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The Solar Atmosphere II
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The Chromosphere-region of partially ionized hydrogen
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The Solar Corona What is it? How did it get that way?
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Corona shines at level of one millionth the photosphere
Corona shines at level of one millionth the photosphere. It is Thompson scattered sunlight
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To understand astronomical objects, astronomers take spectra
The spectrum of the corona reveals its most interesting characteristic
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The dominant ionization state depends on the temperature…example N
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The X-Ray Sun
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The Temperature Profile in the Solar Atmosphere
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The key to understanding the corona is the solar magnetic field
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Above the corona: direct magnetometer measurements in the solar wind
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The Flowing Medium of the Solar Wind
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The Sun on August 16, 2003
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