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Latitudinal and solar-cycle dependence of the interplanetary magnetic field predominant polarity

✍ Scribed by Xenophon Moussas; Basil Tritakis

Publisher
Springer
Year
1982
Tongue
English
Weight
670 KB
Volume
75
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES

A solar cycle variation of the interplan
A solar cycle variation of the interplanetary magnetic field
✍ G. L. Siscoe; N. U. Crooker; L. Christopher πŸ“‚ Article πŸ“… 1978 πŸ› Springer 🌐 English βš– 693 KB

Measurements of the north-south (Bz) component of the interplanetary field as compiled by King (1975) when organized into yearly histograms of the values of IBz[ reveal the following. (1) The histograms decrease exponentially from a maximum occurrence frequency at the value IBz I = 0. (2) The slope

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✍ Basil P. Tritakis πŸ“‚ Article πŸ“… 1979 πŸ› Springer 🌐 English βš– 357 KB

The representation of the sector boundaries, published by Svalgaard (1974Svalgaard ( , 1975) ) in a superposed 27-days Bartels format showed that they have a significant preference to occur in certain days of the solar rotation. Further study of these data, as well as of the polarized days in the vi

Possible use of (a) solar faculae and (b
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✍ G. M. Brown πŸ“‚ Article πŸ“… 1981 πŸ› Springer 🌐 English βš– 250 KB

Two independent methods of predicting the magnitude of the peak of a forthcoming sunspot cycle are summarized. One is based on considerations of the development of spots relative to the area of the faculae within which they form during the early stages of the cycle in question, and gives a lead-time