๐”– Bobbio Scriptorium
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Essential features of the 11-year solar cycle

โœ Scribed by M. N. Gnevyshev

Publisher
Springer
Year
1977
Tongue
English
Weight
474 KB
Volume
51
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES

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โœ M. N. Gnevyshev ๐Ÿ“‚ Article ๐Ÿ“… 1967 ๐Ÿ› Springer ๐ŸŒ English โš– 676 KB

Each 11-years cycle of solar activity consists of two processes with different physical properties. The variety of shapes of the 11-years curves depends on the way these processes overlap. All events in the photosphere, chromosphere and corona, and all kinds of emissions like the radio-and corpuscu

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The synodic rotation period and power spectra of solar microwave sources are investigated using acctlrate data in the interval 1956 to 1970. The variation of the approximate 27 day period is obtained over a complete solar cycle and is thought to be a result of the latitude change over the solar cycl

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โœ H. Daene ๐Ÿ“‚ Article ๐Ÿ“… 2007 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 369 KB

With 3 figures. (Received 196G October IS) I t is shown from measurements of type I11 bursts a t 234 MHz, I I I MHz and 23 MHz during the foregoing solar cycle that the type I11 activity has a relative minimum in 1959 and apparently a second maximum in 1960. This is in accordance with the statement