Results 101 to 110 of about 51,333 (260)

Fast plasmoid-mediated reconnection in a solar flare. [PDF]

Nat Commun, 2022
Yan X, Xue Z, Jiang C, Priest ER, Kliem B, Yang L, Wang J, Kong D, Song Y, Feng X, Liu Z.   +10 more
europepmc   +1 more source

Electron Trapping and Precipitation in Asymmetric Solar Flare Loops [PDF]

, 2000
Markus J. Aschwanden, L. Fletcher, Taro Sakao, T. Kosugi, H. S. Hudson   +4 more
openalex   +1 more source

A Peculiar Feature of the First Ionization Potential Effect Before a Solar Flare Impulsive Phase Observed by MSS-1B, CHASE, and SDO

The Astrophysical Journal
The impulsive phase of solar flares is often accompanied by the depletion of the elements with low first ionization potential (FIP), whose abundance decreases from the coronal level to the photospheric level, and then recovers back to the coronal level ...
Man-Hei Ng, Xiaoping Zhang, P. F. Chen
doaj   +1 more source

Solar flare accelerates nearly all electrons in a large coronal volume. [PDF]

Nature, 2022
Fleishman GD, Nita GM, Chen B, Yu S, Gary DE.   +4 more
europepmc   +1 more source

Sideways displacement of penumbral fibrils by the solar flare on 2006 December 13 [PDF]

, 2010
Jun Zhang, Leping Li, S. K. Solanki
openalex   +1 more source

Three-dimensional Turbulent Reconnection within the Solar Flare Current Sheet [PDF]

, 2023
Yulei Wang, Xin Cheng, M. D. Ding, Zhaoyuan Liu, Jian Liu, Xiaojue Zhu   +5 more
openalex   +1 more source

Data set for solar flare prediction using helioseismic and magnetic imager vector magnetic field data. [PDF]

Data Brief, 2021
Hollanda A, Antunes Da Silva AE, Cinto T.   +2 more
europepmc   +1 more source

Solar Flare Phenomena [PDF]

Nature, 1964
Solar Flares By Henry J. Smith and Elske van Panhuys Smith. Pp. xii + 322. (New York: The Macmillan Company; London: Collier-Macmillan, 1963.) 100s.
openaire   +1 more source

Two Distinctly Different Characteristics of Flare-driven Coronal Rain Revealed from High-resolution Spectroscopic Imaging Observations with FISS/GST

The Astrophysical Journal
We report on a flare-driven coronal rain event observed along postflare loops during the decay phase of an X1.6-class solar flare. Although high-resolution studies of flare-driven coronal rain have been conducted, imaging spectroscopic studies are rare ...
Donguk Song, Eun-Kyung Lim, Jongchul Chae, Maria S. Madjarska, Masahito Kubo, Hannah Kwak, Juhyung Kang, Ryohtaroh T. Ishikawa, Kyoung-Sun Lee   +8 more
doaj   +1 more source

Observations of Geomagnetic Crochet at High‐Latitudes Due To X1.5 Class Solar Flare on 3 July 2021

Space Weather
On 3 July 2021, an X1.5 solar flare from the National Oceanic and Atmospheric Administration solar Active Region AR12838 (24°N, 88°W) occurred at 14:18 UT, peaked at 14:29 UT, and decayed at 14:34 UT. The study of this X1.5 solar flare is significant due
S. S. Rao, Nandita Srivastava, Monti Chakraborty, Sandeep Kumar, D. Chakrabarty   +4 more
doaj   +1 more source