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The Sun - The Big Picture - Boston.com
A sweeping prominence, a huge cloud of relatively cool dense plasma is seen suspended in the Sun’s hot, thin corona. At times, promineces can erupt, escaping the Sun’s atmosphere. Emission in this spectral line shows the upper chromosphere at a temperature of about 60,000 degrees K (over 100,000 degrees F). Every feature in the image traces magnetic field structure. The hottest areas appear almost white, while the darker red areas indicate cooler temperatures. (Courtesy of SOHO/EIT consortium)
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Detailed closeup of magnetic structures on the Sun’s surface, seen in the H-alpha wavelength on August 22, 2003. (Swedish 1-m Solar Telescope (SST) operated by the Royal Swedish Academy of Sciences, Oddbjorn Engvold, Jun Elin Wiik, Luc Rouppe van der Voort) #
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NASA’s STEREO satellite captured the first images ever of a collis...
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