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Interplanetary sector structure in the rising portion of the sunspot cycle

✍ Scribed by Wilcox, John M.; Colburn, David S.

Book ID
119709942
Publisher
American Geophysical Union
Year
1969
Tongue
English
Weight
528 KB
Volume
74
Category
Article
ISSN
0148-0227

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πŸ“œ SIMILAR VOLUMES

Solar source of the interplanetary secto
Solar source of the interplanetary sector structure
✍ John M. Wilcox; Norman F. Ness πŸ“‚ Article πŸ“… 1967 πŸ› Springer 🌐 English βš– 846 KB

The interplanetary sector structure observed by the IMP-1 satellite during three solar rotations in 1963-4 is compared with the photospheric magnetic field structure observed with the solar magnetograph at Mt. Wilson Observatory. The interplanetary sector structure was most prominent on the sun in l

Predicting the maximum amplitude for the
Predicting the maximum amplitude for the sunspot cycle from the rate of rise in sunspot number
✍ Robert M. Wilson πŸ“‚ Article πŸ“… 1988 πŸ› Springer 🌐 English βš– 420 KB

Examined are associational aspects as they relate the maximum amplitude R M for the sunspot cycle to the rate of rise Ral during the ascending phase, where R M is the smoothed sunspot number at cycle maximum and Rat is the sum of the monthly mean sunspot numbers for selected 6-month intervals (At) m