The Contribution of Large Recurrent Sunspot Groups to Solar Activity: Empirical Evidence
We identify large sunspot nestlets (SN) mostly containing recurrent sunspot groups and investigate the indices of solar activity defined as the 11- or 22-year moving average of the daily areas of the SN. These nestlets, 667 in total, are constructed from the daily 1874–2020 RGO/SOON catalogue, which...
Main Author: | Alexander Shapoval |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2022-03-01
|
Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/8/3/180 |
Similar Items
-
Recurrent Large Sunspot Structures and 27-Day Component of Solar Activity as Proxies to Axis-Nonsymmetry
by: Alexander Shapoval, et al.
Published: (2023-06-01) -
Charting the solar cycle
by: S. C. Chapman, et al.
Published: (2023-02-01) -
An Automatic Approach for Grouping Sunspots and Calculating Relative Sunspot Number on SDO/HMI Continuum Images
by: Cui Zhao, et al.
Published: (2024-01-01) -
Extending the sunspot area series from Kodaikanal Solar Observatory
by: Bibhuti Kumar Jha, et al.
Published: (2022-10-01) -
Evolutionary Relationship between Sunspot Groups and Soft X-Ray Flares over Solar Cycles 21–25
by: Jiaqi Lin, et al.
Published: (2023-01-01)