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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3RFK6JL
Repositorysid.inpe.br/mtc-m21c/2018/07.18.15.21
Last Update2021:03.08.19.51.29 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2018/07.18.15.21.06
Metadata Last Update2021:03.08.19.51.30 (UTC) simone
Secondary KeyINPE--PRE/
Citation KeyBisoiSaJaYaAwSr:2018:FiHiTi
TitleEvidence of a distant decimetric spike source connected to the main electron acceleration site: first high time cadence gmrt observations
Year2018
Access Date2024, May 16
Secondary TypePRE CI
Number of Files1
Size61 KiB
2. Context
Author1 Bisoi, Susanta Kumar
2 Sawant, Hanumant Shankar
3 Janardhan, Padmanabhan
4 Yan, Yihua
5 Awasthi, Kumar
6 Srivastava, Shweta
Resume Identifier1
2 8JMKD3MGP5W/3C9JHBU
Group1
2 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 National Astronomical Observatories Of China (NAOC)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Physical Research Laboratory
4 National Astronomical Observatories Of China (NAOC)
5 University of Science and Technology of China
6 University of Science and Technology of China, H
Author e-Mail Address1 susanta@nao.cas.cn
2 sawant@das.inpe.br
3 janardhan.padmanabhan@gmail.com
4 yyh@nao.cas.cn
5 arun.awasthi.87@gmail.com
6 srivashweta@gmail.com
Conference NameCospar Scientific Assembly, 42
Conference LocationPasadena, California
Date14-22 July
History (UTC)2018-07-18 15:22:47 :: simone -> administrator :: 2018
2019-01-04 16:57:07 :: administrator -> simone :: 2018
2019-01-07 13:00:57 :: simone -> administrator :: 2018
2019-01-14 17:06:31 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractWe present a study of decimetric radio activity, associated with two (GOES C1.4 and M1.0 class) flares and a coronal mass ejection (CME) of 20 June 2015, using the first high time cadence (0.5s) 610 MHz observations of the Giant Meterwave Radio Telescope (GMRT). The GMRT images show strong radio sources during the M1.0 flare and CME, which are located near the flaring site, while, in contrary, a strong spike radio source during the C1.4 flare, with no corresponding coronal or magnetic features, are rather located about 500 arcsec away from the flare site in soft X-rays. Although weak radio burst sources are located near the flaring site, during the C1.4 flare maximum, associated with the spike radio source, which show a good temporal correspondence with a metric typeIII burst identified by the Solar Broadband Radio Spectrometer at Yunnan Astronomical Observatory. A multi-wavelength analysis, in combination with potential field source surface extrapolation, has been carried out to investigate the genesis of non-thermal radio emitting electrons, which revealed that the distant spike radio source, noticed during the C1.4 flare, is actually connected to the main electron acceleration sites and is generated by a plasma emission instead of a loss cone maser instability.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Evidence of a...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 18/07/2018 12:21 1.0 KiB 
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3RFK6JL
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3RFK6JL
Languageen
Target Filebisoi_evidence.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item List
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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