On the 11-years cycle of solar activity
β Scribed by M. N. Gnevyshev
- Publisher
- Springer
- Year
- 1967
- Tongue
- English
- Weight
- 676 KB
- Volume
- 1
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
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 corpuscular emissions take part in these two processes.
Events taking place in the magnetosphere, ionosphere, troposphere and perhaps some chemical and biological events reflect the essential properties of the 11-years cycle.
π SIMILAR VOLUMES
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
## Abstract The main aim of the present study is to investigate further the association between total ozone (TOZ) and the 11 year solar cycle (SC) during the period 1979β2010, by employing satellite observations of TOZ made by Nimbusβ7, Meteorβ3, Earth Probe Total Ozone Mapping Spectrometer (TOMS)