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
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
SOIR Data Workshop CO 2 density profiles Factor 10 Factor profiles
SOIR Data Workshop CO 2 rotational temperature profiles 60K
SOIR Data Workshop CO density profiles 80 profiles
SOIR Data Workshop CO rotational temperature profiles
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
SOIR Data Workshop Extinction profiles retrieved 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
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
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 3.0 µm
SOIR Data Workshop Latitudinal variation of the extinction Period of 500 days (orbit till ) spread over all latitudes µm:40 AM & 42 PM Polynomial fit (2 d order) for each altitude
SOIR Data Workshop 80 km Season 11 Season 12 Season 13 Δ = evening terminator O = morning terminator
SOIR Data Workshop Three bands were rotationally analyzed: − G.S. (CO 2 628) ; ( CO 2 628) and G.S. ( CO 2 638) CO 2 spectroscopy 1.ASIMAT: retrieval of atmospheric parameters 2.New bands linelist, calibrated using HDO lines