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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/3GDQ4J8
Repositorysid.inpe.br/plutao/2014/06.03.18.46
Last Update2015:02.10.12.09.12 (UTC) administrator
Metadata Repositorysid.inpe.br/plutao/2014/06.03.18.46.52
Metadata Last Update2018:06.04.23.39.28 (UTC) administrator
DOI10.1002/2013JA019670
ISSN2169-9402
Labellattes: 1272123236892781 4 RaulinTroGimCorMac:2014:NiSeIo
Citation KeyRaulinTroCasCorMac:2014:NiSeIo
TitleNighttime Sensitivity of Ionospheric VLF Measurements to X-ray Bursts From a Remote Cosmic Source
Year2014
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size510 KiB
2. Context
Author1 Raulin, Jean Pierre
2 Trottet, Gerard
3 Castro, Carlos Guillermo Gimenez de
4 Correia, Emilia
5 Macotela, Edith Liliana
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JH2C
Group1
2
3
4 DAS-CEA-INPE-MCTI-GOV-BR
Affiliation1 Universidade Presbiteriana Mackenzie
2 Observatoire de Paris
3 Universidade Presbiteriana Mackenzie
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Universidade Presbiteriana Mackenzie
e-Mail Addressmarcelo.pazos@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume119
Pages4758-4766
History (UTC)2014-06-03 18:46:52 :: lattes -> administrator ::
2018-06-04 23:39:28 :: administrator -> marcelo.pazos@inpe.br :: 2014
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsVLF waves
High energy
X-ray
SGR
GRB
AbstractOn 22 January 2009, a series of X-ray bursts were emitted by the soft gamma ray repeater SGR J1550-5418. Some of these bursts produced enhanced ionization in the nighttime lower ionosphere. These ionospheric disturbances were studied using X-ray measurements from the Anti-Coincidence Shield of the Spectrometer for Integral onboard the International Gamma-Ray Astrophysics Laboratory and simultaneous phase and amplitude records from two VLF propagation paths between the transmitter Naval Radio Station, Pearl Harbor (Hawaii) and the receivers Radio Observatorio do Itapetinga (Brazil) and Estação Antarctica Commandante Ferraz (Antarctic Peninsula). The VLF measurements have been obtained with an unprecedented high time resolution of 20 ms. We find that the illumination factor I (illuminated path length times the cosine of the zenith angle), which characterizes the propagation paths underlying the flaring object, is a key parameter which determines the sensitivity threshold of the VLF detection of X-ray bursts from nonsolar transients. For the present VLF measurements of bursts from SGR J1550-5418, it is found that for I≥1.8 Mm, all X-ray bursts with fluence in the 25 keV to 2 MeV range larger than F25_min~ 1.0 × 106 erg/cm2 produce a measurable ionospheric disturbance. Such a lower limit of the X-ray fluence value indicates that moderate X-ray bursts, as opposed to giant X-ray bursts, do produce ionospheric disturbances larger than the sensitivity limit of the VLF technique. Therefore, the frequency of detection of such events could be improved, for example by increasing the coverage of existing VLF receiving networks. The VLF detection of high-energy astrophysical bursts then appears as an important observational diagnostic to complement their detection in space. This would be especially important when space observations suffer from adverse conditions, like saturation, occultation from the Earth, or the passage of the spacecraft through the South Atlantic anomaly.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Nighttime Sensitivity of...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W/3GDQ4J8
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W/3GDQ4J8
Languageen
User Groupadministrator
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marcelo.pazos@inpe.br
Reader Groupadministrator
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Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
LinkingTrabalho não Vinculado à Tese/Dissertação
Mirror Repositoryiconet.com.br/banon/2006/11.26.21.31
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; AGU; COMPENDEX; SCOPUS.
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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7. Description control
e-Mail (login)marcelo.pazos@inpe.br
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