Astronomical Time Determination
Astronomical Time Determination is a method in geodetic astronomy that determines precise time by observing the apparent positions and motions of celestial bodies relative to an observer's location on Earth.
88
Publications
6.7K
Citations
250
Authors
144
Institutions
Publications per year
2017–2026
19
Parents
88
Time-calibrated Milankovitch cycles for the late Permian
Huaichun Wu, Shihong Zhang, Linda A. Hinnov et al. · Nature Communications · 2013 · 186 citations · Full text
1–5 of 88
250
6
h-index
6
h-index
5
h-index
4
h-index
3
h-index
1–5 of 250
144
Utrecht University
Utrecht, The Netherlands
8 h-index
26 publications
1.4K citations

China University of Geosciences (Beijing)
Beijing, China
7 h-index
20 publications
1.5K citations
China University of Geosciences
Wuhan, China
6 h-index
21 publications
752 citations
United States Naval Observatory
Flagstaff, United States
6 h-index
7 publications
148 citations
State Key Laboratory of Oil and Gas Reservoir Geology and Exploitation
Chengdu, China
4 h-index
5 publications
123 citations

Search for Extraterrestrial Intelligence
Mountain View, United States
3 h-index
4 publications
350 citations
Massachusetts Institute of Technology
Cambridge, United States
3 h-index
3 publications
246 citations

Ames Research Center
Mountain View, United States
3 h-index
7 publications
646 citations
1–8 of 144
4 publications · 386 citations
4
h-index
3 publications · 91 citations
3
h-index
3 publications · 56 citations
3
h-index
3 publications · 181 citations
3
h-index
2 publications · 129 citations
2
h-index
1–5