๐”– Bobbio Scriptorium
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Further Observations of the March 1991 Solar Flare Event

โœ Scribed by T.R. Sanderson; R.G. Marsden; K-P. Wenzel

Book ID
107937149
Publisher
Elsevier Science
Year
1993
Tongue
English
Weight
77 KB
Volume
13
Category
Article
ISSN
0273-1177

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๐Ÿ“œ SIMILAR VOLUMES

The white-light solar flare of March 27,
The white-light solar flare of March 27, 1991
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A white-light flare (WLF) was recorded on March 27, 1991 at Tashkent. The WLF occurred at the penumbra of a large, complex sunspot group. The energy released by the WLF per unit time was 2.4 โ€ข 10 ~ erg s -~ .

Observations of energetic X-rays and sol
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On 23 May 1967 energetic (10-50 kcV) solar flare X-rays were observed by the OGO-III ion chamber during the period 1808-2100 UT. The time-intensity profile for the X-ray event showed three distinct pcaks at ~: 1810, 1841 and 1942 UT. The second peak, which is eqtfivalent to ~-: 2.9 โ€ข 10 -8 ergscm-es