Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Mou, Chaozhou"'
Publikováno v:
A&A 623, A78 (2019)
Our recent observational study shows that the majority of coronal bright points (CBPs) in the quiet Sun are sources of one or more eruptions during their lifetime. Here, we investigate the non-potential time dependent structure of the magnetic field
Externí odkaz:
http://arxiv.org/abs/1901.09875
Autor:
Zhou, Wanyun, Liu, Yufei, Li, Yingxin, Kong, Siqi, Wang, Weilin, Ding, Boyun, Han, Jiyun, Mou, Chaozhou, Gao, Xin, Liu, Juntao
Publikováno v:
In Patterns 10 March 2023 4(3)
We present high-resolution observations of a magnetic reconnection event in the solar atmosphere taken with the New Vacuum Solar Telescope, AIA and HMI. The reconnection event occurred between the threads of a twisted arch filament system (AFS) and c
Externí odkaz:
http://arxiv.org/abs/1801.05983
Autor:
Xie, Haixia, Madjarska, Maria S., Li, Bo, Huang, Zhenghua, Xia, Lidong, Wiegelmann, Thomas, Fu, Hui, Mou, Chaozhou
How the solar corona is heated to high temperatures remains an unsolved mystery in solar physics. In the present study we analyse observations of 50 whole active-region loops taken with the Extreme-ultraviolet Imaging Spectrometer (EIS) on board the
Externí odkaz:
http://arxiv.org/abs/1705.02564
Autor:
Hou, Zhenyong, Huang, Zhenghua, Xia, Lidong, Li, Bo, Madjarska, Maria S., Fu, Hui, Mou, Chaozhou, Xie, Haixia
Various small-scale structures abound in the solar atmosphere above active regions, playing an important role in the dynamics and evolution therein. We report on a new class of small-scale transition region structures in active regions, characterized
Externí odkaz:
http://arxiv.org/abs/1608.04892
Autor:
Mou, Chaozhou, Huang, Zhenghua, Xia, Lidong, Madjarska, Maria S., Li, Bo, Fu, Hui, Jiao, Fangran, Hou, Zhenyong
Coronal bright points (BPs) are associated with magnetic bipolar features (MBFs) and magnetic cancellation. Here, we investigate how BP-associated MBFs form and how the consequent magnetic cancellation occurs. We analyse longitudinal magnetograms fro
Externí odkaz:
http://arxiv.org/abs/1511.09215
Autor:
Jiao, Fangran, Xia, Lidong, Li, Bo, Huang, Zhenghua, Li, Xing, Chandrashekhar, Kalugodu, Mou, Chaozhou, Fu, Hui
Quasi-periodic propagating disturbances (PDs) are ubiquitous in polar coronal holes on the Sun. It remains unclear as to what generates PDs. In this work, we investigate how the PDs are generated in the solar atmosphere by analyzing a fourhour datase
Externí odkaz:
http://arxiv.org/abs/1507.08440
We identify the coronal sources of the solar winds sampled by the ACE spacecraft during 1999-2008, and examine the in situ solar wind properties as a function of wind sources. The standard two-step mapping technique is adopted to establish the photos
Externí odkaz:
http://arxiv.org/abs/1505.00407
The contribution of plumes to the solar wind has been subject to hot debate in the past decades. The EUV Imaging Spectrometer (EIS) on board Hinode provides a unique means to deduce outflow velocities at coronal heights via direct Doppler shift measu
Externí odkaz:
http://arxiv.org/abs/1408.5473
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