DOI

The comparative analysis of solar flares by GOES class M obtained with the Bauman Moscow State Technical University radio telescope RT-7.5 at frequencies of 93 and 140 GHz is presented. A positive slope of the sub-THz flux density spectrum was revealed for three flares between frequencies 93 and 140 GHz. The observational characteristics of these flares involving data in the X-ray, ultraviolet, and microwave ranges were described.
Translated title of the contributionM-CLASS SOLAR FLARE FEATURES OBSERVED WITH RT-7.5 BMSTU RADIO TELESCOPE
Original languageRussian
Title of host publication Солнечная и солнечно-земная физика - 2019
Subtitle of host publicationТруды XXIII Всероссийской ежегодной конференции по физике Солнца
EditorsА.В. Степанов, Ю.А. Наговицын
Place of PublicationСанкт-Петербург
PublisherГлавная (Пулковская) астрономическая обсерватория РАН
Pages357-360
Number of pages4
EditionГАО РАН
ISBN (Print)978-5-9651-1274-6
DOIs
StatePublished - 2019

    Scopus subject areas

  • Physics and Astronomy(all)

ID: 49920644