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On the nature of the correlation between cosmic-ray intensity and cloud cover

โœ Scribed by A. W. Wolfendale; G. Gyalai; A. D. Erlykin; K. Kudela; T. Sloan


Book ID
111501310
Publisher
Allerton Press Inc
Year
2009
Tongue
English
Weight
177 KB
Volume
73
Category
Article
ISSN
1062-8738

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๐Ÿ“œ SIMILAR VOLUMES


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โœ B. Trumpy; H. Trefall ๐Ÿ“‚ Article ๐Ÿ“… 1953 ๐Ÿ› Elsevier Science โš– 504 KB

The results of continuous registrations of different components of cosmic rays in the years 1950-1952 are reported. The cosmic ray intensity at sea level is correlated with the air pressure, the height of the 100 mb level and the temperature just below this level. The barometric coefficient a, the h

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Data of cosmic-ray intensity from the Calgary Super Neutron Monitor and interplanetary plasma and field data are divided into three groups corresponding to the magnetic clouds preceded by shocks, followed by interaction region and clouds without any such association, observed during the period 1967-