Cyclical Behavior of Magnetically Complex Sunspot Groups and Major Flares in Solar Cycles 22 – 24
Author:
Funder
Applied Basic Research Foundation of Yunnan Province
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s11207-022-01965-y.pdf
Reference46 articles.
1. Akasofu, S.-I.: 1984, An essay on sunspots and solar flares. Planet. Space Sci. 32, 1469. DOI. ADS.
2. Babcock, H.W.: 1961, The topology of the Sun’s magnetic field and the 22-year cycle. Astrophys. J. 133, 572. DOI. ADS.
3. Brandenburg, A.: 2005, The case for a distributed solar dynamo shaped by near-surface shear. Astrophys. J. 625, 539. DOI. ADS.
4. Choudhuri, A.R.: 1990, On the possibility of an alpha 2 omega – type dynamo in a thin layer inside the Sun. Astrophys. J. 355, 733. DOI. ADS.
5. Clette, F., Svalgaard, L., Vaquero, J.M., Cliver, E.W.: 2014, Revisiting the sunspot number. A 400-year perspective on the solar cycle. Space Sci. Rev. 186, 35. DOI. ADS.
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