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The Filament Eruption in the 3B Flare of July 29, 1973: Onset and Magnetic Field Configuration

  • Moore R
  • Labonte B
Symposium - International Astronomical Union (1980) 91 207-211
DOI: 10.1017/s0074180900067589
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Abstract

We present direct observational evidence for the preflare magnetic field configuration, the nature of the filament destabilization and triggering of the flare, and the magnetic field configuration after the filament eruption in the large, well-ordered, expanding two-ribbon flare of July 29, 1973.

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Moore, R. L., & Labonte, B. J. (1980). The Filament Eruption in the 3B Flare of July 29, 1973: Onset and Magnetic Field Configuration. Symposium - International Astronomical Union, 91, 207–211. https://doi.org/10.1017/s0074180900067589

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