Progress in coronal physics

Details Progress in coronal physics Progress in coronal physics

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..100..281z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 100, Oct. 1985, p. 281-287.

Physics

4

Solar Activity, Solar Corona, Solar Physics, Stellar Mass Ejection, Atmospheric Heating, Coronal Holes, Coronal Loops, Flow Stability, Solar Magnetic Field, Solar Wind Velocity, Stellar Models

Scientific paper

This paper reviews research highlights of the past five years. Considerable progress has been made in observing and interpreting coronal mass ejections. The stability of coronal loops is much better understood and new observations of the onset of wind streams in coronal holes have been made. Observations from the Solar Maximum Mission should help to clarify the physics of the active corona. The mechanisms that heat the corona and accelerate the high-speed wind streams remain to be identified however.

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