Small scale structures in the solar corona

Details Small scale structures in the solar corona Small scale structures in the solar corona

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...70...37h&link_type=abstract

Space Science Reviews, Volume 70, Issue 1-2, pp. 37-46

Physics

6

Solar Corona, Solar Wind, Small Scale Structures

Scientific paper

The observational characteristics of the small scale magnetic structures are summarized. The temperature structure and temporal variability of the emission from coronal bright points, that pervade the source region of the solar wind in coronal holes and the quiet sun, and from active regions are shown to be remarkably similar. Particular emphasis is given to observations, potentially feasible with SOHO, that could resolve some of the outstanding issues regarding the role of the small scale magnetic structures in the energy balance and properties of the solar wind.

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