ALIGNMENT OF RADIO, SOFT-X-RAY, HARD X-RAY IMAGES OF SOURCES IN IMPULSIVE AND GRADUAL PHASES OF THE FLARE OF 1992 AUGUST 17-18

被引:0
作者
ENOME, S
NAKAJIMA, H
SHIBASAKI, K
NISHIO, M
TAKANO, T
HANAOKA, Y
TORII, C
SHIOMI, Y
SEKIGUCHI, H
BUSHIMATA, T
KAWASHIMA, S
SHINOHARA, N
IRIMAJIRI, Y
KOSHIISHI, H
CHOI, YS
SAKAI, J
TAKAHASHI, M
TAKAKURA, T
SAKAO, T
KOSUGI, T
机构
[1] COMMUN RES LABS,KOGANEI,TOKYO 184,JAPAN
[2] UNIV TOKYO,SCH SCI,DEPT ASTRON,BUNKYO KU,TOKYO 113,JAPAN
[3] TOKAI UNIV,DEPT ENGN,HIRATSUKA,KANAGAWA 25912,JAPAN
[4] TOKAI UNIV,DEPT PHYS,HIRATSUKA,KANAGAWA 25912,JAPAN
[5] NATL ASTRON OBSERV,MITAKA,TOKYO 181,JAPAN
关键词
SUN; FLARE; RADIO RADIATION; X-RAYS;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This is a preliminary report concerning an impulsive flare, which occurred on 1992 August 17-18, and was observed with the Nobeyama Radioheliograph, Yohkoh, and ground-based instruments. Emphasis is put on the alignment of radio images as well as soft X-ray and hard X-ray maps, which axe compared in both impulsive and gradual phases. In the impulsive phase, which continued for about 30 s, nonthermal emission was most remarkable at 17 GHz, and was also seen in hard X-rays at the southern part of the SXT source, which was about 14'' width and 80'' long, extending in the north-east to south-west direction. Thermal emission was detected in soft X-rays and possibly in hard X-rays at the northern Part. During the gradual phase, about 80 s after the onset of the impulsive phase, thermal emission dominated and was located at the northern part of the source over the entire energy range. Difficulties are discussed concerning a possible simple topology of the.magnetic fields.
引用
收藏
页码:L27 / L31
页数:5
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