The Variation of Coronal Holes with Solar Cycle by Steven Chapman

The Variation of Coronal Holes with Solar Cycle

Steven Chapman

336 pages missing pub info (editions)

nonfiction science
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Coronal holes are commonly known to be the source of the open magnetic flux and the high-speed solar wind. In EUV and X-ray emission lines, coronal holes are seen as the regions with reduced emission due to lower temperatures and electron density ...

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