Работы, цитирующие эту работу

Работ: 6

Работа: 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

   СтатьяSolar and Space Plasma DynamicsSolar Physics2010Цитирований: 7

   ABIABI:AkademIndex/openalex/2026.other.307310

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

   Nina Karachik, Alexei Pevtsov, I. Sattarov

   СтатьяSolar and Space Plasma DynamicsThe Astrophysical Journal2006Цитирований: 5

   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

   СтатьяSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society2025Цитирований: 1

   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

   СтатьяSolar and Space Plasma DynamicsAstronomische Nachrichten2014Цитирований: 0

   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

   СтатьяSolar and Space Plasma DynamicsAstronomy Letters2014Цитирований: 0

   ABIABI:AkademIndex/openalex/2014.article.000224

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

   Nina Karachik

   СтатьяSolar and Space Plasma DynamicsMonthly Notices of the Royal Astronomical Society2025Цитирований: 0

   ABIABI:AkademIndex/openalex/2025.article.002370