CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS

We have investigated the cause of three “isolated” negative radio bursts recorded one after another at several frequencies in the 1–17 GHz range at the Nobeyama Radio Observatory, Ussuriysk Astrophysical Observatory, and Learmonth Solar Observatory on April 10–11, 2014. The cause of the rarely obser...

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Main Author: I.V. Kuzmenko
Format: Article
Language:English
Published: INFRA-M 2020-09-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/39462/view
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author I.V. Kuzmenko
author_facet I.V. Kuzmenko
author_sort I.V. Kuzmenko
collection DOAJ
description We have investigated the cause of three “isolated” negative radio bursts recorded one after another at several frequencies in the 1–17 GHz range at the Nobeyama Radio Observatory, Ussuriysk Astrophysical Observatory, and Learmonth Solar Observatory on April 10–11, 2014. The cause of the rarely observed “isolated” negative bursts is the absorption of radio emission from the quiet Sun’s regions or a radio source in the material of a large eruptive filament. Analysis of observations in different spectral ranges using images from the Nobeyama radioheliograph and the Solar Dynamics Observatory/Atmospheric Imaging Assembly has shown that the cause of all the three radio emission depressions was the screening of the limb radio source by the material of recurrent coronal jets. Parameters of the absorbing material were estimated using a previously developed model. These estimates confirmed the absorption of solar radio emission in cold material with a temperature of ~104 K at the bottom of the jets.
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spelling doaj.art-19ce95541fa442c288b6f0ce860263022022-12-22T00:46:51ZengINFRA-MSolar-Terrestrial Physics2500-05352020-09-0163232810.12737/stp-63202003CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTSI.V. Kuzmenko 0Institute of Applied Astronomy RAS, St. Petersburg, RussiaWe have investigated the cause of three “isolated” negative radio bursts recorded one after another at several frequencies in the 1–17 GHz range at the Nobeyama Radio Observatory, Ussuriysk Astrophysical Observatory, and Learmonth Solar Observatory on April 10–11, 2014. The cause of the rarely observed “isolated” negative bursts is the absorption of radio emission from the quiet Sun’s regions or a radio source in the material of a large eruptive filament. Analysis of observations in different spectral ranges using images from the Nobeyama radioheliograph and the Solar Dynamics Observatory/Atmospheric Imaging Assembly has shown that the cause of all the three radio emission depressions was the screening of the limb radio source by the material of recurrent coronal jets. Parameters of the absorbing material were estimated using a previously developed model. These estimates confirmed the absorption of solar radio emission in cold material with a temperature of ~104 K at the bottom of the jets.https://naukaru.ru/en/nauka/article/39462/viewsolar radio emissionmicrowave negative burstradio sourceactive prominencerecurrent coronal jet
spellingShingle I.V. Kuzmenko
CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS
Solar-Terrestrial Physics
solar radio emission
microwave negative burst
radio source
active prominence
recurrent coronal jet
title CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS
title_full CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS
title_fullStr CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS
title_full_unstemmed CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS
title_short CORONAL JETS AS A CAUSE OF MICROWAVE NEGATIVE BURSTS
title_sort coronal jets as a cause of microwave negative bursts
topic solar radio emission
microwave negative burst
radio source
active prominence
recurrent coronal jet
url https://naukaru.ru/en/nauka/article/39462/view
work_keys_str_mv AT ivkuzmenko coronaljetsasacauseofmicrowavenegativebursts