Fine structures of radio bursts observed during the February 12, 2010 flare

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00373248" target="_blank" >RIV/67985815:_____/11:00373248 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Fine structures of radio bursts observed during the February 12, 2010 flare

Original language description

Using the newly reconstructed Ondřejov radio spectrograph the radio emission of the February 12, 2010 flare was studied in details. The high-time resolution of the spectrograph (10 ms) reveals several interesting fine structures in (a) type III burst, (b) reverse drift burst and (c) drifting pulsating structures. Furthermore, an unique type of short-lasting and narrowband spikes was recognized. These fine structures give a more detailed information about superthermal electrons producing these bursts andabout the electron acceleration.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

<a href="/en/project/IAA300030701" target="_blank" >IAA300030701: Radio and X-ray diagnostics of the solar flare magnetic reconnection</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2011

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Central European Astrophysical Bulletin

ISSN

1845-8319

e-ISSN

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Volume of the periodical

35

Issue of the periodical within the volume

1

Country of publishing house

HR - CROATIA

Number of pages

8

Pages from-to

215-222

UT code for WoS article

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EID of the result in the Scopus database

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