Apogee Dynamics

Apogee Dynamics is a theoretical framework within celestial mechanics that specifically models the temporal and spatial evolution of orbital parameters at the apogee point in two-body orbital motion, distinguishing itself from general orbital dynamics by focusing exclusively on the perturbations and stability characteristics unique to the highest altitude in an elliptical orbit.

18

Publications

1K

Citations

62

Authors

36

Institutions

Publications per year

2017–2026

1

Authors

62

  1. AM
    A. Miele

    Rice University, United States

    2 publications · 32 citations

    2

    h-index

  2. TW
    T. Wang

    Rice University, United States

    2 publications · 32 citations

    2

    h-index

  3. TE
    T. E. Moore

    Goddard Space Flight Center, United States

    2 publications · 45 citations

    2

    h-index

  4. LR
    L. R. Lyons

    University of California, Los Angeles, United States

    1 publications · 37 citations

    1

    h-index

  5. AB
    A. Balogh

    Imperial College London, United Kingdom

    1 publications · 160 citations

    1

    h-index

1–5 of 62

Venues

  1. Geophysical Research Letters

    3 publications · 237 citations

    3

    h-index

  2. Journal of Guidance Control and Dynamics

    3 publications · 59 citations

    3

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 3 publications · 413 citations

    3

    h-index

  4. 2

    h-index

  5. Journal of Aerospace Engineering

    1 publications · 11 citations

    1

    h-index

1–5