Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986tuft.rept.....l&link_type=abstract
Annual Report, 1 Sep. 1985 - 30 Oct. 1986 Tufts Univ., Medford, MA. Dept. of Physics and Astronomy.
Astronomy and Astrophysics
Astronomy
Antenna Arrays, Coronal Loops, Magnetic Fields, Solar Activity, Solar Maximum Mission, Very Large Array (Vla), Cyclotron Radiation, Field Strength, Microwaves, Plasma Interactions, Solar Prominences
Scientific paper
The research deals mainly with Very Large Array and Solar Maximum Mission observations of the ubiquitous coronal loops that dominate the structure of the low corona. As illustrated, the observations of thermal cyclotron lines at microwave wavelengths provide a powerful new method of accurately specifying the coronal magnetic field strength. Processes are delineated that trigger solar eruptions from coronal loops, including preburst heating and the magnetic interaction of coronal loops. Evidence for coherent burst mechanisms is provided for both the Sun and nearby stars, while other observations suggest the presence of currents that may amplify the coronal magnetic field to unexpectedly high levels. The existence is reported of a new class of compact, variable moving sources in regions of apparently weak photospheric field.
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