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SOIR Data Workshop SOIR science status A.C. Vandaele, A. Mahieux, S. Robert, R. Drummond, V. Wilquet, E. Neefs, B. Ristic, S. Berkenbosch, R. Clairquin
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SOIR Data Workshop Scientific results From SOIR measurements, construction of a database of vertical profiles of CO 2 density CO density H 2 O density HCl density HF density + isotopologues CO 2 rotational temperature CO rotational temperature Aerosols Measurements occur at terminator All latitudes covered Since 06/2006 till now
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SOIR Data Workshop CO 2 density profiles Factor 10 Factor 5 500 profiles
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SOIR Data Workshop CO 2 rotational temperature profiles 60K
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SOIR Data Workshop CO density profiles 80 profiles
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SOIR Data Workshop CO rotational temperature profiles
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SOIR Data Workshop Retrieval technique – Extinction profiles Transmittances Extinction : With aerosol slant opacity T the transmittance dz i the thickness of layer i I i the atmospheric intensity of layer i I 0 the full sun intensity β i the extinction of layer i The SOIR instrument has the potential of characterizing the aerosols in the mesosphere of Venus. Previous work combining the 3 channels of SPICAV/SOIR showed aerosol layers in successive orbits corresponding to the presence of mode 2 particles of radius up to ~1.0 µm in the upper haze (not observed before). V. Wilquet, et al., J. Geophys. Research, Vol. 114, E00B42, 13 pp., 2009 Aerosols
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SOIR Data Workshop Extinction profiles retrieved simultaneously @ different wavelength At high latitude North : extinction profiles are different for each wavelength Around the equator: the extinction coefficient is less sensitive to the wavelength
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SOIR Data Workshop Method: Fit of the extinction in function of the wavelength Refraction index model: spherical particles, 75% H 2 SO 4 Mie theory to derive extinction cross-section / Log-normal size distribution (r g, g ) Normalization of the extinction (experimental and model) Fitting experimental with theoretical values (minimization of merit function) Particle size and number density retrievals
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SOIR Data Workshop Spatial coverage of measurements Data spread over 3 years Better coverage close to the North pole, due to the geometry of the orbit Poor coverage between 40 and 60° N, due to orbit Green crosses:spectra registered @ 3.0 µm
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SOIR Data Workshop Latitudinal variation of the extinction Period of 500 days (orbit 884.2 till 1382.1) spread over all latitudes 82 measurements @ 3.0 µm:40 AM & 42 PM Polynomial fit (2 d order) for each altitude
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SOIR Data Workshop Aerosols @ 80 km Season 11 Season 12 Season 13 Δ = evening terminator O = morning terminator
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SOIR Data Workshop Three bands were rotationally analyzed: 2 + 3 − G.S. (CO 2 628) ; 2 1 + 2 - 2 ( CO 2 628) and 2 1 - G.S. ( CO 2 638) CO 2 spectroscopy 1.ASIMAT: retrieval of atmospheric parameters 2.New bands linelist, calibrated using HDO lines
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