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The Solar Atmosphere II

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Presentation on theme: "The Solar Atmosphere II"— Presentation transcript:

1 The Solar Atmosphere II

2 The Chromosphere-region of partially ionized hydrogen

3 The Solar Corona What is it? How did it get that way?

4 Corona shines at level of one millionth the photosphere
Corona shines at level of one millionth the photosphere. It is Thompson scattered sunlight

5 To understand astronomical objects, astronomers take spectra
The spectrum of the corona reveals its most interesting characteristic

6 The dominant ionization state depends on the temperature…example N

7 The X-Ray Sun

8 The Temperature Profile in the Solar Atmosphere

9 The key to understanding the corona is the solar magnetic field

10 Above the corona: direct magnetometer measurements in the solar wind

11 The Flowing Medium of the Solar Wind

12 The Sun on August 16, 2003


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