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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/44EDDR5
Repositorysid.inpe.br/mtc-m21c/2021/04.02.15.14   (restricted access)
Last Update2021:04.02.15.14.47 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2021/04.02.15.14.47
Metadata Last Update2022:04.03.19.24.35 (UTC) administrator
DOI10.1016/j.icarus.2021.114403
ISSN0019-1035
Citation KeyShahHaiMolAbdBat:2021:CoMoD
TitleA coupled model of the D and E regions of Mars' ionosphere for flare and non-flare electron density profiles
Year2021
MonthJune
Access Date2024, May 16
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size7775 KiB
2. Context
Author1 Shah, Siddhi Y.
2 Haider, S. A.
3 Molina-Cuberos, G. J.
4 Abdu, Mangalathayil Ali
5 Batista, Inez Staciarini
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHNK
5 8JMKD3MGP5W/3C9JHDA
Group1
2
3
4 DIHPA-CGCE-INPE-MCTI-GOV-BR
5 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Physical Research Laboratory
2 Physical Research Laboratory
3 University of Murcia
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2 haider@prl.res.in
3
4 ma.abdu@inpe.br
5 inez.batista@inpe.br
JournalIcarus
Volume361
Pagese114403
Secondary MarkA1_GEOCIÊNCIAS A2_ASTRONOMIA_/_FÍSICA
History (UTC)2021-04-02 15:14:47 :: simone -> administrator ::
2021-04-02 15:14:48 :: administrator -> simone :: 2021
2021-04-02 15:15:25 :: simone -> administrator :: 2021
2022-04-03 19:24:35 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractSolar X-ray flare responses in the E region of Mars' ionosphere were observed from Mars Global Surveyor (MGS) on 6 April 2001 and 17 March 2003. We have developed a coupled model for the calculation of Ionospheric Electron Content (IEC), flare and non-flare electron density profiles due to impact of X-rays (0.590 Å) and Galactic Cosmic Rays (GCR) in the D and E regions of Mars' ionosphere simultaneously. In the non-flare profile the D layer is produced at 25 km due to impact of GCR and hard X-rays (0.53 Å) with electron densities 1.0 × 102 cm−3 and 8 × 102 cm−3 respectively while E layer is produced at 100110 km with electron density ~ 45 × 104 cm−3 due to impact of soft X-rays (390 Å). The D flare peak is produced at 30 km with electron density ~ 24 × 104 cm−3. The E flare peak is produced at 100 km with electron density 12 × 105 cm−3. The predicted flare E-peak density is higher by a factor of ~2 than the measurements carried out by MGS. The D peak density of flare profile is larger by 12 orders of magnitude than that produced for non-flare profiles. Our model suggests that hard X-ray is a major source of the D layer in the Martian ionosphere.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > A coupled model...
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4. Conditions of access and use
Languageen
Target Fileshah_coupled.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.54.26 1
sid.inpe.br/mtc-m21/2012/07.13.14.50.14 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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