in large solar flares and coronal mass ejections that, in turn, can result in … effects at Earth. These include impacts on communications, GPS and possibly electrical grid systems.
So, when a sunspot like AR2786 occurs, solar scientists and other sun-watchers start watching for solar storms, and the sudden, bright solar flares that go with them. This activity on the sun creates what is called space weather, which NASA describes as:
… conditions on the sun, in the solar wind, and within Earth’s magnetosphere, ionosphere and thermosphere that can influence the performance and reliability of space-borne and ground-based technological systems and can endanger human life or health.
According to the website SpaceWeather.com, the smaller sunspot AR2785, which is near AR2786 on the sun, has already produced a C4-class solar flare, late in the day on November 23. SpaceWeather reported:
The explosion hurled a plume of plasma more than 350,000 km [217,000 miles] across the sun. NASA’s Solar Dynamics Observatory recorded the splashdown [see the animated image below].
SpaceWeather reported that a pulse of ultraviolet radiation from AR2785:
… hit Earth, briefly ionizing the top of our atmosphere. This, in turn, caused a shortwave radio blackout over the South Pacific, including eastern Australia and all of New Zealand: blackout map here. Frequencies affected were mainly below 10 MHz.
More solar flares are in the offing. Three of the biggest sunspots of young Solar Cycle 25 (AR2783, AR2785, AR2786) are either facing Earth or turning in our direction. They all pose a threat for C-class flares (like the one shown below) with a slight chance of even stronger M-flares.
On November 23, 2020, a solar flare from the smaller sunspot near AR2786 – AR2785 – hurled a plume of plasma across the sun that ultimately affected Earth. This sort of event is why scientists study activity on the sun. Image via NASA SDO/ SpaceWeather.com.
The National Solar Observatory helps track these events on the sun, via its GONG network, which consists of six monitoring stations positioned across the globe. The six stations give the GONG network 24-hour coverage of the sun.
Valentin Martinez Pillet, director of the National Solar Observatory, commented:
The GONG network is providing an essential service to United States space weather preparedness. But GONG is close to three decades old and is in need of an upgrade. The original system was not created with space weather in mind, so we are exploring options for the Next Generation GONG network, with modern instrumentation specially attuned with space weather as a priority.
NSF-funded GONG network uses sound waves to measure changes inside the sun, indicative of sunspots on the side pointing away from Earth. These diagrams of the sun’s internal acoustic waves with no sunspots (top panel) and with sunspots (bottom panel) show how the sunspot’s magnetic field perturbs the acoustic waves, changing their signature. Measuring this change allows scientists to predict sunspots on the far side of the sun. Image via NSO/ AURA/ NSF.
Giant sunspot AR2786 as seen from Australia on the morning of November 24, 2020. The sunspot is on the very edge, or “limb” of the sun, in nearly the 9 o’clock position; the image shows AR2786 just as it rotated into view. Image via NSO.
Bottom line: On November 18, scientists at the National Solar Observatory used the technique of helioseismology to predict a large sunspot would emerge from behind the sun. Now that sunspot – AR2786 – is visible. Here’s how they made the prediction.
from EarthSky https://ift.tt/2V3hlLk
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