Differential Image Motion

Differential Image Motion is a metric in observational astronomy that quantifies the degradation of astronomical image quality due to atmospheric turbulence by measuring the differences in positional shifts of a star's image across two or more spatially separated subapertures of a telescope.

83

Publications

3.8K

Citations

338

Authors

121

Institutions

Publications per year

2017–2026

14

Authors

338

  1. JV
    J. Vernin

    Université Côte d'Azur, France

    9 publications · 493 citations

    9

    h-index

  2. MS
    M. Sarazin

    European Southern Observatory, Germany

    7 publications · 443 citations

    7

    h-index

  3. AZ
    A. Ziad

    Université Côte d'Azur, France

    7 publications · 276 citations

    7

    h-index

  4. MS
    Matthias Schöck

    TMT Observatory, United States

    5 publications · 150 citations

    5

    h-index

  5. AT
    Andreï Tokovinin

    Cerro Tololo Inter-American Observatory, Chile

    5 publications · 615 citations

    5

    h-index

1–5 of 338

Venues

  1. Publications of the Astronomical Society of the Pacific

    PASP · 12 publications · 721 citations

    12

    h-index

  2. 11

    h-index

  3. 8

    h-index

  4. Astronomy and Astrophysics

    7 publications · 177 citations

    7

    h-index

  5. Astronomy and Astrophysics Supplement Series

    5 publications · 305 citations

    5

    h-index

1–5