Topocentric Coordinates

Topocentric Coordinates is a coordinate system in solar system astrometry that specifies the position of a celestial object relative to an observer's location on the surface of the Earth, differing from geocentric or heliocentric systems by accounting for the observer's local topography and parallax effects.

18

Publications

711

Citations

49

Authors

29

Institutions

Publications per year

2017–2026

4

Authors

49

  1. DS
    D. S. Caprette

    Goddard Space Flight Center, United States

    3 publications · 93 citations

    3

    h-index

  2. JW
    James W. Ryan

    University of Miami, United States

    3 publications · 93 citations

    3

    h-index

  3. GF
    Giovanni F. Gronchi

    University of Pisa, Italy

    2 publications · 49 citations

    2

    h-index

  4. CM
    Chao Ma

    Goddard Space Flight Center, United States

    2 publications · 47 citations

    2

    h-index

  5. ZK
    Zoran Knežević

    University of Pisa, Italy

    1 publications · 35 citations

    1

    h-index

1–5 of 49

Venues

  1. The Astronomical Journal

    AJ · 2 publications · 45 citations

    2

    h-index

  2. NASA Technical Reports Server (NASA)

    Repository · 2 publications · 70 citations

    2

    h-index

  3. 2

    h-index

  4. The Astrophysical Journal

    ApJ · 1 publications · 33 citations

    1

    h-index

  5. Journal of Geodesy

    1 publications · 15 citations

    1

    h-index

1–5