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 |
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| container_end_page | 664 |
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| container_issue | 2 |
| container_start_page | 654 |
| container_title | The Astrophysical journal |
| container_volume | 358 |
| creator | Schmahl, E. J. Kundu, M. R. Schmelz, J. T. Saba, J. L. R. Strong, K. T. |
| description | 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. |
| doi_str_mv | 10.1086/169018 |
| format | Article |
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J.</creatorcontrib><creatorcontrib>Kundu, M. R.</creatorcontrib><creatorcontrib>Schmelz, J. T.</creatorcontrib><creatorcontrib>Saba, J. L. R.</creatorcontrib><creatorcontrib>Strong, K. T.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Schmahl, E. J.</au><au>Kundu, M. R.</au><au>Schmelz, J. T.</au><au>Saba, J. L. R.</au><au>Strong, K. T.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Microwave and X-ray observations of a major confined solar flare</atitle><jtitle>The Astrophysical journal</jtitle><date>1990-08-01</date><risdate>1990</risdate><volume>358</volume><issue>2</issue><spage>654</spage><epage>664</epage><pages>654-664</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>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.</abstract><cop>Legacy CDMS</cop><pub>University of Chicago Press</pub><doi>10.1086/169018</doi><tpages>11</tpages></addata></record> |
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| ispartof | The Astrophysical journal, 1990-08, Vol.358 (2), p.654-664 |
| issn | 0004-637X 1538-4357 |
| language | eng |
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| source | NASA Technical Reports Server; Alma/SFX Local Collection |
| subjects | 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 |
| title | Microwave and X-ray observations of a major confined solar flare |
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