Martian phase function: Modeling the visible to near-infrared surface photometric function using HST-WFPC2 data
Ozone abundance on Mars from infrared heterodyne spectra. I. Acquisition, retrieval, and anticorrelation with water vapor
Properties of Martian soils, rocks, and atmospheric dust derived from analysis of Hubble Space Telescope and Mars Exploration Rover data
Ultraviolet dust aerosol properties as observed by MARCI
Instrument
STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
2001-01-16T16:08:13Z/2001-09-15T18:18:12Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, James comma Philip B., 2007, 'Ozone, Condensates, and Dust in the Martian Atmosphere', 1.0, European Space Agency, https://doi.org/10.5270/esa-u2herv8