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Solar wind properties obtained from the study of the 11-year cosmic-ray cycle: 1

✍ Scribed by Dorman, I. V.; Dorman, L. I.


Book ID
119727041
Publisher
American Geophysical Union
Year
1967
Tongue
English
Weight
652 KB
Volume
72
Category
Article
ISSN
0148-0227

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The cosmic-ray 1.68-year variation: A cl
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Using the maximum entropy method (MEM), the cosmic-ray power spectral density in the frequency range 3 x 10-9-2 β€’ 10-Hz has been estimated for the period . Cosmic-ray intensity data were integrated from the ion chamber at Huancayo and the neutron monitor at Deep River, following the method of Nagash