Solar fine structures: Their importance in the sun's physics and their observation

Details Solar fine structures: Their importance in the sun's physics and their observation Solar fine structures: Their importance in the sun's physics and their observation

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.235..169h&link_type=abstract

In ESA Future Missions in Solar, Heliospheric and Space Plasma Physics p 169-174 (SEE N86-27330 18-12)

Physics

Atmospheric Stratification, Fine Structure, Solar Atmosphere, Solar Physics, Plasma Heating, Soho Mission, Solar Activity, Solar Corona, Solar Heating, Solar Wind Velocity

Scientific paper

Structures in the Sun's atmosphere are reviewed. The essential role of these structures in the physics of the Sun's convective zone and atmosphere is stressed, and it is emphasized that the same physics is crucial in a number of other systems of planetological or astrophysical interest. The problem of solar coronal heating is considered, and its relation to the solar wind acceleration problem is discussed. The diagnosing of nonthermal heating phenomena is shown to involve elaborate observations with high spectral, spatial and temporal resolution. It is concluded that the SOHO project appears to be the best step to take.

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