The growth of facular area surrounding large, decaying sunspots

被引:4
|
作者
Chapman, G. A. [1 ]
Hoffer, A. S. [1 ]
机构
[1] Calif State Univ Northridge, Dept Phys & Astron, San Fernando Observ, Northridge, CA 91330 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
D O I
10.1007/s11207-006-0118-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In a previous paper, we investigated the facular area around 31 decaying sunspots of varied size. The growth of facular area as a function of spot decay was marginally significant (r(2) = 0.1255, p = 0.05). Using new data, this paper examines the change in facular area surrounding large decaying sunspots some of which grew very rapidly. The data are from full-disk photometric images taken with CFDT2 (2.5 '' pixels). For 10 sunspots, we find a statistically significant increase in facular area as a function of the spot decay rate with a regression coefficient, squared, of r(2) = 0.611 (p < 0.02).
引用
收藏
页码:321 / 328
页数:8
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