Ушбу ишга иқтибос қилган ишлар

6 та иш

Иш: Variation of the X‐Ray Bright Point Number over the Solar Activity Cycle

1. Solar Cycle 23 in Coronal Bright Points

   I. Sattarov, Alexei Pevtsov, Nina Karachik +2

   МақолаSolar and Space Plasma DynamicsSolar Physics20107 иқтибос

   ABIABI:AkademIndex/openalex/2026.other.307310

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

   Nina Karachik, Alexei Pevtsov, I. Sattarov

   МақолаSolar and Space Plasma DynamicsThe Astrophysical Journal20065 иқтибос

   ABIABI:AkademIndex/openalex/2006.article.000035

3. 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

   ABIABI:AkademIndex/openalex/2025.article.000855

4. What SDO tells us about structure and evolution of coronal bright points

   Nina Karachik, E.P. Minenko, I. Sattarov +2

   МақолаSolar and Space Plasma DynamicsAstronomische Nachrichten20140 иқтибос

   ABIABI:AkademIndex/openalex/2014.article.000207

5. Investigation of the evolution of coronal bright points and magnetic field topology

   E.P. Minenko, Nina Karachik, I. Sattarov +1

   МақолаSolar and Space Plasma DynamicsAstronomy Letters20140 иқтибос

   ABIABI:AkademIndex/openalex/2014.article.000224

6. 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

   ABIABI:AkademIndex/openalex/2025.article.002370