Anomaly Conversion

Anomaly Conversion is a computational method in celestial mechanics that transforms orbital position information between different types of Keplerian anomalies—specifically, mean, eccentric, and true anomalies—by solving the underlying transcendental equations to enable consistent characterization of time-dependent orbital motion.

4

Publications

174

Citations

8

Authors

7

Institutions

Publications per year

2017–2026

2

Authors

8

  1. LH
    Louis Hecker

    Collecte Localisation Satellites (France), France

    1 publications · 29 citations

    1

    h-index

  2. CC
    Chein‐I Chang

    University of Maryland, Baltimore County, United States

    1 publications · 45 citations

    1

    h-index

  3. PC
    P. C. Gregory

    University of British Columbia, Canada

    1 publications · 88 citations

    1

    h-index

  4. PŠ
    Petr Štěpánek

    Research Institute of Geodesy, Topography and Cartography, Czechia

    1 publications · 29 citations

    1

    h-index

  5. RH
    Rasha H. Ibrahim

    University of Baghdad, Iraq

    1 publications · 12 citations

    1

    h-index

1–5 of 8

Venues

  1. Iraqi Journal of Science

    1 publications · 12 citations

    1

    h-index

  2. Advances in Space Research

    1 publications · 29 citations

    1

    h-index

  3. 1

    h-index

  4. 1

    h-index

1–4