Solar Spicules
Solar Spicules is a dynamic chromospheric phenomenon characterized by narrow, jet-like protrusions of plasma extending from the solar limb, distinguished by their rapid vertical motion and short-lived nature within the Sun's lower atmosphere.
168
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9.2K
Citations
290
Authors
154
Institutions
Publications per year
2017–2026
26
168
Seismology of the sun and sun-like stars
E. J. Rolfe · ESASP · 1988 · 273 citations
High‐Resolution Observations and Modeling of Dynamic Fibrils
Bart De Pontieu, V. H. Hansteen, L. Rouppe van der Voort et al. · The Astrophysical Journal · 2007 · 243 citations · Full text
Natural Sciences, Astronomy, Physics +17
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154

University of Oslo
Oslo, Norway
23 h-index
76 publications
6.8K citations
Lockheed Martin (United States)
Bethesda, United States
20 h-index
43 publications
6.5K citations
University of Sheffield
Sheffield, United Kingdom
15 h-index
28 publications
2.2K citations
NSF NCAR High Altitude Observatory
Boulder, United States
12 h-index
16 publications
1K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
10 h-index
22 publications
911 citations

Evgeni Kharadze Georgian National Astrophysical Observatory
Tbilisi, Georgia
10 h-index
14 publications
916 citations
Max Planck Institute for Solar System Research
Göttingen, Germany
10 h-index
22 publications
1.1K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
9 h-index
19 publications
2.2K citations
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ApJ · 73 publications · 3.6K citations
34
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24 publications · 907 citations
18
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16 publications · 1K citations
15
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12 publications · 394 citations
11
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5 publications · 522 citations
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