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The differences in the relationship between ionospheric critical frequencies and sunspot number for different sunspot cycles

✍ Scribed by Ostrow, S. M.; PoKempner, M.

Book ID
119721985
Publisher
American Geophysical Union
Year
1952
Tongue
English
Weight
304 KB
Volume
57
Category
Article
ISSN
0148-0227

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## Abstract Duration of the extended solar cycles is taken into the consideration. The beginning of cycles is counted from the moment of polarity reversal of large‐scale magnetic field in high latitudes, occurring in the sunspot cycle n till the minimum of the cycle __n__ + 2. The connection betwee