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Ish: Two Types of Coronal Bright Points in the 24-th Cycle of Solar Activity

1. 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

2. Latitudinal-Temporal Analysis of Long-Periodic Variations of Coronal Bright Points

   E.P. Minenko, Sh. A. Ehgamberdiev

   MaqolaSolar and Space Plasma DynamicsGeomagnetism and Aeronomy20210 iqtibos

   ABIABI:AkademIndex/openalex/2021.article.001017