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  SDO Observes Massive Eruption, Scor...
  SDO Observes Massive Eruption, Scorching Rain - April 27, 2010: Just last week, scientists working with NASA's new Solar Dynamics Observatory (SDO) released the most astonishing movies of the sun anyone had ever seen. Now, they're doing it again. "SDO has just observed a massive eruption on the sun—one of the biggest in years," says Lika Guhathakurta of NASA headquarters in Washington DC. "The footage is not only dramatic, but also could solve a longstanding mystery of solar physics." Karel Schrijver of Lockheed Martin's Solar and Astrophysics Lab is leading the analysis. "We can see a billion tons of magnetized plasma blasting into space while debris from the explosion falls back onto the sun surface. These may be our best data yet." One of SDO's game-changing capabilities is temperature sensing. Using an array of ultraviolet telescopes called the Atmospheric Imaging Assembly (AIA), the observatory can remotely measure the temperature of gas in the sun's atmosphere. Coronal rain turns out to be relatively cool—"only" 60000 K. When the rains falls, it is supported, in part, by an underlying cushion of much hotter material, between 1000000 and 2200000 K. "You can see the hot gas in the color-coded temperature movie," says Schrijver. "Cool material is red, hotter material is blue-green. The hot gas effectively slows the descent of the coronal rain." Dick Fisher, the head of NASA's Heliophysics Division in Washington DC, has been working in solar physics for nearly forty <b>...</b>
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  SDO Observes Massive Eruption, Scor...
  A color-coded temperature movie of the eruption. Red and oranges are cool (60000 K - 80000 K); blues and greens are hot (1000000 - 2200000 K). The black "hair-like object" is a speck of dust on the CCD camera. Credit: SDO/AIA. One of SDO's game-changing capabilities is temperature sensing. Using an array of ultraviolet telescopes called the Atmospheric Imaging Assembly (AIA), the observatory can remotely measure the temperature of gas in the sun's atmosphere. Coronal rain turns out to be relatively cool—"only" 60000 K. When the rains falls, it is supported, in part, by an underlying cushion of much hotter material, between 1000000 and 2200000 K. "You can see the hot gas in the color-coded temperature movie," says Schrijver. "Cool material is red, hotter material is blue-green. The hot gas effectively slows the descent of the coronal rain." Dick Fisher, the head of NASA's Heliophysics Division in Washington DC, has been working in solar physics for nearly forty years. "In all that time," he says, "I've never seen images like this." "I wonder, what will next week bring?" Credit: NASA SDO / Lockheed Space Systems Company for AIA
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