Работы, цитирующие эту работу

Работ: 4

Работа: Variation of X-ray bright point number over the solar activity cycle

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

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

   СтатьяSolar and Space Plasma DynamicsThe Astrophysical Journal2002Цитирований: 9

   ABIABI:AkademIndex/openalex/2026.other.168818

2. 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

3. 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

4. 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