Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..279l&link_type=abstract
In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 279-289 (SEE N87-20871 13-92)
Astronomy and Astrophysics
Astronomy
Coronal Loops, Radio Emission, Solar Magnetic Field, Solar X-Rays, Stellar Atmospheres, High Resolution, Radio Astronomy, Radio Telescopes, X Ray Telescopes
Scientific paper
This is an introduction to this part of the proceedings and an overview of coronal diagnostics. The current understanding of coronal loops is summarized. Included are observations from ground-based radio telescopes and from X ray telescopes lofted above the atmosphere, as well as theoretical interpretations of these observations. Also included in these introductory remarks is a discussion of the three dimensional structure of coronal loops. Alternative radiation mechanisms are then described within the context of both the radio and X ray emission. Various methods of determining the strength and structure of the coronal magnetic field are then described, followed by the coronae of nearby stars and future prospects for radio diagnostic of coronal loops.
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