Simultaneous observation of a Moreton wave on 1997 November 3 in Hα and soft X-rays

被引:93
作者
Narukage, N [1 ]
Hudson, HS
Morimoto, T
Akiyama, S
Kitai, R
Kurokawa, H
Shibata, K
机构
[1] Kyoto Univ, Kwasan Observ, Kyoto 6078471, Japan
[2] Kyoto Univ, Hida Observ, Kyoto 6078471, Japan
关键词
shock waves; Sun : chromosphere; Sun : corona; Sun : flares; Sun : magnetic fields;
D O I
10.1086/341599
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the observation of a Moreton wave in Halpha (line center and +/-0.8 Angstrom) with the Flare Monitoring Telescope at the Hida Observatory of Kyoto University at 4:36-4:41 UT on 1997 November 3. The same region (NOAA Active Region 8100) was simultaneously observed in soft X-rays with the soft X-ray telescope on board Yohkoh, and a wavelike disturbance ("X-ray wave") was also found. The position of the wave front as well as the direction of propagation of the X-ray wave roughly agree with those of the Moreton wave. The propagation speeds of the Moreton wave and the X-ray wave are about 490+/-40 and 630+/-100 km s(-1), respectively. Assuming that the X-ray wave is an MHD fast-mode shock, we can estimate the propagation speed of the shock, on the basis of MHD shock theory and the observed soft X-ray intensities ahead of and behind the X-ray wave front. The estimated fast shock speed is 400-760 km s(-1), which is in rough agreement with the observed propagation speed of the X-ray wave. The fast-mode Mach number of the X-ray wave is also estimated to be about 1.15-1.25. These results suggest that the X-ray wave is a weak MHD fast-mode shock propagating through the corona and hence is the coronal counterpart of the Moreton wave.
引用
收藏
页码:L109 / L112
页数:4
相关论文
共 19 条
[1]   The rate of magnetic reconnection observed in the solar atmosphere [J].
Dere, KP .
ASTROPHYSICAL JOURNAL, 1996, 472 (02) :864-873
[2]  
ETO S, 2002, IN PRESS PASJ
[3]   RADIO EVIDENCE OF DIRECTIVE SHOCK-WAVE PROPAGATION IN SOLAR CORONA [J].
KAI, K .
SOLAR PHYSICS, 1969, 10 (02) :460-&
[4]   X-ray observations of a large-scale solar coronal shock wave [J].
Khan, JI ;
Aurass, H .
ASTRONOMY & ASTROPHYSICS, 2002, 383 (03) :1018-1031
[5]   Homologous sudden disappearances of transequatorial interconnecting loops in the solar corona [J].
Khan, JI ;
Hudson, HS .
GEOPHYSICAL RESEARCH LETTERS, 2000, 27 (08) :1083-1086
[6]   Catalogue of the 1997 SOHO-EIT coronal transient waves and associated type II radio burst spectra [J].
Klassen, A ;
Aurass, H ;
Mann, G ;
Thompson, BJ .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 2000, 141 (03) :357-369
[7]   Observations of solar H alpha filament disappearances with a new solar flare-monitoring telescope at Hida Observatory [J].
Kurokawa, H ;
Ishiura, K ;
Kimura, G ;
Nakai, Y ;
Kitai, R ;
Funakoshi, Y ;
Shinkawa, T .
JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY, 1995, 47 (11) :1043-1052
[8]  
Mann G, 1999, ESA SP PUBL, V446, P477
[9]   H-ALPHA OBSERVATIONS OF FLARE-INITIATED DISTURBANCES WITH VELOCITIES - 1000 KM/SEC [J].
MORETON, GE .
ASTRONOMICAL JOURNAL, 1960, 65 (09) :494-495
[10]  
Priest E, 1982, SOLAR MAGNETOHYDRODY