Available in PDS4 - CERTIFIED
    July 4 1997 - September 27 1997 - 83 sols (Martian Year 23, 142.3 - Ls 188)







    Pathfinder Opacity pic
    Prototype of IMP NASA/JPL
    Pathfinder Opacity pic Pathfinder Opacity pic

    Atmospheric Opacity
    These atmospheric opacities were derived from images of the sun obtained with the Imager for Mars Pathfinder (IMP). The filter set allowed opacities to be obtained at 450, 670, 883, and 989 nm. The goal was to derive the average daily opacity and its wavelength variation. These atmospheric opacities were derived from images of the sun obtained with the Imager for Mars Pathfinder (IMP). The filter set allowed opacities to be obtained at 450, 670, 883, and 989 nm. The goal was to derive the average daily opacity and its wavelength variations.

    Useful Mission Documents


    The Data Description
    These data are tabulated as simple CVS files with PDS4 XML labels. The data were derived by assuming Beer’s Law and are composed of 2 tables: Total Opacity where Ls, Sol, Dust tau, Rayleigh tau and RMS residuals are tabulated (imp_taum.csv) and Wavelength Dependent Opacity where Ls, Sol. Airmass and opacity at 450, 670, 883 and 989 nm are listed (imp_tau.csv).

    Accessing the Data Bundle

    Bundle Documentation
    MPF Atmospheric Opacity (xml, pdf)

    Accessing the data
    Derived Data
    imp_tau (xml, csv)
    imp_taum (xml, csv)
    Raw Data

    Citing Datasets for Publication
    P. H. Smith, P. H., M. Lemmon, M., and R. Beebe, (2015), Derived opacities from Mars Pathfinder, NASA Planetary Data System, https://doi.org/10.17189/1518586