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Quantum fluctuations in science, space and society, from quarks to Hubble and Mars. Served up by Alan Boyle, NBC News Digital science editor. E-mail Alan, or connect via Facebook, Twitter or Google+.

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  • 21
    Jul
    2011
    11:17pm, EDT

    Last looks at the shuttle in orbit

    Thierry Legault / Astrophoto.fr

    A three-image composite tracks the International Space Station and the shuttle Atlantis as they move across the sun's disk on July 15.

    By Alan Boyle, Science Editor, NBC News

    They look like alien bugs hopping across the sun, but these specks may represent the very last pictures of a space shuttle in orbit as seen from Earth.

    French astrophotographer Thierry Legault, an expert in the technique of tracking spacecraft silhouettes, captured these views of the International Space Station and the shuttle Atlantis during their final rendezvous. Atlantis landed today, bringing the 30-year space shuttle program to an end.


    The picture above is a composite, showing three views of the station-shuttle complex as it passed over the sun's disk on July 15. Legault had to travel to just the right location to get the shot. This one was taken from Caen in France. The entire transit took just seven-tenths of a second. Legault has labeled the shuttle and elements of the space station in this higher-resolution view:

    Thierry Legault / Astrophoto.fr

    The labels on this image point out the position of Atlantis and components of the International Space Station during a July 15 transit.

    In an email, Legault told me that he traveled through the Czech Republic, Germany and the Netherlands to capture the silhouettes. One picture, snapped north of Prague and posted to Legault's website, shows the space station and the shuttle side by side, 50 minutes after Atlantis' undocking earlier this week.

    Legault produced the piece de resistance today during a stopover near Emden, in northern Germany. It may not look quite as impressive as the others, but it could well be more historic. Legault wrote that the picture was taken "just 21 minutes before the deorbit burn, therefore there are chances that it is the very last image of a space shuttle in orbit."

    Here's a composite of four images, taken during the 0.9-second-long transit. The silhouettes of Atlantis are highlighted within white circles:

    Thierry Legault / Astrophoto.fr

    A four-image composite tracks Atlantis' transit across the sun's disk, just 21 minutes before today's deorbit burn. The white circles highlight Atlantis.

    For the telescope and camera buffs out there, Legault says the images were produced using a Takahashi TOA-150 6-inch apochromatic refractor (focal length 3600mm) on an EM-400 mount, with a Baader Herschel wedge. The camera is a Canon 5D Mark II, set for an exposure of 1/8000s, 100 ISO, working in continuous shooting at four frames per second. Transit forecasts were calculated by www.calsky.com.

    Merci beaucoup to Thierry for sharing his pictures with us through the years.

    More great views of Atlantis:

    • Space station crew watches Atlantis descend
    • Photographers capture Atlantis' last landing
    • Southern lights are sweeter in space
    • Aircraft captures unique view of launch 
    • Shuttle Atlantis' last trek to liftoff 
    • Atlantis' flight on PhotoBlog

    Connect with the Cosmic Log community by "liking" the log's Facebook page or following @b0yle on Twitter. You can also check out "The Case for Pluto," Alan's book about the controversial dwarf planet and the search for new worlds.

    11 comments

    Nice photos! Did anyone read the story about the 3 missing astronauts?

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  • 14
    Jun
    2011
    1:37pm, EDT

    Solar forecast hints at a big chill

    AFP - Getty Images

    The sun unleashes a powerful solar flare from the right side of its disk on June 7, as seen in this image from NASA's Solar Dynamics Observatory. Scientists say the sun is heading toward a peak in its activity cycle in 2013 or so, but may enter a period of hibernation afterward.

    By Alan Boyle, Science Editor, NBC News

    Last updated 3:15 p.m. ET

    The latest long-range space forecast predicts a prolonged drop in solar activity after the next peak — and scientists say that might cool down temperatures here on Earth, or at least slow down the warming trend a bit. 

    Scientists have studied sunspots and the sun's 11-year activity cycle for 400 years, and they're getting increasingly savvy about spotting the harbingers of "space weather" years in advance, just as meteorologists can figure out what's coming after the next storm.

    Storms from the sun are expected to build to a peak in 2013 or so, but after that, the long-range indicators are pointing to an extended period of low activity — or even hibernation.

    "This is important because the solar cycle causes space weather ... and may contribute to climate change," Frank Hill, associate director of the National Solar Observatory's Solar Synoptic Network, told journalists today.

    In the past, such periods have coincided with lower-than-expected temperatures on Earth. The most famous example is the Maunder Minimum, a 70-year period with virtually no sunspots from 1645 to 1715. Average temperatures in Europe sank so low during that period that it came to be known as "the Little Ice Age."

    The linkage between solar activity and climate change is still a matter of scientific debate. And even if there is a link, it's not clear how solar-caused global cooling might interact with industrial global warming due to greenhouse-gas emissions. Climate scientists say the swings in solar activity that they've studied so far have had little or no impact on temperatures or other climate indicators — and they don't expect to see a big impact even if the sun goes quiet for a decade or longer.

    But if today's forecast is correct, solar physicists and climatologists will have a golden opportunity to find out for sure.

    Hill said scientists had "no way of predicting" how long the hibernation period might last. "It may very well last as long as the Maunder Minimum ... if it occurs," he said.

    Hill and other experts on solar activity announced the long-range forecast today at the annual meeting of the American Astronomical Society's Solar Physics Division, being conducted this week at New Mexico State University in Las Cruces, N.M. 

    How do they know?
    The forecast is based on three indicators thought to be tied to long-range solar activity, the comparative rise and fall of sunspots over the activity cycle, as well as the brightness of those sunspots; patterns in the sun's internal "jet stream" of superheated plasma; and the pace of migration in the sun's magnetic field toward the poles, as seen in the sun's corona.

    An unusually low number of sunspots have been observed during the current cycle, and the spots are fainter than average. Scientists say they have seen no sign of a characteristic east-west flow of internal plasma, which usually sets the stage for future increases in activity. And the magnetic "rush to the poles" appears to be slowing down.

    All these signs suggest that the current solar cycle, Cycle 24, "may be the last one for quite some time," Hill said. The next upswing in solar storms, Cycle 25, may be "very much delayed ... very weak, or may not happen at all."

    Beyond the climate effect, solar activity is known to have a significant potential impact on satellite operations, electric power grids and even exposure to radiation at high-altitudes. Solar storms can disrupt satellite signals or air-traffic navigation systems. In 1989, a solar outburst caused a widespread power outage in Quebec. And particularly strong solar flares have forced astronauts to take shelter in shielded areas of the space shuttle or the International Space Station.

    Some observers have worried about the possibility of a massive geomagnetic super-storm like the one that swept over Earth in 1859, known as the "Carrington event." For those folks, the news that the sun appears to be settling down, coupled with indications that the 2013 solar maximum is not expected to be unusually strong, should be reassuring.

    About that ice age ...
    Hill and two other solar physicists involved in formulating the forecast, NSO researcher Matt Penn and Richard Altrock of the U.S. Air Force's coronal research program, said there was not yet enough data to firm up a climate connection to solar activity. But they and other scientists have noted that historic lulls in sunspots, such as the Maunder Minimum and another solar minimum between 1790 and 1830, coincided with cooler temperatures.

    Gavin Schmidt, a climatologist at NASA's Goddard Institute for Space Studies and one of the founders of the RealClimate blog, said the effects of solar activity on climate over the past 30 years have been "at the margin of what we can detect."

    "They are detectable in the high atmosphere, but when you get down to the surface, there is so much other stuff going on that it's been really hard to get a clean signal," he told me.

    One of the reasons why so little is known about solar effects on climate is that the sun's highs and lows have been within such a narrow range in recent history.

    "If we were to see a return to what's called Maunder Minimum conditions in the next 50 years or so, that would be interesting," Schmidt said. "I think we'd learn a lot about solar physics and solar variability. ... It's going to be scientifically very exciting if all this pans out."

    Even then, however, he estimated that the effect of greenhouse-gas emissions would be on the order of 10 times as great. "What you might see over a 20- to 30-year period is a slight slowdown in the pace of warming," Schmidt said. "In terms of how we should think about climate change prediction in the future, reducing emissions and so on, it really wouldn't make much of a difference."

    But what about the Little Ice Age in the 1600s, when Swiss Alpine villages were reported destroyed by encroaching glaciers? Schmidt said that period also coincided with an upswing in volcanic emissions, which are known more definitely to contribute to global cooling.

    "Parsing out how much of that was solar, how much of that was volcanic and how much of that was just noise ... that's tricky," Schmidt said.

    Will this latest forecast be used to argue that we don't need to worry about global warming? Or will the effect of solar hibernation (if it even occurs) turn out to be a blip at best? Feel free to weigh in with your comments below.

    More on solar weather:

    • U.N. to upgrade space weather forecasts
    • Sun unleashes 'spectacular' solar storm
    • Solar cycle sparks doomsday buzz; don't panic
    • Still more about space weather from msnbc.com

    The studies presented at this week's SPD meeting in Las Cruces include "Large-Scale Zonal Flows During the Solar Minimum — Where Is Cycle 25?" by Frank Hill, R. Howe, R. Komm, J. Christensen-Dalsgaard, T.P. Larson, J. Schou and M.J. Thompson; "A Decade of Diminishing Sunspot Vigor" by W.C. Livingston, M. Penn and L. Svalgard; and "Whither Goes Cycle 24? A View From the Fe XIV Corona" by R.C. Altrock.

    You can connect with the Cosmic Log community by "liking" the log's Facebook page or following @b0yle on Twitter. Also, give a look to "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

    205 comments

    I often envy the climate change deniers: It must be nice and comforting to be able to see the world through such simple eyes.

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  • 6
    Jun
    2011
    3:37pm, EDT

    NASA / GSFC / STEREO

    On May 30, 2011, the STEREO Behind spacecraft caught a prominence in the process of leaping from one part of the sun to another.

    Massive solar flare somersaults

    The "Behind" member of NASA's STEREO spacecraft studying the sun has captured spectacular imagery of a rare somersaulting coronal mass ejection.


    A movie of the event combines images captured with the spacecraft's Extreme Ultraviolet Imager (EUVI) and Inner Coronograph (COR1) telescopes.

    The prominence is first seen erupting in the EUVI images and then in white light with COR1. In the white light images, the prominence pauses. Some of the material then drains back down, but most of it is defected to the north and ends up raining down on a different part of the sun.

    According to NASA, this is unusual behavior and will be studied carefully by scientists.

    To check our more images from NASA missions, be sure to check out the NASA Goddard stream on Flickr.


    Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    3 comments

    Global warming is making the sun too hot!

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  • 31
    Mar
    2011
    3:14pm, EDT

    NASA / GSFC / SDO

    A March 29 image from NASA's Solar Dynamics Observatory captures a "space eclipse," in which Earth's disk obscures part of the sun.

    'Tis the season for space eclipses

    By Alan Boyle, Science Editor, NBC News

    NASA's Solar Dynamics Observatory stares at the sun 24/7, but twice a year, Earth gets slightly in the way for up to 72 minutes a day. That creates an "eclipse" that blocks part of the sun's disk. The spring eclipse season is now under way, as you can see in this picture captured on Tuesday. Your typical partial solar eclipse involves the moon's sharply defined disk passing in front of the sun, but during the Solar Dynamics Observatory's eclipses, Earth's atmosphere creates a fuzzy line between the sun and the darkness. Some of the sun's brighter features manage to shine through the murk.

    Check out NASA's Eclipse website for upcoming opportunities to see eclipses from Earth, including a partial solar eclipse on June 1 and total lunar eclipses on June 15 and Dec. 10.

    More out-of-the-ordinary eclipses:

    • European probe tracks solar eclipse from outer space
    • Eclipse seen by moon probe as Earth blocks the sun
    • Sun gets double-crossed by moon and space station
    • Watch a partial eclipse and a sunset on Mars

    Join the Cosmic Log community by clicking the "like" button on our Facebook page or by following msnbc.com science editor Alan Boyle as b0yle on Twitter. To learn more about my book on Pluto and the search for planets, check out the website for "The Case for Pluto."

    2 comments

    it is a wonder we can't use a nuetron interferometer to infer the moons interior during these events....

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  • 23
    Mar
    2011
    10:56am, EDT

    Brown dwarf as cool as coffee found

    ESO / L. Calcada

    This artist's impression shows the pair of brown dwarfs named CFBDSIR 1458+10. Observations with ESO's Very Large Telescope and two other telescopes have shown that this is the coolest pair of brown dwarfs found so far. The cooler of the two components (in the background) is a candidate for the brown dwarf with the lowest temperature ever found - the surface temperature is similar to that of a cup of hot coffee. The two components are both about the same size as Jupiter.

    By John Roach, Contributing Writer, NBC News

    Astronomers have found a star that's only as hot as a cup of coffee, making it a candidate for the coldest star known. That is, assuming it's a star.

    While a cup of coffee may sound hot — the newly discovered object is about 200 degrees Fahrenheit (100 degrees Celsius) — our sun is about 10,000 degrees F (5,500 degrees C). So, by comparison, it really is quite cold.

    The object is considered a brown dwarf, a cosmic misfit that's cold enough to blur the lines between small cold stars and big hot planets. Astronomers consider brown dwarfs failed stars because they lack the mass and gravity to trigger the nuclear reactions that make stars shine brightly.


    The newly discovered brown dwarf, identified as CFBDSIR 1458+10B, is the dimmer member of a binary brown dwarf system located about 75 light-years from Earth.

    "In terms of its physical properties, it is really much closer to typical gas planets that are being found by radial velocity surveys than most brown dwarfs we know about," Michael Liu of the University of Hawaii's Institute for Astronomy told me.

    Unique properties
    Indeed, with a coffeelike temperature, astronomers expect the brown dwarf to exhibit the properties of a gas giant planet, such as the presence of water clouds in its atmosphere.

    "We think as we accumulate more data on its different colors and its spectra we should be able to learn more about its atmosphere, and that will be very unique," Liu added. For example, the color of hotter brown dwarfs is largely shaped by the presence of sodium and potassium atoms in the atmosphere.

    At cooler temperatures, according to theory, the sodium and potassium will lock themselves into molecules such as potassium chloride and be removed from the atmosphere. Liu and colleagues have asked for time on the Hubble Space Telescope to observe the system in optical wavelengths.

    "The optical colors of this object should be very different than any previously known brown dwarf," Liu said.

    Dwarf vs. planet
    But is it a brown dwarf? One definition astronomers use to differentiate between stars, brown dwarfs and planets is mass. Anything below about 13 Jupiter masses doesn't get hot enough or dense enough to fuse anything in its interior, so it considered a planet.

    The smaller member of the binary system is estimated to be between six and 15 Jupiter masses. "So, most likely it is below the line, and so by that measure one could call it a planet," Liu said.

    "But at the same time, I think most of us (astronomers) feel that the way in which something forms, which is difficult to measure, probably has something to do with the way we should classify them," he added.

    And this is without a doubt a binary star system – that is two stars orbiting around a common center of mass. Liu and colleagues think it likely formed as low-mass tail of the star forming process, which is different than the way a gas giant planet forms in a disc of material around a star.

    "Even though it formed in a different way, it is very low mass, very little energy is coming out and it is very, very cool," Liu said. "And it is a significant leap over the previous coolest known brown dwarf."

    More cool dwarfs
    Today's announcement comes days after another cool brown dwarf, CFBDS J005910.83-011401.3 located about 40 light years from our solar system, was pronounced as possibly the coldest. This free floating star is about 660 degrees F (350 C).

    In addition, two recent brown dwarf discoveries from the Spitzer Space Telescope are also contenders for the coolest objects known, though their temperatures are less well constrained.

    Preliminary measurements put the coolest of the Spitzer discoveries at 86 degrees F – about perfect beach weather – and orbiting a white dwarf star at a distance of about 2,500 times that of Earth and the sun, Discovery News reports.

    Further observations of the Spitzer object with other telescopes, Liu said, should help pin down its temperature.

    "My bet is that will turn out to be slightly colder than our object," he noted. "But I think the real interesting thing … is that all three objects may be in this completely new regime that people have been trying to get into for several years."

    New tools
    Key to the discovery of the brown dwarf Liu is reporting was adaptive optics instrumentation on the Keck II Telescope in Hawaii, which essentially cancels out much of Earth's atmospheric interference.

    This allowed the astronomers to confirm the double dwarfs were linked. The Canada-France-Hawaii Telescope was used to determine distance to the duo.

    The binary system was originally detected in 2010 with the European Southern Observatory's Very Large Telescope in Chile, though it was thought to be a single object – albeit with a temperature cool enough to make it the third coldest star known.

    "We were very excited originally to see this object had such a low temperature, but we never guessed that it would turn out to be a binary star and have an even more interesting, even colder companion," Phillipe Delorme of the University of Grenoble, said in a press release.

    The researchers are reporting their discovery in an upcoming issue of Astrophysical Journal. The paper is available online.

    More stories on cool brown dwarfs:

    • A new brown dwarf? If so, this one's even cooler
    • Astronomers discover the coldest stars yet
    • Planetary seeds spotted around brown dwarfs
    • Baby brown dwarf twins seen by astronomers
    • Mystery looms over possible brown dwarf star

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    54 comments

    yet another example of why the IAU can go suck eggs. > I say "Ni"! <

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  • 9
    Mar
    2011
    3:50pm, EST

    Stunning views of the sun ... and Discovery?!

    By Jonathan Woods

    Amateur astrophotographer Alan Friedman has done it again. Adding to an already impressive collection of outer space images, he just published two more magnificent photos of the sun. First, here's a view of a gassy prominence flaring off the sun like a cloud:

    Alan Friedman

    This section of the solar disk was imaged at the Winter Star Party on West Summerland Key in Florida, in the midst of 30 mph winds. The massive detached solar prominence was visible for hours. Skies were quite steady, despite the wind.

    To add some perspective on the sheer magnitude of what Friedman is documenting, look at the dark spot below the prominence. That spot is roughly twice the size of the Earth. 

    Using the same specialized equipment he used in October 2010 to produce the last set of breathtaking images, Friedman looks at the deep red end of the light spectrum to capture the emissions given off by hydrogen gas in the sun's atmosphere.

    He also came away with a historic glimpse of Discovery as it was docked to the International Space Station, during the space shuttle's final mission.

    Friedman said he captured the event, lasting just a fifth of a second, after making an 1,800-mile drive from Buffalo, N.Y., to the Winter Star Party in West Summerland Key, Fla.

    He went to the Florida gathering "for the steady skies, warm temperatures and the company of good astronomy friends." But when he learned that the International Space Station would cross paths with the sun, and that the sight would be visible 20 miles north of where the star party was being held, he felt compelled to document the flyover.

    "I jumped into the car with solar imaging gear, and we got set up just in time to catch it." he said. "I underestimated the narrowness of this event. We were about 5,000 feet south of the centerline in a good location... another 500 feet and we would have missed it entirely. Lucky day!"

    Alan Friedman

    Silhouetted by the sun, the space shuttle Discovery can be seen docked to the International Space Station during its final mission.

    Friedman talks with TODAY.com's Dara Brown about his latest work:

    More imagery of the sun and the shuttle:

    • Stare at the sun: An unusual view by Alan Friedman
    • Greatest hits from the space shuttle Discovery
    • More space shots for shuttle fans
    • Month in Space Pictures

    31 comments

    The article calls Friedman an "amateur astrophotographer", but I think we can just call him "astrophotographer" after this. There's nothing "amateur" about these images. They are magnificent.

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  • 28
    Feb
    2011
    6:45pm, EST

    NASA released some amazing solar flare video today

    By Stokes Young

    Images like these, captured by NASA's Solar Dynamics Observatory on Feb. 24, make we wish our video player had a "loop" function.

    Check out some previous posts of solar photography on PhotoBlog:

    • Sun shoots out monster blast ... but Earth is safe (A still photograph of the event in the video above, with more reporting from John Roach)
    • Double whammy on the sun (Two simultaneous flares occured in January)
    • Stare at the sun (Nov. 2, 2010 - one of our most popular posts shows pictures by amateur astrophotographer Alan Friedman--if you haven't seen it before, you should take a look.)

    Comment

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  • 10
    Feb
    2011
    4:42pm, EST

    Hinode / XRT

    An X-ray image of the sun shows gaping holes in the corona. Plasma escapes to space through these coronal holes.

    Satellite spots the sun's latest leaks

    By John Roach, Contributing Writer, NBC News

    A Japanese-led satellite mission that's studying the sun in extreme ultraviolet and X-ray wavelengths has revealed gaping holes in the solar corona through which plasma can easily escape into space. The so-called coronal holes are the darker areas in this X-ray image — one at the top center and another capping the solar south pole, about where Antarctica is on Earth.


    Scientists believe the sun's magnetic field traps jets of plasma from the sun's surface, heating up the solar atmosphere, or corona, to millions of degrees. Coronal holes represent gaps in the magnetic field, allowing the plasma to stream straight out into space. The lack of trapped plasma also means the holes are relatively cool in temperature, compared to the active regions nearby.

    The Hinode satellite, which made this image, is part of a swarm of scientific instruments dedicated to monitoring the sun to help scientists improve forecasts of space weather. Coronal holes are thought to be the start of the space weather chain that can wreak havoc on Earth by knocking out communications satellites and power grids.

    SpaceWeather.com is one of the best places on the Web to keep yourself up to date on the solar outlook. Today's highlights include the passage of an active sunspot around the sun's far side, plus an amazing Hubble flare and a beautiful recap of last week's northern lights.

    More stories on sun and space weather:

    • Astronomers discover source of solar wind
    • Sun's magnetic secret revealed
    • Hot news: See the sun's corona in full
    • Sun's super-hot shell cooked by plasma jets

    Tip o' the Log to Ian O'Neill at Discovery News.

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    6 comments

    Celestial alignment, gravity, Xrays, gamma rays..... whew.... yellowstone bulging, Krakatoa growing, north, south poles going haywire, .... things are happening, maybe too slow to notice. K heres my horrible hypothisisisisiis, .... the center of the galaxy's gravitiational forces ,will align with t …

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  • 4
    Feb
    2011
    2:05pm, EST

    Solar blasts spark Earthlike clouds

    NASA

    Instabilities build up on one flank of clouds of material exploding from the sun. The instabilities may explain why coronal mass ejections bend and twist instead of following a straight path.

    By John Roach, Contributing Writer, NBC News

    When clouds of material explode from the sun, instabilities appear to form and build up on one flank of the ejected material, new observations from NASA's Solar Dynamics Observatory show. Because these instabilities are similar to those observed in Earth's clouds and oceans, researchers have a new tool for predicting space weather. 

    The observations of the outbursts, called coronal mass ejections or CMEs, were made in the extreme ultraviolet at a temperature range previously unavailable — 11 million Kelvin, according to astrophysicists at the University of Warwick in Britain, who are studying the images made with the observatory's Atmospheric Imaging Assembly.


    According to the team, the so-called Kelvin-Helmholtz (or KH) instabilities appear to roll up into growing whirls at boundaries between materials moving at different speeds. The difference in speed produces boundary instabilities.

    The instabilities in the CMEs closely parallel instabilities seen in Earth's atmosphere, and in waves on the surface of the seas. Scientists had predicted they occur within the solar system's weather, but this is the first time the ripples have been directly observed in the sun's corona.

    The researchers studying the images are particularly intrigued by how the instabilities build up on one side of the CME — this may explain why CMEs appear to bend and twist instead of following a straight path from the surface of the sun. Further understanding the results could assist physicists trying to understand and predict space weather.

    "If the instabilities form on just one flank, they may increase drag on one side of the CME causing it to move slower than the rest of the CME," Claire Foullon, a researcher at the University of Warick, said in an image advisory.

    A paper outlining the observations and detailed modeling on how they the phenomenon occurs appears in the Astrophysical Journal Letters.

    More stories on coronal mass ejections:

    • Here comes the sun storm
    • Solar shocker: Sun storms change directions
    • Photoblog: Double whammy on the sun
    • See a twister on the sun

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

     

     

     

    9 comments

    Is Drag strictly Friction on the atmosphere of the sun, or would magnetic pull or gravity also be in play? Drag could be one of the reasons the universe is expanding at different rates and making it larger in size. Much like a shotshell being fired. The shot doesn't stay together in one mass nor in  …

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  • 28
    Jan
    2011
    4:58pm, EST

    NASA

    The Solar Dynamics Observator caught nearly simultaneous solar eruptions on opposite sides of the sun. Recent research suggests the activity might be linked.

    Double whammy on the sun

    By John Roach, Contributing Writer, NBC News

    A spectacular double eruption on the sun was captured today by NASA's Solar Dynamics Observatory. The eruptions happened nearly simultaneously on opposite sides of the solar disk, SpaceWeather.com reported. The plasma clouds produced by the event are expected to miss Earth, so there's no threat to us or to satellites orbiting the planet.

    On the lower left in this image of the sun, a magnetic filament erupted, and on the upper right a departing sunspot produced the strongest solar flare of the year so far, an M1-class event. The double whammy may be more than a mere coincidence: Recent research suggests that solar activity is interconnected by magnetism over large distances, and that solar storms can go global.

    For still more stunning views of the cosmos, check out the latest edition of Month in Space Pictures.


    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    328 comments

    Wow! And to think that whole gigantic thing is a huge ball of mostly hydrogen undergoing fusion to form helium, lithium, carbon and other heavier elements as it radiates the excess energy from the lost mass converted by e=mc^2 into heat and light. It's no wonder the ancient Egyptians worshipped it a …

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  • 4
    Jan
    2011
    4:42pm, EST

    Thierry Legault / Astrophoto.fr

    Belgian astrophotographer Thierry Legault's picture of Tuesday's partial solar eclipse also shows the International Space Station passing over the sun's disk.

    Sun gets double-crossed

    By Alan Boyle, Science Editor, NBC News

    There are plenty of jaw-dropping pictures of today's partial solar eclipse — but this one is something special, even in the eclipse category. French astrophotographer Thierry Legault traveled to Oman to take some vacation, and take in the eclipse from a region where the chances of clear skies were close to 100 percent. The moon's disk covers up part of the sun at lower left ... but wait, is that a "Star Wars" tie fighter visible at upper left? Nope, it's the International Space Station, which Legault knew would be crossing over the sun's disk for less than a second while the eclipse was taking place. A smattering of sunspots can be seen as well.

    "The image shows three planes in space: the sun at 150 million kilometers, the moon at about 400,000 kilometers and the ISS at 500 kilometers," Legault writes.

    For photo buffs, here are the technical details: The telescope was a Takahashi FSQ-106ED refractor on an EM-10 mount. The camera was a Canon 5D Mark II, and the exposure was one-5,000th of a second at 100 ISO.

    Check out Legault's space station transit imagery on Astrosurf.com and SpaceWeather.com. You'll find still more amateur photography of the eclipse on SpaceWeather.com. Here's another one of Legault's amazing pictures from last May, showing the space station as well as the space shuttle Atlantis crossing in front of the sun's disk. For much, much more from Legault, feast your eyes on his Astrophoto.fr webpage.


    Connect with Cosmic Log by "liking" our Facebook page or hooking up on Twitter, and check out "The Case for Pluto," science editor Alan Boyle's book about Pluto and the planet quest.

    11 comments

    LOL for a sec i thought Canada had marked the sun for itself lol.

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  • 4
    Jan
    2011
    2:27pm, EST

    Hot news: See the sun's corona in full

    NASA / LMSAL / SAO

    This photograph of the sun, taken by the Atmospheric Imaging Assembly instrument on NASA's Solar Dynamics Observatory, shows how image processing techniques can reveal the faint, inner corona. At the sun's limb, prominences larger than the Earth arc into space. Bright active regions like the one on the sun's face at lower center are often the source of huge eruptions known as coronal mass ejections.

    By John Roach, Contributing Writer, NBC News

    Solar eclipse chasers are drawn to the fleeting moments of totality, when the sun’s outer atmosphere — called the corona — becomes visible to the naked eye. Now, thanks to an instrument onboard NASA’s Solar Dynamics Observatory as well as a new image-processing program, that moment can last 24 hours a day, seven days a week.

    The corona is hotter than the sun’s surface, but so tenuous that its light is overwhelmed by the much brighter solar disk. Therefore it is only visible from Earth when the sun is blocked, such as during an eclipse.


    SDO was launched last February on a mission to study the sun and its influence on Earth and near-Earth space. Even before the mission, solar astronomers didn’t have to wait around for solar eclipses and clear skies to get a view of the corona — but their tool of choice, called a coronograph, partially blocks the area immediately surrounding the sun, leaving only the outer corona visible. The effect is akin to holding your hand in front of your face as you drive into the sun.

    The AIA allows astronomers to “follow the corona all the way down to the sun’s surface,” Leon Golub of the Harvard-Smithsonian Center for Astrophysics, said in a statement from the Harvard-Smithsonian Center for Astrophysics, or CfA. The instrument essentially fills the gap created by the limitations of the coronograph.

    CfA astronomers Steven Crammer and Alec Engell developed a computer program for processing the AIA images of the corona. These processed images, including the one above, imitate the blocking-out effect that occurs during a total solar eclipse, revealing the highly dynamic nature of the inner corona.

    The resulting images provide a full frontal view of the sun and its corona, highlighting the ever-changing connections between the gas captured by the sun’s magnetic field and the gas escaping into interplanetary space.

    The sun’s magnetic field molds and shapes the corona. Hot solar plasma streams outward in vast loops larger than Earth before plunging back onto the sun’s surface. Some of the loops expand and stretch bigger and bigger until they break, belching plasma outward.

    These belches of plasma, called coronal mass ejections, are responsible for creating brilliant auroral displays and can even knock out power grids, communications satellites, and pose a risk to astronauts on the International Space Station.

    In August, the SDO captured one such eruption directed right at Earth. The eruption was the first in what is expected to be increasing solar activity as the sun ramps up from a low in its 11-year activity cycle.

    The processed AIA images will be used to study the initial eruption phase of coronal mass ejections as they leave the sun and test theories of solar wind acceleration based on magnetic reconnection.

    For more on the sun and space weather check out the stories below:

    • Huge solar explosions can rock the entire sun
    • A ‘snake’ slithers across the sun
    • Solar outbursts? No worries for spacewalk
    • New solar observatory to unlock sun’s mysteries
    • The sun is yours … on a computer
    • ‘Spectacular’ sights come from solar probe 

    John Roach is a contributing writer for msnbc.com. Connect with the Cosmic Log community by hitting the "like" button on the Cosmic Log Facebook page or following msnbc.com's science editor, Alan Boyle, on Twitter (@b0yle).

    1 comment

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