ONGOING PARTIAL RECONNECTION IN A LIMP FLARE

被引：14

作者：

DEJAGER, C

INDAKOIDE, M

KOIDE, S

SAKAI, J

机构：

来源：

SOLAR PHYSICS | 1995年 / 158卷 / 02期

关键词：

D O I：

10.1007/BF00795673

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The limb flare on August 2, 1993 08:30 UT, consisting of two crossed loops, shows evidence of partial X-type reconnection. The observations suggest that partial reconnection was an ongoing process during about 10 min until flare ignition.

引用

页码：391 / 394

页数：4

共 5 条

[1]

HARA M, 1992, PUBLIC ASTRON SOC, V44, pL135

[2]

Mewe R., 1985, Astronomy & Astrophysics Supplement Series, V62, P197

[3]

SAKAI JI, 1995, IN PRESS SOLAR PHYS, V156

[4] THE SOFT-X-RAY TELESCOPE FOR THE SOLAR-A MISSION [J].

TSUNETA, S ;

ACTON, L ;

BRUNER, M ;

LEMEN, J ;

BROWN, W ;

CARAVALHO, R ;

CATURA, R ;

FREELAND, S ;

JURCEVICH, B ;

MORRISON, M ;

OGAWARA, Y ;

HIRAYAMA, T ;

OWENS, J .

SOLAR PHYSICS, 1991, 136 (01) :37-67

[5] CHARACTERISTICS OF PLASMA TEMPERATURE-VARIATION DURING 2-CURRENT-LOOP COLLISIONS [J].

ZHAO, J ;

CHARGEISHVILI, B ;

SAKAI, J .

SOLAR PHYSICS, 1993, 147 (01) :131-136

← 1 →