Cme Interplanetary Evolution

CME Interplanetary Evolution is a theoretical construct in solar and space physics that describes the dynamic alteration of coronal mass ejection structures and kinematics as they propagate through the interplanetary medium, distinguished from related phenomena by its focus on the continuous evolution of magnetic, thermal, and plasma properties from the solar corona to the outer heliosphere.

103

Publications

6.3K

Citations

329

Authors

170

Institutions

Publications per year

2017–2026

34

Authors

329

  1. EP
    Erika Palmerio

    Goddard Space Flight Center, United States

    9 publications · 301 citations

    9

    h-index

  2. TN
    Teresa Nieves‐Chinchilla

    Goddard Space Flight Center, United States

    8 publications · 287 citations

    8

    h-index

  3. CM
    Christian Möstl

    Space Research Institute, Austria

    7 publications · 546 citations

    7

    h-index

  4. MT
    Manuela Temmer

    University of Graz, Austria

    7 publications · 827 citations

    7

    h-index

  5. PR
    Pete Riley

    Predictive Science (United States), United States

    6 publications · 678 citations

    6

    h-index

1–5 of 329

Venues

  1. The Astrophysical Journal

    ApJ · 23 publications · 1.6K citations

    20

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 20 publications · 1.8K citations

    17

    h-index

  3. Solar Physics

    13 publications · 495 citations

    13

    h-index

  4. Space Weather

    8 publications · 417 citations

    8

    h-index

  5. Astronomy and Astrophysics

    7 publications · 228 citations

    7

    h-index

1–5