Synodic Rotation is a planetary rotation measurement defined by the time interval between successive alignments of a celestial body with the Sun as observed from a fixed external reference frame, distinguishing it from sidereal rotation by referencing solar conjunctions rather than distant stars.
54
Publications
1.6K
Citations
189
Authors
107
Institutions
Publications per year
2017–2026
10
Publications
54
1–5 of 54
Authors
189
- HW
3
h-index
- RB
3
h-index
- DH
2
h-index
- SG
2
h-index
- EB
2
h-index
1–5 of 189
Institutions
107
Lowell Observatory
Flagstaff, United States
4 h-index
4 publications
91 citations
University of Zagreb
Zagreb, Croatia
4 h-index
10 publications
377 citations
Institut für Sonnenphysik
Freiburg im Breisgau, Germany
4 h-index
5 publications
222 citations
Jet Propulsion Laboratory
Pasadena, United States
3 h-index
8 publications
113 citations
Stanford University
Stanford, United States
3 h-index
5 publications
186 citations
The University of Tokyo
Tokyo, Japan
3 h-index
4 publications
76 citations
Instituto de Astrofísica de Andalucía
Granada, Spain
2 h-index
4 publications
122 citations
University of Rijeka
Rijeka, Croatia
2 h-index
4 publications
88 citations
1–8 of 107
Venues
- The Astrophysical Journal
ApJ · 15 publications · 634 citations
13
h-index
- Astronomy and Astrophysics
6 publications · 192 citations
6
h-index
- Journal of Geophysical Research Atmospheres
JGR · 4 publications · 149 citations
4
h-index
- Solar Physics
4 publications · 116 citations
4
h-index
- The Astronomical Journal
AJ · 3 publications · 103 citations
3
h-index
1–5