Ushbu ishga iqtibos qilgan ishlar

4 ta ish

Ish: 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

   MaqolaSolar and Space Plasma DynamicsThe Astrophysical Journal20029 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.168818

2. 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

3. 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

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

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

   MaqolaSolar and Space Plasma DynamicsAstronomy Letters20140 iqtibos

   ABIABI:AkademIndex/openalex/2014.article.000224