国家重点基础研究发展计划(G2006CB806303)

作品数:6被引量:5H指数:2
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相关期刊:《Research in Astronomy and Astrophysics》《Science China(Physics,Mechanics & Astronomy)》更多>>
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Two types of dynamic cool coronal structures observed with STEREO and Hinode
《Research in Astronomy and Astrophysics》2009年第12期1368-1376,共9页Jun Zhang Le-Ping Li 
supported by the National Natural Science Foundation of China(Grant Nos.40890161 and 40674081);the CAS Project KJCX2-YW-T04,and the National Basic Research Program of China(Grant No.G2006CB806303)
Solar coronal loops show significant plasma motions during their formation and eruption stages. Dynamic cool coronal structures, on the other hand, are often observed to propagate along coronal loops. We report on the...
关键词:Sun: chromosphere -- Sun: UV radiation -- Sun: activity 
Emergence and cancellation of small-scale magnetic flux in a quiet region被引量:2
《Science China(Physics,Mechanics & Astronomy)》2009年第11期1691-1695,共5页ZHANG Jun JIN ChunLan 
Supported by the National Natural Science Foundation of China (Grant Nos. G10573025, 10873020, 10603008, 40890161, 10733020, 40674081,and 10703007);the CAS Project (Grant No. KJCX2-YW-T04);the National Basic Research Program of China (Grant No. G2006CB806303)
This paper studies the relationship between the development of granules and emergence (cancellation) of magnetic flux at small spatial scales (~1″) in a quiet region taken with the spectro-polarimeter (SP) of the So...
关键词:photosphere magnetic FIELDS polarimetric evolution EMERGENCE 
Chromospheric oscillations observed with BBSO and TRACE被引量:2
《Science China(Physics,Mechanics & Astronomy)》2009年第11期1718-1722,共5页SONG Qiao ZHANG Jun 
Supported by the National Natural Science Foundation of China (Grant Nos. G10873020, 10603008, 40890161, 10703020, 40674081, and10703007);the CAS Project (Grant No. KJCX2-YW-T04);the National Basic Research Program of China (Grant No. G2006CB806303)
We examine chromospheric oscillations in both a coronal hole (CH) and a quiet Sun (QS) region, by employing Transition Region and Coronal Explorer (TRACE) and Big Bear Solar Observatory (BBSO) data on September 14 and...
关键词:CHROMOSPHERE OSCILLATIONS UV radiation magnetic fields QUIET Sun CORONAL hole 
A statistical study on the brightening propagation of post-flare loops被引量:3
《Science China(Physics,Mechanics & Astronomy)》2009年第11期1723-1727,共5页LI LePing DUAN HongYu ZHANG Jun 
Supported by the National Natural Science Foundation of China (Grant Nos. G10703007, 40890161, 10603008, 40674081, and 10733020);the CAS Project (Grant No. KJCX2-YW-T04);the National Basic Research Program of China (Grant No. G2006CB806303)
After examining the data observed by TRACE 171 and 195  from May 1998 to December 2006, we choose as our sample 190 (39 X-class and 151 M-class) flare events which display post-flare loops (PFLs). We investigate the...
关键词:FLARES magnetic FIELDS CORONA UV radiation 
Magnetic non-potentiality on the quiet Sun and the filigree被引量:3
《Research in Astronomy and Astrophysics》2009年第8期933-944,共12页Meng Zhao Jing-Xiu Wang Chun-Lan Jin Gui-Ping Zhou 
supported by the National Natural Science Foundation of China (10873020, 10703007, G10573025, 40674081, 10603008, 10733020 and 40890161);the Chinese Academy of Sciences Project KJCX2-YW-T04;the National Basic Research Program of China(G2006CB806303)
From the observed vector magnetic fields by the Solar Optical Telescope/ Spectro-Polarimeter aboard the satellite Hinode, we have examined whether or not the quiet Sun magnetic fields are non-potential, and how the G-...
关键词:SUN magnetic fields -- Sun photosphere -- Sun network bright point 
Flare-induced signals in polarization measurements during the X2.6 flare on 2005 January 15
《Research in Astronomy and Astrophysics》2009年第7期812-828,共17页Meng Zhao Jing-Xiu Wang Sarah Matthews Ming-De Ding Hui Zhao Chun-Lan Jin 
supported by the National Natural Science Foundation of China (10873020,10703007,G10573025, 40674081and 10603008);the CAS Project KJCX2-YW-T04;the National Basic Research Program of China (G2006CB806303)
Flare-induced signals in polarization measurements which were manifested as apparent polarity reversal in magnetograms have been reported since 1981. We are motivated to further quantify the phenomenon by asking two q...
关键词:Sun: magnetic field - Sun: flare - Sun: activity 
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