Electron kinetic processes in the solar corona and wind
The Sun is surrounded by a 10^6 K hot atmosphere, the corona. The corona and the solar wind are fully ionized, and therefore in the plasma state. Magnetic fields play an important role in a plasma, since they bind electrically charged particles to their field lines. EUV spectroscopes, like the SUMER...
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| Format: | Others |
| Language: | English |
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Universität Potsdam
2012
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| Online Access: | http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-65259 http://opus.kobv.de/ubp/volltexte/2013/6525/ |