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Features of the Gnevyshev-Waldmeier Rule for Various Lifetimes and Areas of Sunspot Groups
- Source :
- Astronomy Letters. 45:695-699
- Publication Year :
- 2019
- Publisher :
- Pleiades Publishing Ltd, 2019.
-
Abstract
- Based on a sample of 7696 nonrecurrent and 566 recurrent sunspot groups, we have investigated the Gnevyshev–Waldmeier rule using the Catalogue of Solar Activity by R.S. Gnevysheva (1954–1978). The maximum recorded sunspot group lifetime is 160 days. The general Gnevyshev–Waldmeier rule for all lifetimes is Amax = (12.1 ± 0.70)LT (Amax is the maximum sunspot group area during the lifetime and LT is the sunspot group lifetime). However, the general rule has turned out to deviate from the derived linear form for the population of small short-living sunspot groups (SSG): it has a significant nonlinear scaling form Amax = (8.02 ± 0.41)LT(1.105±0.022). For the population of large long-living sunspot groups (LLG) there is a linear form Amax = (12.9 ± 1.1)LT. Allowance only for recurrent sunspot groups with lifetimes more than 40 days gives Amax = (13.93 ± 0.41)LT.
- Subjects :
- Physics
Sunspot
education.field_of_study
Nonlinear scaling
010308 nuclear & particles physics
Group (mathematics)
AMAX
Population
Astronomy and Astrophysics
Allowance (engineering)
Astrophysics
01 natural sciences
Space and Planetary Science
0103 physical sciences
education
010303 astronomy & astrophysics
Subjects
Details
- ISSN :
- 15626873 and 10637737
- Volume :
- 45
- Database :
- OpenAIRE
- Journal :
- Astronomy Letters
- Accession number :
- edsair.doi...........f8d1ed875c3ebb7493fc890499456328
- Full Text :
- https://doi.org/10.1134/s1063773719100050