Coronal Polarimetry

Coronal Polarimetry is a specialized observational technique within solar polarimetry that measures the polarization state of light emitted or scattered in the solar corona to infer the physical properties and magnetic field structure of coronal plasma.

72

Publications

4.1K

Citations

297

Authors

134

Institutions

Publications per year

2017–2026

14

Authors

297

  1. ST
    S. Tomczyk

    NSF NCAR High Altitude Observatory, United States

    6 publications · 1.3K citations

    6

    h-index

  2. SF
    Silvano Fineschi

    Osservatorio Astrofisico di Torino, Italy

    5 publications · 75 citations

    5

    h-index

  3. SE
    S. E. Gibson

    NSF National Center for Atmospheric Research, United States

    5 publications · 292 citations

    5

    h-index

  4. LR
    Laurel Rachmeler

    Marshall Space Flight Center, United States

    4 publications · 242 citations

    4

    h-index

  5. PG
    P. G. Judge

    NSF National Center for Atmospheric Research, United States

    4 publications · 1.2K citations

    4

    h-index

1–5 of 297

Venues

  1. The Astrophysical Journal

    ApJ · 24 publications · 693 citations

    17

    h-index

  2. Solar Physics

    10 publications · 649 citations

    10

    h-index

  3. Astronomy and Astrophysics

    6 publications · 121 citations

    6

    h-index

  4. 5

    h-index

  5. 4

    h-index

1–5