Работы, на которые ссылается эта работа

Работ: 5

Работа: Two types of coronal bright points their characteristics, and evolution

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

   L. Golub, A. S. Krieger, G. S. Vaiana

   Статья1975Цитирований: 7

   ABIABI:AkademIndex/openalex/2026.other.168825

3. Nine Years Of Euv Bright Points

   Scott W. McIntosh, J. B. Gurman

   Статья2005Цитирований: 7

   ABIABI:AkademIndex/openalex/2026.other.307308

4. 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

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

   I. Sattarov, Alexei Pevtsov, Nina Karachik +1

   СтатьяSolar and Space Plasma DynamicsAdvances in Space Research2007Цитирований: 1

   ABIABI:AkademIndex/openalex/2007.article.000194