Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Sushree S. Nayak"'
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 1, p 143 (2024)
Coronal jets are the captivating eruptions that are often found in the solar atmosphere and primarily formed due to magnetic reconnection. Despite their short-lived nature and lower energy compared to many other eruptive events, e.g., flares and coro
Externí odkaz:
https://doaj.org/article/d8e493c933fd4ffa960ec677e6a756f8
Publikováno v:
Solar Physics. 296
Three-dimensional (3D) magnetohydrodynamic simulations are carried out to explore magnetic reconnections in the presence of 3D magnetic nulls and quasi-separatrix layers (QSLs). The initial magnetic fields are created by superposing uniform vertical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5b8f1591b5d0bbac96da0a8c3e83c4d
https://doi.org/10.1007/s11207-021-01768-7
https://doi.org/10.1007/s11207-021-01768-7
Publikováno v:
Physics of Plasmas. 28:024502
We present a three-dimensional magnetohydrodynamic simulation of the NOAA active region 12017 to explore the onset of an X-class flare on 2014 March 29 at 17:48 UT. The simulation is initiated with a magnetic field constructed by non-force-free-field
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::80ed6b7ce7620583fbf8c113ece5a824
https://doi.org/10.1063/5.0035086
https://doi.org/10.1063/5.0035086
Publikováno v:
The Astrophysical Journal. 892:44
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ef30aafd6992729ff5a67c64dbca4c19
https://doi.org/10.3847/1538-4357/ab75bb
https://doi.org/10.3847/1538-4357/ab75bb
Magnetic reconnections (MRs) for various magnetic field line (MFL) topologies are believed to be the initiators of various solar eruptive events like flares and coronal mass ejections (CMEs). Consequently, important is a thorough understanding and qu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::849f4487c9a089ea6ed3becb3d2bb5eb
The solar active region (AR) 12192 was one of the most flare productive region of solar cycle 24, which produced many X-class flares; the most energetic being an X3.1 flare on October 24, 2014 at 21:10 UT. Customarily, such events are believed to be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f4c1d2dcede09ef55dc239b506c01d72
Publikováno v:
The Astrophysical Journal. 875:10
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::81086d4e684fcd42b2c96eb9d6323563
https://doi.org/10.3847/1538-4357/ab0a0b
https://doi.org/10.3847/1538-4357/ab0a0b
Publikováno v:
The Astrophysical Journal. 860:96
Magnetohydrodynamics of the solar corona is simulated numerically. The simulation is initialized with an extrapolated non-force-free magnetic field using the vector magnetogram of the active region (AR) NOAA 12192 obtained on the solar photosphere. P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3cc2e15210476a76d082fb8793b60467
https://doi.org/10.3847/1538-4357/aac265
https://doi.org/10.3847/1538-4357/aac265
Publikováno v:
Astrophysical Journal; 4/10/2019, Vol. 875 Issue 1, p1-1, 1p
Publikováno v:
Astrophysical Journal; 6/20/2018, Vol. 860 Issue 2, p1-1, 1p