Propagating Slow Magnetoacoustic Waves along the Continuous Outflows Observed with EIS/Hinode

被引:0
|
作者
Nishizuka, Naoto [1 ]
Matsumoto, Takuma [1 ]
Morita, Satoshi [1 ]
Hara, Hirohisa
Shibata, Kazunari [1 ]
机构
[1] Kyoto Univ, Kwasan Observ, Kyoto 6068501, Japan
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关键词
LONGITUDINAL INTENSITY OSCILLATIONS; EUV IMAGING SPECTROMETER; ACTIVE-REGION; CORONAL LOOPS; SPECTROSCOPIC OBSERVATIONS; MAGNETIC-FIELDS; SOLAR-WIND; HINODE; TRACE; BRIGHTENINGS;
D O I
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The high temporal relation data obtained from EIS/Hinode has been analyzed. In the 'sit-and-stare' mode observations, we focused on continuous outflows at the edge of the active region NOAA 10942 on 2007 February 20. We found that the Doppler blueshift (similar to 20-50 km s(-1)) components, in Fe XII 195 angstrom emission line, propagating with the continuous plasma outflows from the edge of the active region, with the transverse velocity ranging 140-160 km s(-1). This suggests slow magnetoacoustic wave propagation along the open field line. We also found a jet around the active region, whose transverse velocity similar to 170 km s(-1) and line-of-sight Doppler velocity similar to 150 km s(-1).
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页码:157 / 161
页数:5
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