Statistical analysis of soft x-ray flares during the 23rd solar cycle

被引：0
作者：
Tang, Y. Q. [1 ]
Le, G. M. [1 ]
机构：
[1] China Meteorol Adm, Natl Ctr Space Weather Monitor & Forecast, Beijing 100084, Peoples R China
来源：
Proceedings of the 29th International Cosmic Ray Conference Vol 1: SH1 and SH2 | 2005年
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
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页码：5 / 8
页数：4
相关论文
共 6 条
[1]   DISTRIBUTION OF FLARES ON THE SUN DURING 1955-1985 - HOT SPOTS (ACTIVE ZONES) LASTING FOR 30 YEARS [J].
BAI, T .
ASTROPHYSICAL JOURNAL, 1988, 328 (02) :860-&
[2]   EVIDENCE FOR SOLAR-CYCLE EVOLUTION OF NORTH SOUTH FLARE ASYMMETRY DURING CYCLES 20 AND 21 [J].
GARCIA, HA .
SOLAR PHYSICS, 1990, 127 (01) :185-197
[3]   ASYMMETRIES DURING THE MAXIMUM PHASE OF SOLAR-CYCLE-22 [J].
JOSHI, A .
SOLAR PHYSICS, 1995, 157 (1-2) :315-324
[4]   Statistical analysis of the X-ray flares (M≥1) during the maximum period of solar cycle 22 [J].
Li, KJ ;
Schmieder, B ;
Li, QS .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1998, 131 (01) :99-104
[5]   NORTH-SOUTH DISTRIBUTION OF MAJOR SOLAR-FLARE EVENTS, SUNSPOT MAGNETIC CLASSES AND SUNSPOT AREAS (1955-1974) [J].
ROY, JR .
SOLAR PHYSICS, 1977, 52 (01) :53-61
[6]  
Temmer M, 2002, ESA SP PUBL, V477, P175
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