Physics
Scientist
Tashkent State Pedagogical University, 103 Yusuf Khos Khojib Street, Tashkent, 700100 Uzbekistan
National Solar Observatory
National Solar Observatory, Sunspot, NM 88349, USA Solar Observatory, Sunspot, NM 88349, USA
Active Longitudes in Distribution of EIT Bright Points
Coronal Bright Points at the Minimum of Sunspot Activity
Does Visibility Effect Fully Explain Cycle Variations of Coronal Bright Points?
Formation of Coronal Holes on the Ashes of Active Regions
Large-scale Structures in Distribution of Coronal Bright Points
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