Hostname: page-component-8448b6f56d-wq2xx Total loading time: 0 Render date: 2024-04-24T17:20:03.076Z Has data issue: false hasContentIssue false

The Distribution of Sunspot Decay Rates

Published online by Cambridge University Press:  12 April 2016

V. Martínez Pillet
Affiliation:
Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
F. Moreno-Insertis
Affiliation:
Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
M. Vázquez
Affiliation:
Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The distribution of sunspot decay rates is studied using the Greenwich Photoheliographic Results (GPR). The decay rates are seen to be lognormally distributed. An analysis of the lognormal distributions associated to each sunspot group type and for isolated spots is presented. As a remarkable property of the decay process, we show that it happens at a constant total to umbral area ratio.

Type
Session 1. Structure of Active Regions
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Bumba, V.: 1963, Bull. astr. Inst. Czech., 14, 91 Google Scholar
Gokhale, M.H., and Zwaan, C.: 1972, Solar Phys., 26, 52 Google Scholar
Harvey, K., and Harvey, J.: 1973, Solar Phys., 28, 61 Google Scholar
Howard, R.F.: 1992, Solar Phys., 137, 51 Google Scholar
Meyer, F., Schmidt, H.U., Weiss, N.O., and Wilson, P.R.: 1974, M.N.R.A.S., 169, 35 Google Scholar
Moreno-Insertis, F., and Vázquez, M.: 1988, Astr. Ap., 205, 289 Google Scholar
Schmidt, H.U.: 1968, in Kipenheuer, K.O. (ed.), Structure and Development of Solar Active Regions, Reidel, Dordrecht Google Scholar
Simon, G. W., and Leighton, R.B.: 1964, Ap. J., 140, 1120 Google Scholar