Prominence Current Sheets
Prominence Current Sheets is a theoretical construct in solar physics denoting a thin, localized layer of intense electric current that develops within the magnetic field topology of a solar prominence, distinguishing itself by facilitating the dissipation of magnetic energy and enabling plasma instabilities critical to prominence dynamics and eruption mechanisms.
54
Publications
2.4K
Citations
128
Authors
78
Institutions
Publications per year
2017–2026
6
Parents
54
Volumetric heating in coronal streamers
S. T. Suess, A.-H. Wang, S. T. Wu · Journal of Geophysical Research Atmospheres · 1996 · 95 citations
1–5 of 54
128
5
h-index
5
h-index
3
h-index
2
h-index
P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Russia
1 publications · 17 citations
2
h-index
1–5 of 128
78

University of St Andrews
St Andrews, United Kingdom
6 h-index
7 publications
369 citations

University of Oslo
Oslo, Norway
4 h-index
11 publications
909 citations
NSF NCAR High Altitude Observatory
Boulder, United States
4 h-index
8 publications
395 citations

NSF National Center for Atmospheric Research
Boulder, United States
4 h-index
8 publications
395 citations

Imperial College London
London, United Kingdom
3 h-index
5 publications
116 citations

Chinese Academy of Sciences
Beijing, China
3 h-index
3 publications
48 citations
University of California, Los Angeles
Los Angeles, United States
3 h-index
5 publications
219 citations

U.S. National Science Foundation
Alexandria, United States
3 h-index
6 publications
286 citations
1–8 of 78
ApJ · 11 publications · 665 citations
11
h-index
9 publications · 297 citations
10
h-index
5 publications · 202 citations
5
h-index
JGR · 5 publications · 316 citations
5
h-index
2 publications · 146 citations
3
h-index
1–5