It is suggested that the experimental data on the solar neutrino flux as measured by Davis and his collaborators from 1970 to 1982 vary with the solar activity cycle to a very high level of statistical significance for all the available tests of the hypothesis (e.g., t-test, z2-test, run test, Wilco
On the proposed associations of solar neutrino flux with solar particles, cosmic rays, and the solar activity cycle
โ Scribed by Robert M. Wilson
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 882 KB
- Volume
- 112
- Category
- Article
- ISSN
- 0038-0938
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The cosmic-ray intensity during the 18th and 19th solar cycles is examined in the light of Gnevyshev's suggestion of the presence of two maxima in each solar cycle. The 18th solar cycle has two prominent and widely separated cosmic-ray minima corresponding in phase with the two maxima in Bartel's Ap
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 โข 10 -8 ergscm-es