Solar Loops

Solar Loops is a physical phenomenon in solar astrophysics characterized as magnetized plasma structures that trace the Sun's coronal magnetic field lines, distinguished by their arched, loop-like morphology and emission in extreme ultraviolet and X-ray wavelengths due to high-temperature plasma confinement.

569

Publications

28.9K

Citations

841

Authors

324

Institutions

Publications per year

2017–2026

113

Authors

841

  1. VM
    V. M. Nakariakov

    University of Warwick, United Kingdom

    32 publications · 2.4K citations

    25

    h-index

  2. HP
    Hardi Peter

    Max Planck Institute for Solar System Research, Germany

    18 publications · 1.2K citations

    18

    h-index

  3. JA
    J. A. Klimchuk

    Goddard Space Flight Center, United States

    17 publications · 1.1K citations

    16

    h-index

  4. MJ
    Markus J. Aschwanden

    Lockheed Martin (United States), United States

    16 publications · 1.7K citations

    15

    h-index

  5. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    15 publications · 731 citations

    15

    h-index

1–5 of 841

Venues

  1. The Astrophysical Journal

    ApJ · 252 publications · 14K citations

    60

    h-index

  2. Astronomy and Astrophysics

    110 publications · 5.9K citations

    43

    h-index

  3. The Astrophysical Journal Letters

    40 publications · 2.2K citations

    30

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 15 publications · 513 citations

    14

    h-index

  5. Solar Physics

    21 publications · 1.1K citations

    13

    h-index

1–5