Show simple item record

Nightglow in the Upper Atmosphere of Mars and Implications for Atmospheric Transport

dc.contributor.authorBertaux, J.-L.
dc.contributor.authorLeblanc, F.
dc.contributor.authorPerrier, S.
dc.contributor.authorQuemerais, E.
dc.contributor.authorKorablev, O.
dc.contributor.authorDimarellis, E.
dc.contributor.authorReberac, A.
dc.contributor.authorForget, F.
dc.contributor.authorSimon, P.C.
dc.contributor.authorStern, S.A.
dc.contributor.authorSandel, B.
dc.contributor.authorthe SPICAM team
dc.date2005
dc.date.accessioned2016-12-07T10:36:06Z
dc.date.available2016-12-07T10:36:06Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4641
dc.descriptionWe detected light emissions in the nightside martian atmosphere with the SPICAM (spectroscopy for the investigation of the characteristics of the atmosphere of Mars) ultraviolet (UV) spectrometer on board the Mars Express. The UV spectrum of this nightglow is composed of hydrogen Lyman α emission (121.6 nanometers) and the γ and δ bands of nitric oxide (NO) (190 to 270 nanometers) produced when N and O atoms combine to produce the NO molecule. N and O atoms are produced by extreme UV photodissociation of O 2, CO2, and N2 in the dayside upper atmosphere and transported to the night side. The NO emission is brightest in the winter south polar night because of continuous downward transport of air in this region at night during winter and because of freezing at ground level.
dc.languageeng
dc.titleNightglow in the Upper Atmosphere of Mars and Implications for Atmospheric Transport
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeMartian surface analysis
dc.subject.freeNitric acid
dc.subject.freePhotodissociation
dc.subject.freeSpectroscopic analysis
dc.subject.freeUltraviolet spectrometers
dc.subject.freeUpper atmosphere
dc.subject.freeMartian atmosphere
dc.subject.freeNightglow
dc.subject.freeUV spectrum
dc.subject.freeLight emission
dc.subject.freenitric oxide
dc.subject.freeMars
dc.subject.freearticle
dc.subject.freeastronomy
dc.subject.freeatmospheric transport
dc.subject.freedissociation
dc.subject.freefreezing
dc.subject.freelight
dc.subject.freepriority journal
dc.subject.freespectroscopy
dc.subject.freeultraviolet radiation
dc.subject.freewinter
dc.subject.freeAtmosphere
dc.subject.freeCarbon Dioxide
dc.subject.freeExtraterrestrial Environment
dc.subject.freeHydrogen
dc.subject.freeMars
dc.subject.freeNitric Oxide
dc.subject.freeNitrogen
dc.subject.freeOxygen
dc.subject.freeSeasons
dc.subject.freeSpacecraft
dc.subject.freeSpectrophotometry, Ultraviolet
dc.subject.freeTemperature
dc.subject.freeUltraviolet Rays
dc.source.titleScience
dc.source.volume307
dc.source.issue5709
dc.source.page566-569
Orfeo.peerreviewedYes
dc.identifier.doi10.1126/science.1106957
dc.identifier.scopus2-s2.0-19944432374


Files in this item

Thumbnail
Name:
Bertaux(2005b).pdf
Size:
359.0Kb
Format:
PDF
View/Open

This item appears in the following Collection(s)

Show simple item record