Show simple item record

dc.contributor.authorHaider, S.A.
dc.contributor.authorChoksi, V.R.
dc.contributor.authorSingh, V.
dc.contributor.authorMaguire, W.C.
dc.contributor.authorVerigin, M.I.
dc.date.accessioned2013-03-21T13:30:07Z
dc.date.available2013-03-21T13:30:07Z
dc.date.issued2007-12-01
dc.identifier.citationHaider , S A , Choksi , V R , Singh , V , Maguire , W C & Verigin , M I 2007 , ' Calculated densities of H3O+(H2O)n,NO2− (H2O)n, CO3− (H2O)n and electron in the nighttime ionosphere of Mars : Impact of solar wind electron and galactic cosmic rays ' , Journal of Geophysical Research , vol. 112 , no. A12 , A12309 . https://doi.org/10.1029/2007JA012530
dc.identifier.issn0148-0227
dc.identifier.otherPURE: 1443408
dc.identifier.otherPURE UUID: acdb400e-f02b-4082-ac49-866a4ed71aa2
dc.identifier.otherScopus: 84901007935
dc.identifier.urihttp://hdl.handle.net/2299/10252
dc.descriptionCopyright 2008 Elsevier B.V., All rights reserved.
dc.description.abstractWe have calculated the densities of positive ions and negative ions in the ionosphere of Mars at solar zenith angle 106° between height interval 0 km and 220 km. This model couples ion-neutral, electron neutral, dissociation of positive and negative ions, electron detachment, ion-ion, ion-electron recombination processes through 117 chemical reactions. Of the 34 ions considered in the model, the chemistry of 17 major ions (O2+, NO+, CO2+, H3O+H2O, H3O+(H2O)2, H3O+(H2O)3, H3O+(H2O)4, O2+CO2, H3O+, CO4−, CO3−, CO3−H2O, CO3− (H2O)2, NO2−H2O, NO2− (H2O)2, NO3−H2O, and NO3− (H2O)2) are discussed in this paper. At altitude below 70 km, the electron density is mainly controlled by hydrated hydronium ions and water clusters of NO2− and CO3−. The ions O2+ and NO+ dominate above this altitude. This calculation suggests that the ionosphere of Mars contains F and D peaks at altitude ∼130 km and ∼30 km due to precipitation of solar wind electron and galactic cosmic rays respectively. F peak is mainly produced by O2+ after heavy loss of CO2+ with atomic oxygen. D peak occurs due to high efficiency of electron attachment to Ox molecules, which entails that concentration of negative ions is higher than that of electron below 30 km. These results are compared with radio measurements made by Mars 4 and Mars 5 in the nighttime ionosphere.en
dc.language.isoeng
dc.relation.ispartofJournal of Geophysical Research
dc.titleCalculated densities of H3O+(H2O)n,NO2− (H2O)n, CO3− (H2O)n and electron in the nighttime ionosphere of Mars : Impact of solar wind electron and galactic cosmic raysen
dc.contributor.institutionCentre for Atmospheric and Climate Physics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=40149110536&partnerID=8YFLogxK
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.versionofrecordhttps://doi.org/10.1029/2007JA012530
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record