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

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 structu...

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Veröffentlicht in:	The Astrophysical journal 1990-08, Vol.358 (2), p.654-664
Hauptverfasser:	Schmahl, E. J., Kundu, M. R., Schmelz, J. T., Saba, J. L. R., Strong, K. T.
Format:	Artikel
Sprache:	eng
Schlagworte:	640104 - Astrophysics & Cosmology- Solar Phenomena Astronomy CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC RADIO SOURCES Earth, ocean, space ELECTROMAGNETIC RADIATION ENERGY LOSSES Exact sciences and technology Flares, bursts, and related phenomena IONIZING RADIATIONS LOSSES MICROWAVE RADIATION MICROWAVE SPECTRA MORPHOLOGY RADIATIONS SOLAR ACTIVITY SOLAR FLARES Solar Physics Solar system SPECTRA X RADIATION
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