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Post-impulsive millimeter emission of the 2022-05-04 solar flare
G. G. Motorina, Yu. T. Tsap, V. V. Smirnova +2
The present work aims at analyzing the nature of millimeter (mm) emission observed during the post-impulsive phase of the solar flare SOL2022-05-04T08:45 (M5.7), detected by the RT…
Pre-impulsive and Impulsive Phases of the Sub-Terahertz Flare of March 28, 2022
G. G. Motorina, Yu. T. Tsap, V. V. Smirnova +3
Properties of the solar radio spectrum, as well as the temporal profiles of flare emission, indicate the thermal nature of the sub-terahertz (sub-THz) component observed as the gro…
On the origin of 140 GHz emission from the 4 July 2012 solar flare
Yuriy T. Tsap, Victoria V. Smirnova, Alexander S. Morgachev +4
The sub-THz event observed on the 4 July 2012 with the Bauman Moscow State Technical University Radio Telescope RT-7.5 at 93 and 140~GHz as well as Kislovodsk and Metsähovi radio t…