CME Angular Width is a measurement metric in solar physics that quantifies the angular extent of a coronal mass ejection as observed in heliospheric imaging, distinguishing it from other CME characteristics by specifically describing its apparent width in the plane of the sky relative to the Sun's center.
55
Publications
4.4K
Citations
161
Authors
91
Institutions
Publications per year
2017–2026
12
Variants
Coronal Mass Ejection Angular Width
Parents
Publications
55
1–5 of 55
Authors
161
- YM
6
h-index
- NG
5
h-index
- SY
5
h-index
- RA
4
h-index
- HX
4
h-index
1–5 of 161
Institutions
91
Goddard Space Flight Center
Greenbelt, United States
10 h-index
13 publications
2.5K citations
University of America
Murrieta, United States
9 h-index
20 publications
5.7K citations
Catholic University of America
Washington D.C., United States
8 h-index
19 publications
5.5K citations
Kyung Hee University
Seoul, South Korea
6 h-index
17 publications
367 citations
Chinese Academy of Sciences
Beijing, China
4 h-index
11 publications
185 citations
United States Naval Research Laboratory
Washington, United States
4 h-index
12 publications
3.7K citations
Jagiellonian University
Krakow, Poland
4 h-index
4 publications
345 citations
Observatoire de Paris
Paris, France
3 h-index
8 publications
1.1K citations
1–8 of 91
Venues
- The Astrophysical Journal
ApJ · 14 publications · 577 citations
13
h-index
- Journal of Geophysical Research Atmospheres
JGR · 7 publications · 2K citations
7
h-index
- Solar Physics
5 publications · 115 citations
5
h-index
- Journal of Geophysical Research Space Physics
5 publications · 150 citations
4
h-index
- Space Weather
3 publications · 190 citations
3
h-index
1–5