Feasibility of high-spatial-resolution nighttime near-IR imaging of Venus’ surface from a platform just below the clouds: A radiative transfer study accounting for the potential of haze

Author:

Davis Anthony B.ORCID,Baines Kevin H.,Sutin Brian M.,Cutts James A.,Dorsky Leonard I.,Byrne Paul K.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference59 articles.

1. Spatially resolved measurements of H2O, HCl, CO, OCS, SO2, cloud opacity, and acid concentration in the venus near-infrared spectral windows;Arney;J. Geophys. Res.: Planets,2014

2. Blurring of Light Due to Multiple Scattering by the Medium: A Path Integral Approach;Ashikhmin,2004

3. Detection of sub-micron radiation from the surface of Venus by Cassini/VIMS;Baines;Icarus,2000

4. Baines, K.H., Cutts, J.A., Mcgarey, P., Sutin, B.M., Davis, A.B., 2021. High Spatial Resolution Imaging of the Surface of Venus via a Balloon-Borne Tow-Body Camera System. In: 52Nd Lunar and Planetary Science Conference. p. 2498, Abstract No. 2548.

5. Geologic interpretation of the near-infrared images of the surface taken by the Venus Monitoring Camera, Venus Express;Basilevsky;Icarus,2012

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