Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Beili Ying"'
Autor:
Shuting Li, Li Feng, Beili Ying, Lei Lu, Kaifan Ji, Ying Li, Guanglu Shi, Hui Li, Yu Huang, Weiqun Gan
Publikováno v:
The Astrophysical Journal Letters, Vol 969, Iss 1, p L16 (2024)
H i Ly α emission in the chromosphere and transition region is a key ingredient of the incident radiation to coronal neutral hydrogen for modeling corona Ly α emission. The Ly α emission distribution across the solar disk can be obtained from a Ly
Externí odkaz:
https://doaj.org/article/26f625d8043e4bd4a47f92f3806d311b
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 2, p 131 (2024)
Solar magnetic fields are closely related to various physical phenomena on the Sun, which can be extrapolated with different models from photospheric magnetograms. However, the open flux problem (OFP), the underestimation of the magnetic field derive
Externí odkaz:
https://doaj.org/article/2f3d50db268949f6aa0b586e9ff75608
Autor:
Alessandro Bemporad, Guanglu Shi, Shuting Li, Beili Ying, Li Feng, Jun Lin, Lucia Abbo, Vincenzo Andretta, Aleksandr Burtovoi, Vania Da Deppo, Yara De Leo, Silvano Fineschi, Federica Frassati, Silvio Giordano, Catia Grimani, Giovanna Jerse, Federico Landini, Salvatore Mancuso, Giampiero Naletto, Gianalfredo Nicolini, Maurizio Pancrazzi, Marco Romoli, Giuliana Russano, Clementina Sasso, Daniele Spadaro, Marco Stangalini, Roberto Susino, Luca Teriaca, Michela Uslenghi
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 1, p 92 (2024)
For the first time the evolution of the coronal reconfiguration after a coronal mass ejection (CME) was observed by the multichannel Metis Coronagraph on board the ESA–Solar Orbiter mission. The images acquired in visible light (VL) between 3.0 and
Externí odkaz:
https://doaj.org/article/ee7dc9aee2d5440589b3a0a99b9e8c55
Autor:
Li Feng, Weiqun Gan, Siqing Liu, Huaning Wang, Hui Li, Long Xu, Weiguo Zong, Xiaoxing Zhang, Yaguang Zhu, Haiyan Wu, Anqin Chen, Yanmei Cui, Xinghua Dai, Juan Guo, Han He, Xin Huang, Lei Lu, Qiao Song, Jingjing Wang, Qiuzhen Zhong, Ling Chen, Zhanle Du, Xingliang Guo, Yu Huang, Hu Li, Ying Li, Senlin Xiong, Shenggao Yang, Beili Ying
Publikováno v:
Frontiers in Physics, Vol 8 (2020)
The Advanced Space-based Solar Observatory (ASO-S) is a mission aiming at exploring solar flares, coronal mass ejections (CMEs), solar magnetic field and their relationships. To fulfill its major scientific objectives, ASO-S has three elaborately-des
Externí odkaz:
https://doaj.org/article/a25ca1539a14446fae824b7172441285
Publikováno v:
The Astrophysical Journal, Vol 942, Iss 1, p 3 (2022)
Stealthy coronal mass ejections (CMEs), lacking low coronal signatures, may result in significant geomagnetic storms. However, the mechanism of stealthy CMEs is still highly debated. In this work, we investigate whether there are differences between
Externí odkaz:
https://doaj.org/article/f0ff63baa8114d6f980aedc4b178316c
Publikováno v:
Astronomy and Astrophysics
Context. Observations reveal that shocks can be driven by fast coronal mass ejections (CMEs) and play essential roles in particle accelerations. A critical ratio, $\delta$, derived from a shock standoff distance normalized by the radius of curvature
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::479cc86cb4da1af3e10a0cc6ed4d5296
https://hdl.handle.net/21.11116/0000-000C-9354-F
https://hdl.handle.net/21.11116/0000-000C-9354-F
Autor:
Lei Lu, Li Feng, Alexander Warmuth, Astrid M. Veronig, Jing Huang, Siming Liu, Weiqun Gan, Zongjun Ning, Beili Ying, Guannan Gao
Magnetic reconnection is a fundamental physical process converting magnetic energy into not only plasma energy but also particle energy in various astrophysical phenomena. In this letter, we show a unique dataset of a solar flare where various plasmo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98a4cacb03211f1f108dc49ea1e9b6c2
http://arxiv.org/abs/2112.07857
http://arxiv.org/abs/2112.07857
Flat-field reflects the non-uniformity of the photometric response at the focal plane of an instrument, which uses digital image sensors, such as Charge Coupled Device (CCD) and Complementary Metal-Oxide-Semiconductor (CMOS). This non-uniformity must
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f110f581139f257f3b464b43e3c5fe78
http://arxiv.org/abs/2012.10110
http://arxiv.org/abs/2012.10110
Autor:
Hai-Yan Wu, Anqin Chen, Han He, Xingliang Guo, Yaguang Zhu, Huaning Wang, Xiaoxing Zhang, Qiuzhen Zhong, Xin Huang, Xinghua Dai, Lei Lu, Senlin Xiong, Hu Li, Beili Ying, Weiqun Gan, Yu Huang, Hui Li, Zhanle Du, Ying Li, Shenggao Yang, Jingjing Wang, Yanmei Cui, Ling Chen, Qiao Song, Juan Guo, Long Xu, Li Feng, Weiguo Zong, Siqing Liu
Publikováno v:
Frontiers in Physics, Vol 8 (2020)
The Advanced Space-based Solar Observatory (ASO-S) is a mission aiming at exploring solar flares, coronal mass ejections (CMEs), solar magnetic field and their relationships. To fulfill its major scientific objectives, ASO-S has three elaborately-des
Autor:
Matthew J. West, Li Feng, Marilena Mierla, Joseph Plowman, Weiqun Gan, Beili Ying, Bernd Inhester, Lei Lu
Coronal waves are large-scale disturbances often driven by coronal mass ejections (CMEs). We investigate a spectacular wave event on 7 March 2012, which is associated with an X5.4 flare (SOL2012-03-07). By using a running center-median (RCM) filterin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::29cd005cd381ff9b14954e5d6a0217d0