Coronal Jets

Coronal Jets is a transient, collimated ejection of plasma and magnetic flux in the solar corona, distinguished from other coronal mass eruptions by its narrow, beam-like morphology and frequent association with small-scale magnetic reconnection events at the base of the corona.

321

Publications

18.8K

Citations

585

Authors

276

Institutions

Publications per year

2017–2026

119

Authors

585

  1. AC
    Alphonse C. Sterling

    Marshall Space Flight Center, United States

    21 publications · 2K citations

    19

    h-index

  2. CR
    C. R. DeVore

    United States Naval Research Laboratory, United States

    18 publications · 1.8K citations

    17

    h-index

  3. RL
    Ronald L. Moore

    Marshall Space Flight Center, United States

    16 publications · 1.4K citations

    15

    h-index

  4. SK
    S. K. Antiochos

    United States Naval Research Laboratory, United States

    12 publications · 1.2K citations

    12

    h-index

  5. JY
    Jiayan Yang

    Yunnan Observatories, China

    11 publications · 422 citations

    11

    h-index

1–5 of 585

Venues

  1. The Astrophysical Journal

    ApJ · 148 publications · 9.9K citations

    57

    h-index

  2. The Astrophysical Journal Letters

    29 publications · 1.3K citations

    23

    h-index

  3. Astronomy and Astrophysics

    36 publications · 1.3K citations

    22

    h-index

  4. Solar Physics

    20 publications · 999 citations

    17

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 8 publications · 191 citations

    8

    h-index

1–5