The total brightness of the solar corona during the eclipse June 21ST it 2001

被引:0
作者
Pintér, T [1 ]
Klocok, L [1 ]
Minarovjech, M [1 ]
Rybansky, M [1 ]
机构
[1] Slovak Cent Observ, Hurbanovo 94701, Slovakia
来源
SOLAR VARIABILITY AS AN INPUT TO THE EARTH'S ENVIRONMENT | 2003年 / 535卷
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The total brightness of the white-light corona in the standart region (1.03-6.00 R-o) alter during the solar activity cycle in relation 1:3 [3]. We have used for its determination during the 2001 solar eclipse a calibrated photographic observation. We obtained a value 1.15x10(-6) of the total blightness of the Sun in the same spectral region.
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页码:243 / 245
页数:3
相关论文
共 5 条
[1]  
PIERCE AK, 1977, SOL PHYS, V51, P25, DOI 10.1007/BF00240442
[2]  
RUSIN V, 1985, B ASTRON I CZECH, V36, P77
[3]  
RYBANSKY M, 1975, B ASTRON I CZECH, V26, P206
[4]  
RYBANSKY M, 1985, B ASTRON I CZECH, V36, P73
[5]  
WALDMEIER M, 1963, SOLAR CORONA, P129