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Ish: Rotation of Solar Corona from Tracking of Coronal Bright Points

1. Solar Cycle 23 in Coronal Bright Points

   I. Sattarov, Alexei Pevtsov, Nina Karachik +2

   MaqolaSolar and Space Plasma DynamicsSolar Physics20107 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.307310

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

   I. Sattarov, Alexei Pevtsov, Nina Karachik +1

   MaqolaSolar and Space Plasma DynamicsAdvances in Space Research20071 iqtibos

   ABIABI:AkademIndex/openalex/2007.article.000194

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

   Nina Karachik, E.P. Minenko

   MaqolaSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society20251 iqtibos

   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

   MaqolaSolar and Space Plasma DynamicsAstronomische Nachrichten20140 iqtibos

   ABIABI:AkademIndex/openalex/2014.article.000207

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

   Nina Karachik

   MaqolaSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.002370