Coronal Morphology and Heating Mechanism Observations at Total Eclipses Through 1992
Abstract
The author describes the change of overall coronal morphology over the sunspot cycle, using most recently the total eclipse of 30 June 1992. He describes a series of eclipse observations meant to test a model of coronal heating via surface Alfvén waves by searching for 1 Hz coronal oscillations in coronal loops in the green line.
- Publication:
-
IAU Colloq. 144: Solar Coronal Structures
- Pub Date:
- 1994
- Bibcode:
- 1994scs..conf..523P
- Keywords:
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- Solar Eclipses: Solar Corona;
- Morphology: Solar Corona;
- Heating: Solar Corona;
- Solar Eclipses: 1992 June 30