Reference Frame Transformations

Reference Frame Transformations is a formal method in astrometry that specifies the mathematical procedures and kinematic models required to convert positional and rotational measurements from one celestial or terrestrial reference frame to another, accounting for time-dependent effects such as Earth rotation, polar motion, and relativistic frame-dragging.

188

Publications

11K

Citations

414

Authors

225

Institutions

Publications per year

2017–2026

44

Authors

414

  1. VA
    V. A. Brumberg

    Institute of Applied Astronomy, Russia

    4 publications · 154 citations

    4

    h-index

  2. GB
    Gunnar Blohm

    Queen's University, Canada

    4 publications · 134 citations

    4

    h-index

  3. TS
    Tomás Soler

    NOAA National Geodetic Survey, United States

    3 publications · 60 citations

    3

    h-index

  4. GB
    G. B. Malykin

    Russian Academy of Sciences, Russia

    3 publications · 80 citations

    3

    h-index

  5. JH
    Jen-Yu Han

    National Taiwan University, Taiwan

    3 publications · 67 citations

    3

    h-index

1–5 of 414

Venues

  1. IEEE Transactions on Industrial Electronics

    6 publications · 471 citations

    6

    h-index

  2. Physical review. D/Physical review. D.

    PRD · 6 publications · 194 citations

    6

    h-index

  3. GPS Solutions

    5 publications · 220 citations

    5

    h-index

  4. Journal of Surveying Engineering

    5 publications · 110 citations

    5

    h-index

  5. American Journal of Physics

    5 publications · 225 citations

    5

    h-index

1–5