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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3S9T7C8
Repositorysid.inpe.br/mtc-m21c/2018/11.26.15.19
Last Update2018:11.26.15.19.08 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2018/11.26.15.19.08
Metadata Last Update2019:04.05.18.20.56 (UTC) administrator
DOI10.1029/2018JA025773
ISSN2169-9402
Citation KeyPalitRaulCorr:2018:NuSiIo
TitleLower ionospheric plasma-chemical evolution and VLF signal modulation by a series of SGR x-ray bursts: numerical simulation with an ion-chemistry model
Year2018
MonthSept.
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1227 KiB
2. Context
Author1 Palit, Sourav
2 Raulin, Jean-Pierre
3 Correia, Emília
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JH2C
ORCID1 0000-0003-2932-3666
Group1
2
3 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Presbiteriana Mackenzie
2 Universidade Presbiteriana Mackenzie
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 souravspace@gmail.com
2
3 emilia.correia@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume123
Number9
Pages7930-7942
History (UTC)2018-11-26 15:19:08 :: simone -> administrator ::
2018-11-26 15:19:09 :: administrator -> simone :: 2018
2018-11-26 15:19:26 :: simone -> administrator :: 2018
2019-01-04 16:57:14 :: administrator -> simone :: 2018
2019-01-07 11:38:39 :: simone -> administrator :: 2018
2019-04-05 18:20:56 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsionosphere
SGR
X-ray
VLF
Monte Carlo
ion chemistry
AbstractThe X-ray and gamma ray radiation from astrophysical transient sources, like X-ray bursts from soft gamma repeaters (SGRs) and gamma ray bursts (GRBs), can affect the plasma properties of the lower ionosphere and middle atmosphere. Multiple very low frequency (VLF) receivers in South America, with an unprecedented high time resolution of 20 ms, detected one such series of bursts from SGR J1550-5418 on 22 January 2009. Due to lack of other suitable means of observation corresponding to the lower part of Earth's ionosphere (similar to 60-100 km), the VLF detection and analysis of transient ionizing events (mostly of solar origin) has emerged as an excellent method to investigate various chemical and plasma characteristics at these heights. Extragalactic events, like SGR bursts and GRBs, with sharp modulation in their radiation time profile and very high energy photon abundances provide most unique opportunities of such studies with the possibility of extending even lower heights in the atmosphere. Here, for the first time, an extensive computer model, consisting of the combination of Monte Carlo ionization rate computation, a one dimensional atmospheric chemistry module, and VLF waveguide mode calculation, for the reconstruction of VLF signal modulation produced by SGR X-ray burst starting from the observed spectrum and lightcurve of the event is presented. We gain some valuable insight on the nature of chemical and dynamic evolution over the entire height range of the atmosphere examined from the exercise.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Lower ionospheric plasma-chemical...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/3S9T7C8
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/3S9T7C8
Languageen
Target Filepalit_lower.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item List
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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