Zobrazeno 1 - 10
of 7 244
pro vyhledávání: '"W, Ni"'
Publikováno v:
The Astrophysical Journal Letters, Vol 973, Iss 1, p L1 (2024)
The periodic coronal rain and in-phase radiative intensity pulsations have been observed in multiple wavelengths in recent years. However, due to the lack of three-dimensional coronal magnetic fields and thermodynamic data in observations, it remains
Externí odkaz:
https://doaj.org/article/f8c215f1ae0443eea213f1d2876966af
Autor:
J. H. Guo, Y. W. Ni, Y. Guo, C. Xia, B. Schmieder, S. Poedts, Z. Zhong, Y. H. Zhou, F. Yu, P. F. Chen
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 140 (2024)
Magnetic flux ropes are a bundle of twisted magnetic field lines produced by internal electric currents, which are responsible for solar eruptions and are the major drivers of geomagnetic storms. As such, it is crucial to develop a numerical model th
Externí odkaz:
https://doaj.org/article/741115ca414a4df8b24f40a82ececfd9
Publikováno v:
The Astrophysical Journal Letters, Vol 958, Iss 2, p L42 (2023)
We present imaging and spectroscopic diagnostics of a long filament during its formation with the observations from the Chinese H α Solar Explorer and Solar Dynamics Observatory. The seed filament first appeared at about 05:00 UT on 2022 September 1
Externí odkaz:
https://doaj.org/article/cfc06f4bed6d44f0aa640f4c69dc2d76
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 2, p 119 (2023)
Solar filaments often exhibit rotation and deflection during eruptions, which would significantly affect the geoeffectiveness of the corresponding coronal mass ejections (CMEs). Therefore, understanding the mechanisms that lead to such rotation and l
Externí odkaz:
https://doaj.org/article/394f096c54c04d4f8c1c8663d93e5bc1
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 266, Iss 1, p 3 (2023)
Solar filament eruptions, flares, and coronal mass ejections (CMEs) are manifestations of drastic releases of energy in the magnetic field, which are related to many eruptive phenomena, from the Earth’s magnetosphere to black hole accretion disks.
Externí odkaz:
https://doaj.org/article/78352865032245a4befc20b62158119f
Akademický článek
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Autor:
Thomas A. Cooper, Seyed H. Zandavi, George W. Ni, Yoichiro Tsurimaki, Yi Huang, Svetlana V. Boriskina, Gang Chen
Publikováno v:
Nature Communications, Vol 9, Iss 1, Pp 1-10 (2018)
Solar steam generation is limited by fouling of solar converters, and the steam temperature is usually pinned to 100 °C. Here, both limitations are overcome in a system utilizing a solar absorber and light down-converter to achieve radiative heating
Externí odkaz:
https://doaj.org/article/0ec3f69d114d42ccbf43fee98b7ecf00
Publikováno v:
ACS Omega, Vol 3, Iss 11, Pp 14902-14909 (2018)
Externí odkaz:
https://doaj.org/article/f38872f9eb1f482b991856f3234be242
Publikováno v:
Galaxies, Vol 10, Iss 2, p 58 (2022)
We present here the kinematics of the EUV wave associated with a GOES M1.0-class solar flare, which originates in NOAA AR 12740. The event is thoroughly observed with Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) with hi
Externí odkaz:
https://doaj.org/article/0b95abdbd23c4aa4bfc56e02c29ddd91
Autor:
P. Ke, M. Xu, J. Xu, X. Yuan, W. Ni, Y. Sun, H. Zhang, Y. Zhang, Q. Tian, R. Dowling, H. Jiang, Z. Zhao, Z. Lu
Publikováno v:
Journal of Endocrinological Investigation. 46:327-335