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7 та иш

Иш: Observation of a non-uniform component in the distribution of coronal bright points

  1. X‐Ray Bright Points and Photospheric Bipoles during Cycles 22 and 23

    I. Sattarov, Alexei Pevtsov, A. S. Hojaev +1

    МақолаSolar and Space Plasma DynamicsThe Astrophysical Journal20029 иқтибос
    ABI

  2. Solar Cycle 23 in Coronal Bright Points

    I. Sattarov, Alexei Pevtsov, Nina Karachik +2

    МақолаSolar and Space Plasma DynamicsSolar Physics20107 иқтибос
    ABI

  3. Rotation of Solar Corona from Tracking of Coronal Bright Points

    Nina Karachik, Alexei Pevtsov, I. Sattarov

    МақолаSolar and Space Plasma DynamicsThe Astrophysical Journal20065 иқтибос
    ABI

  4. On anticorrelation of number of coronal bright points with sunspot number during 1996–2006

    I. Sattarov, Alexei Pevtsov, Nina Karachik +1

    МақолаSolar and Space Plasma DynamicsAdvances in Space Research20071 иқтибос
    ABI

  5. Hemispheric asymmetry of coronal bright point’s number and area over solar cycles 23–24

    Nina Karachik, E.P. Minenko

    МақолаSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society20251 иқтибос
    ABI

  6. Two types of coronal bright points their characteristics, and evolution

    I. Sattarov, Nina Karachik, Chori T. Sherdanov +2

    МақолаSolar and Space Plasma DynamicsProceedings of the International Astronomical Union20100 иқтибос
    ABI

  7. Two types of coronal bright points as indicators of global and local dynamo processes

    Nina Karachik

    МақолаSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society20250 иқтибос
    ABI