True Anomaly

True Anomaly is the angular position of an orbiting body measured from the focus of its elliptical orbit, specifically the angle between the direction of periapsis and the current position vector of the body in its orbital plane, serving as a fundamental parameter in the description of Keplerian orbits within the two-body problem.

80

Publications

3K

Citations

204

Authors

120

Institutions

Publications per year

2017–2026

15

Authors

204

  1. GZ
    Gang Zhang

    Harbin Institute of Technology, China

    3 publications · 70 citations

    3

    h-index

  2. RB
    R. Broucke

    The University of Texas at Austin, United States

    2 publications · 24 citations

    2

    h-index

  3. LG
    L. Gergely

    University of Szeged, Hungary

    2 publications · 63 citations

    2

    h-index

  4. TE
    Thomas E. Carter

    Eastern Connecticut State University, United States

    2 publications · 461 citations

    2

    h-index

  5. ÁG
    Á. Giménez

    Instituto de Astrofísica de Andalucía, Spain

    2 publications · 186 citations

    2

    h-index

1–5 of 204

Venues

  1. Journal of Guidance Control and Dynamics

    18 publications · 866 citations

    16

    h-index

  2. The Astronomical Journal

    AJ · 10 publications · 317 citations

    10

    h-index

  3. Astronomy and Astrophysics

    5 publications · 314 citations

    5

    h-index

  4. The Astrophysical Journal

    ApJ · 4 publications · 113 citations

    4

    h-index

  5. 3

    h-index

1–5