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The spectrum of solar cosmic rays: Data of observations and numerical simulation

✍ Scribed by Yu. V. Balabin; É. V. Vashenyuk; O. V. Mingalev; A. I. Podgorny; I. M. Podgorny

Book ID
110144208
Publisher
Springer
Year
2005
Tongue
English
Weight
194 KB
Volume
49
Category
Article
ISSN
1063-7729

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✍ S. R. Kane; J. R. Winckler 📂 Article 📅 1969 🏛 Springer 🌐 English ⚖ 727 KB

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 • 10 -8 ergscm-es