About: On a Flat-shape Emission in the Solar Flare on 7th June 2012

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rdf:type	skos:Concept http://linked.opendata.cz/ontology/domain/vavai/Vysledek
Description	We present results of the study of the C1.5 solar flare(SOL2012-06-07T05:56) which occurred on June 7, 2012. This weak flare showed an extraordinary long flat emission in the X-ray flux curve in the 3-12 keV energy band. Duration of this flat period was about 10 minutes while the duration of the flare was almost 20 minutes. As this particular shape was observed both by RHESSI and FERMI, it could not be caused by an instrumental effect. We analyzed the optical spectra and slit-jaw images from the solar spectrograph in Ondřejov and in the hard X-ray by RHESSI as well as EUV data obtained by SDO and all available microwave data. We found that the %22flat emission%22 period was also observed in microwaves (5-17 GHz). During this period the motion of the flare source from the spot to south direction was revealed. We present results of the study of the C1.5 solar flare(SOL2012-06-07T05:56) which occurred on June 7, 2012. This weak flare showed an extraordinary long flat emission in the X-ray flux curve in the 3-12 keV energy band. Duration of this flat period was about 10 minutes while the duration of the flare was almost 20 minutes. As this particular shape was observed both by RHESSI and FERMI, it could not be caused by an instrumental effect. We analyzed the optical spectra and slit-jaw images from the solar spectrograph in Ondřejov and in the hard X-ray by RHESSI as well as EUV data obtained by SDO and all available microwave data. We found that the %22flat emission%22 period was also observed in microwaves (5-17 GHz). During this period the motion of the flare source from the spot to south direction was revealed. (en)
Title	On a Flat-shape Emission in the Solar Flare on 7th June 2012 On a Flat-shape Emission in the Solar Flare on 7th June 2012 (en)
skos:prefLabel	On a Flat-shape Emission in the Solar Flare on 7th June 2012 On a Flat-shape Emission in the Solar Flare on 7th June 2012 (en)
skos:notation	RIV/67985815:_____/13:00398907!RIV14-GA0-67985815
http://linked.open...avai/riv/aktivita	I P
http://linked.open...avai/riv/aktivity	I, P(GA13-24782S), P(GAP209/12/1652)
http://linked.open...iv/cisloPeriodika	2
http://linked.open...vai/riv/dodaniDat	2014
http://linked.open...aciTvurceVysledku	Bárta, Miroslav Kotrč, Pavel
http://linked.open.../riv/druhVysledku	J - Článek v odborném periodiku
http://linked.open...iv/duvernostUdaju	S - Úplné a pravdivé údaje nepodléhající ochraně podle zvláštních právních předpisů
http://linked.open...titaPredkladatele	Astronomický ústav AV ČR, v. v. i.
http://linked.open...dnocenehoVysledku	93636
http://linked.open...ai/riv/idVysledku	RIV/67985815:_____/13:00398907
http://linked.open...riv/jazykVysledku	eng - angličtina
http://linked.open.../riv/klicovaSlova	solar flare; energy relase; energy transport (en)
http://linked.open.../riv/klicoveSlovo	solar flare energy relase energy transport
http://linked.open...odStatuVydavatele	HR - Chorvatská republika
http://linked.open...ontrolniKodProRIV	[0F8E2DCA3F73]
http://linked.open...i/riv/nazevZdroje	Central European Astrophysical Bulletin
http://linked.open...in/vavai/riv/obor	BN
http://linked.open...ichTvurcuVysledku	2 (xsd:int)
http://linked.open...cetTvurcuVysledku	4 (xsd:int)
http://linked.open...vavai/riv/projekt	Analysis of the non-thermal electron distribution in the solar corona and transition region Turbulent energy transport in magnetic reconnection: Advanced numerical modeling and application to solar flares and eruptions
http://linked.open...UplatneniVysledku	2013
http://linked.open...v/svazekPeriodika	37
http://linked.open...iv/tvurceVysledku	Bárta, Miroslav Kashapova, L. K. Kotrč, Pavel Kupryakov, Yu. A.
issn	1845-8319
number of pages	8 (xsd:int)

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