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Features of cosmic ray variation at the phase of the minimum between the 23rd and 24th solar cycles

✍ Scribed by G. A. Bazilevskaya; M. B. Krainev; V. S. Makhmutov; A. K. Svirzhevskaya; N. S. Svirzhevsky; Yu. L. Stozhkov


Book ID
111502271
Publisher
Allerton Press Inc
Year
2011
Tongue
English
Weight
147 KB
Volume
75
Category
Article
ISSN
1062-8738

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Analysis of the time series into trigonometric series allows the investigation of cosmic-ray (CR) intensity variations in a range of periodicities from a few days to 1 year. By this technique the amplitude and the phase of all observed uctuations can be given. For this purpose, daily CR intensity va