The energetics and mass transfer during the X-ray flare of 18:31 GMT on 5 September, 1973 have been studied using the observations in the objective grating mode of the AS&E X-ray spectrographic telescope on Skylab. The flare was a moderately energetic one, Class M1 according to Solrad. In Ha, howeve
Flare parameters for the 7 September, 1973 two-ribbon flare
โ Scribed by J. G. Doyle; J. C. Raymond
- Book ID
- 104645400
- Publisher
- Springer
- Year
- 1984
- Tongue
- English
- Weight
- 748 KB
- Volume
- 90
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
A study is made of the relative importance of the various energy loss mechanisms for the long-decay event of 7 September, 1973, using spectral scans in the 400/~-1335/~ range. This spectral range contains many of the important electron density and temperature diagnostic line ratios for the solar transition zone. We refine earlier analyses of the flare energy budget using more detailed emission measure curves and density diagnostics. We examine the constant pressure assumptions used in both coronal loop models and in the interpretation of observations in terms of flare energetics. We find that much of the upper transition region emission originates in cooling loops. Radiative losses are found to dominate.
๐ SIMILAR VOLUMES
We present high resolution detailed observations of the class 3N two-ribbon flare of 1973, July 29 (McMath 12461), which was associated with the disappearance of a large filament ('disparition brusque'). This flare occurred in a diffuse bipolar magnetic region completely devoid of sunspots, and was