HR: 1340h
AN: P33C-0251 [Abstracts]
TI: Spectral Imaging of Titan's Tropospheric Methane and Lower Atmosphere Haze Profile
AU: * Anderson, C M
EM: carrande@nmsu.edu
AF: New Mexico State University, Astronomy Department
1320 Frenger Street, Las Cruces, NM 88003
United States
AU: Young, E F
EM: efy@boulder.swri.edu
AF: Southwest Research Institute, 1050 Walnut Street, Boulder, CO 80302
United States
AU: Chanover, N J
EM: nchanove@nmsu.edu
AF: New Mexico State University, Astronomy Department
1320 Frenger Street, Las Cruces, NM 88003
United States
AU: McKay, C P
EM: cmckay@mail.arc.nasa.gov
AF: NASA Ames Research Center
NASA Ames Research Center, Space Science Division
NASA Mail Stop 245-3, Moffett Field, CA 94035
United States
AB:
We report high spatial resolution images of Titan between 0.6 and 1 micron taken at Ls=240 in November 2000, acquired with
the Space Telescope Imaging Spectrograph as part of program GO-8580. We utilize more than 100 wavelengths that traverse the
0.6 to 1 micron spectral region to address the methane abundance and degree of methane saturation in the troposphere, and
Titan's vertical distribution of haze below 100 km. The 0.619 micron methane band is of particular interest because previous
investigators have had difficulty matching Titan's modeled and observed albedo spectrum simultaneously at 0.619 and 0.888
micron. We employ a 1D radiative transfer fractal aerosol model with a Bayesian parameter estimation algorithm that computes
Titan's geometric albedo per pixel by adjusting the haze vertical distribution below 100 km and the methane mixing ratio
below 40 km. Results of this work will help to constrain Titan's lower atmospheric haze opacity in dynamical models, and
examine the spatially varying degree of methane saturation in conjunction with areas of known cloud formation. The
correlation of our results with the Huygens GCMS and DISR results will be discussed.
DE: 0300 ATMOSPHERIC COMPOSITION AND STRUCTURE
DE: 0305 Aerosols and particles (0345, 4801, 4906)
DE: 0360 Radiation: transmission and scattering
DE: 0368 Troposphere: constituent transport and chemistry
DE: 5210 Planetary atmospheres, clouds, and hazes (0343)
SC: Planetary Sciences [P]
MN: Fall Meeting 2005