Solar Declination
Solar Declination is the angular position of the Sun relative to the Earth's equatorial plane, specifically defined as the latitude on Earth where the Sun is directly overhead at solar noon on a given day, distinguishing it from other solar angles by its annual variation due to the tilt of the Earth's axis.
82
Publications
3.4K
Citations
224
Authors
148
Institutions
Publications per year
2017–2026
17
Variants
Solar Declination Angle
Parents
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148

Cornell University
Ithaca, United States
3 h-index
10 publications
672 citations

Chinese Academy of Sciences
Beijing, China
3 h-index
10 publications
850 citations

University of Milano-Bicocca
Milan, Italy
3 h-index
3 publications
199 citations
Arcetri Astrophysical Observatory
Florence, Italy
3 h-index
9 publications
597 citations
National Institute for Astrophysics
Rome, Italy
3 h-index
8 publications
688 citations

University of Bologna
Bologna, Italy
3 h-index
3 publications
199 citations

Universidad de Extremadura
Badajoz, Spain
2 h-index
7 publications
115 citations

U.S. National Science Foundation
Alexandria, United States
2 h-index
2 publications
124 citations
1–8 of 148
JGR · 8 publications · 453 citations
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AJ · 4 publications · 112 citations
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3 publications · 253 citations
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3 publications · 50 citations
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2 publications · 62 citations
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