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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/QAMqE
Repositorysid.inpe.br/mtc-m17@80/2007/06.29.14.00   (restricted access)
Last Update2008:06.05.12.06.21 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/06.29.14.00.54
Metadata Last Update2018:06.05.03.30.25 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1016/j.asr.2007.05.056
ISSN0273-1177
Citation KeySethJaya:2008:LoDiTh
TitleLongitudinal distribution of thermospheric densities and ionization rates in the upper atmosphere of Mars at mid-latitude using MGS ACC data
Year2008
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size453 KiB
2. Context
Author1 Seth, S. P.
2 Jayanthi, Uadya Bhaskaram
Group1
2 DAS-CEA-INPE-MCT-BR
Affiliation1 Department of Physics, Bhavan’s R.A College of Science
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 sseth2002@yahoo.com.in
JournalAdvances in Space Research
Volume41
Number9
Pages1353-1360
History (UTC)2008-06-05 12:06:22 :: simone -> administrator ::
2012-07-13 22:23:15 :: administrator -> banon ::
2013-02-19 13:56:19 :: banon -> simone :: 2008
2013-02-20 15:20:00 :: simone -> administrator :: 2008
2018-06-05 03:30:25 :: administrator -> marciana :: 2008
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsMars
Ionosphere
Peak altitude
Ionization rate
Planetary waves
Tides
AbstractThe Accelerometer Experiment (ACC) onboard Mars Global Surveyor (MGS) measured 1600 density profiles in the upper atmosphere of Mars during aerobraking. These measurements reveal large-scale and small-scale structure in the thermosphere of Mars. Here, the measurements of mass density for 115 orbits (#P0670P0789) from November 1 to 30, 1998, under spring equinox and medium solar activity conditions (average F10.7 137) during phase 2 of the aerobraking in the thermosphere of Mars at different altitudes and longitudes are presented for northern mid-latitude (1742°N) in the dayside atmosphere using ACC onboard MGS. From these mass densities, the neutral densities of different gases are derived from their mixing ratios. Using these neutral densities, the longitudinal distribution of photoionization rates and photoelectron impact ionization rates are calculated at wavelength range 1102.57 nm due to EUV and soft X-ray radiation under photochemical controlled region using Analytical Yield Spectrum approach (AYS). These conditions are appropriate for MGS Phase 2 aerobraking period from which the accelerometer data is used. Under the photochemical equilibrium condition, the electron density near the peak varies as the square root of the total peak ionization rate. Using this fact, an attempt is being made to estimate the mean primary and secondary peak electron density by averaging the longitudinal variations of total peak ionization rates in the northern mid-latitude (1742°N) ionosphere of Mars, as there is no radio science measurement at this latitude region by MGS.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Longitudinal distribution of...
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4. Conditions of access and use
Languageen
Target Filelongitudinal distribution.pdf
User Groupadministrator
banon
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
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7. Description control
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