Microwave and X-ray observations of a major confined solar flare

Details Microwave and X-ray observations of a major confined solar flare Microwave and X-ray observations of a major confined solar flare

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...358..654s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 358, Aug. 1, 1990, p. 654-664. Research supported by the Lockheed Independe

Computer Science

Sound

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Energy Dissipation, Microwave Sounding, Solar Flares, Solar X-Rays, Thermal Energy, Line Spectra, Microwave Spectra, Plasma Temperature, Very Large Array (Vla)

Scientific paper

Observations of an X4 flare of May 19, 1984 using the VLA and the SMM X-ray Polychromator are discussed. The 6 cm radio source remained stationary throughout the decay phase. Combined with other evidence, this indicates that the flare was magnetically confined and did not disrupt the complex structure of its region. The observed structures may be associated with a neutral sheet connecting the two bipoles.

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