SPICAV on Venus Express: Three spectrometers to study the global structure and composition of the Venus atmosphere

作者: Jean-Loup Bertaux , D. Nevejans , O. Korablev , E. Villard , E. Quémerais

DOI: 10.1016/J.PSS.2007.01.016

关键词: PhysicsAtmosphere of VenusSpectrometerPlanetary Fourier SpectrometerAirglowOccultationSolar windGlobal Ozone Monitoring by Occultation of StarsAstronomyVenus

摘要: Abstract Spectroscopy for the investigation of characteristics atmosphere Venus (SPICAV) is a suite three spectrometers in UV and IR range with total mass 13.9 kg flying on Express (VEX) orbiter, dedicated to study from ground level outermost hydrogen corona at more than 40,000 km. It derived SPICAM instrument already board Mars (MEX) great success, addition new high-resolution spectrometer, solar occultation (SOIR), working mode. The consists simple data processing unit providing interface these channels spacecraft. A spectrometer (118–320 nm, resolution 1.5 nm) identical MEX version. nadir viewing, limb viewing vertical profiling by stellar occultation. In orientation, SPICAV will analyse albedo spectrum (solar light scattered back clouds) retrieve SO2, distribution UV-blue absorber (of still unknown origin) dayside implications cloud structure atmospheric dynamics. On nightside, γ δ bands NO be studied, as well emissions produced electron precipitations. mode sensor measure profiles CO2, temperature, SO, clouds aerosols. density/temperature obtained constrain aid development dynamical models, top (∼60 km) 160 km atmosphere. This essential future missions that would rely aerocapture aerobraking. observations upper allow studies ionosphere through CO, CO+, CO2+, its direct interaction wind. H corona, two different scale heights, it better understanding escape mechanisms estimates their magnitude, crucial insight into long-term evolution VIS-IR (0.7–1.7 μm, 0.5–1.2 nm) employs pioneering technology: an acousto-optical tunable filter (AOTF). thermal emission peeping clouds, complementing both VIRTIS Planetary Fourier Spectrometer (PFS) VEX. this channel H2O, SOIR λ=2.2–4.3 μm, spectral λ/Δλ>15,000, highest concept includes combination echelle grating AOTF crystal sort out one order time. main objective HDO H2O occultation, characterize D atoms give about water Venus. also isotopes CO2 minor species, provides sensitive search species attempt nightside emission, which measurement lower atmosphere, compared ratio possibly discover constituents.

参考文章(65)
S. W. Bougher, A. I. F. Stewart, S. J. Bauer, A. F. Nagy, C. A. Barth, D. M. Hunten, Aeronomy of the current Martian atmosphere. Mars. pp. 1054- 1089 ,(1992)
R. Santer, L. V. Ksanfomaliti, M. Deschamps, A. Dollfus, Photopolarimetric analysis of the Martian atmosphere by the Soviet MARS-5 orbiter. I - White clouds and dust veils Astronomy and Astrophysics. ,vol. 150, pp. 217- 228 ,(1985)
Gerald R. Smith, Donald M. Hunten, Study of planetary atmospheres by absorptive occultations Reviews of Geophysics. ,vol. 28, pp. 117- 143 ,(1990) , 10.1029/RG028I002P00117
Andrew F. Nagy, Thomas E. Cravens, Hot oxygen atoms in the upper atmospheres of Venus and Mars Geophysical Research Letters. ,vol. 15, pp. 433- 435 ,(1988) , 10.1029/GL015I005P00433
Mark A. Gurwell, Evolution of deuterium on Venus. Nature. ,vol. 378, pp. 22- 23 ,(1995) , 10.1038/378022B0
Vladimir A Krasnopolsky, Michael J Mumma, G Randall Gladstone, Detection of Atomic Deuterium in the Upper Atmosphere of Mars Science. ,vol. 280, pp. 1576- 1580 ,(1998) , 10.1126/SCIENCE.280.5369.1576
C. A. Barth, J. B. Pearce, K. K. Kelly, L. Wallace, W. G. Fastie, Ultraviolet Emissions Observed near Venus from Mariner V. Science. ,vol. 158, pp. 1675- 1678 ,(1967) , 10.1126/SCIENCE.158.3809.1675
P. D. FELDMAN, H. W. MOOS, J. T. CLARKE, A. L. LANE, Identification of the UV nightglow from Venus Nature. ,vol. 279, pp. 221- 222 ,(1979) , 10.1038/279221A0
Anna Fedorova, Oleg Korablev, Severine Perrier, Jean-Loup Bertaux, Frank Lefevre, Alexander Rodin, Observation of O2 1.27 μm dayglow by SPICAM IR: Seasonal distribution for the first Martian year of Mars Express Journal of Geophysical Research. ,vol. 111, ,(2006) , 10.1029/2006JE002694
O. Korablev, J.-L. Bertaux, A. Grigoriev, E. Dimarellis, Yu. Kalinnikov, A. Rodin, C. Muller, D. Fonteyn, An AOTF-based spectrometer for the studies of Mars atmosphere for Mars Express ESA mission Advances in Space Research. ,vol. 29, pp. 143- 150 ,(2002) , 10.1016/S0273-1177(01)00581-6