Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Tuan-Hui Zhou"'
Publikováno v:
Atmosphere, Vol 12, Iss 9, p 1176 (2021)
Based on the daily sunspot number (SN) data (1954–2011) from the Purple Mountain Observatory, the extreme value theory (EVT) is employed for the research of the long-term solar activity. It is the first time that the EVT is applied on the Chinese S
Externí odkaz:
https://doaj.org/article/f4dd38681dd944a3935879be0a23f280
Publikováno v:
Journal of Astrophysics and Astronomy. 43
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6008e63350e947ac466d3bc72ec8472c
https://doi.org/10.1007/s12036-022-09831-w
https://doi.org/10.1007/s12036-022-09831-w
Publikováno v:
Atmosphere
Volume 12
Issue 9
Atmosphere, Vol 12, Iss 1176, p 1176 (2021)
Volume 12
Issue 9
Atmosphere, Vol 12, Iss 1176, p 1176 (2021)
Based on the daily sunspot number (SN) data (1954–2011) from the Purple Mountain Observatory, the extreme value theory (EVT) is employed for the research of the long-term solar activity. It is the first time that the EVT is applied on the Chinese S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53e57c16424f790c80e4124ceb83cf47
Autor:
Zhi Xu, Zhen-Tong Li, Jian-Chao Xue, Hui Li, Jean-Claude Vial, Tuan-Hui Zhou, Yang Su, Ying-Na Su
Publikováno v:
Research in Astronomy and Astrophysics. 21:222
Prominence plumes are evacuated upflows that emerge from bubbles below prominences, whose formation mechanism is still unclear. Here we present a detailed study of plumes in a quiescent prominence using the high-resolution H-alpha filtergrams at the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ed31a8d7ab0315c992016e906f236c69
https://doi.org/10.1088/1674-4527/21/9/222
https://doi.org/10.1088/1674-4527/21/9/222
Publikováno v:
Research in Astronomy and Astrophysics. 13:961-977
We carry out a detailed analysis of the X3.5 solar flare that occurred on 2002 July 20, which is the strongest partially limb-occulted flare ever observed by the RHESSI satellite. The main results are: (1) during the main impulsive phase that lasts s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7ae165fa8ca7b6bb1d2aba0fe2c7ab5a
https://doi.org/10.1088/1674-4527/13/8/008
https://doi.org/10.1088/1674-4527/13/8/008
Publikováno v:
Research in Astronomy and Astrophysics. 13:526-536
With the aim of studying the relationship between the relative motions of the loop-top (LT) source and footpoints (FPs) during the rising phase of solar flares, we give a detailed analysis of the X7.1 class flare that occurred on 2005 January 20. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::79748c1c81c89d9ac8fb2e2acd07a052
https://doi.org/10.1088/1674-4527/13/5/004
https://doi.org/10.1088/1674-4527/13/5/004
Autor:
Haisheng Ji, Tuan-Hui Zhou
Publikováno v:
Research in Astronomy and Astrophysics. 9:323-332
We give an extensive multi-wavelength analysis of an eruptive M1.0/1N class solar flare, which occurred in the active region NOAA 10044 on 2002 July 26. Our emphasis is on the relationship between magnetic shear and flare shear. Flare shear is define
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e599fa1568f83998ace17719313f5ef5
https://doi.org/10.1088/1674-4527/9/3/007
https://doi.org/10.1088/1674-4527/9/3/007
Publikováno v:
The Astrophysical Journal. 686:L37-L40
This Letter is to investigate the physics of a newly discovered phenomenon -- contracting flare loops in the early phase of solar flares. In classical flare models, which were constructed based on the phenomenon of expansion of flare loops, an energy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d59299f5b71060dcd123dbf3f115c332
https://doi.org/10.1086/592835
https://doi.org/10.1086/592835
Publikováno v:
Advances in Space Research. 41:1195-1201
In this paper, we analyze the footpoint motion of two large solar flares using observations made by the Transition Region and Coronal Explorer (TRACE) and Reuven Ramaty High Energy Solar Spectroscopic imager (RHESSI). The two flares are the M5.7 flar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bbe7e653d67df4567846eda75657bdce
https://doi.org/10.1016/j.asr.2007.04.095
https://doi.org/10.1016/j.asr.2007.04.095
Publikováno v:
Solar Physics. 239:137-148
Using one-minute cadence vector magnetograms from Big Bear Solar Observatory (BBSO), we analyze the temporal behavior of derived longitudinal electric currents associated with two flares on July 26, 2002. One of the events is an M1.0 flare which occu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cdfdd1ca54fb9f219e3d516b0c33824a
https://doi.org/10.1007/s11207-006-0120-7
https://doi.org/10.1007/s11207-006-0120-7