Published March 18, 2022 | Version v1

Surface emissivity of Mars from MGS Thermal Emission Spectrometer, sampled to Mars Odyssey THEMIS bands 3-9

Authors/Creators

  • 1. Stony Brook University

Description

These maps are described in Pankine et al. (submitted to Planetary and Space Science). Surface emissivity was derived from MGS TES data, and then binned at a spatial resolution of 8 pixels-per-degree. The binned surface emissivity was then convolved to THEMIS spectral bandpasses between bands 3-9 (~7.9 to 12.5 microns).

Each map covers the range -180 to 180 degrees longitude, and -70 to 70 degrees latitude. Null data values are set to zero. 

A longitudinal offset of 0.271 degrees was applied so that the maps align with data sets that use the IAU 2000 prime meridian.

These products may be uploaded as custom maps into the JMARS GIS software.

Files

Files (90.4 MB)

Name Size
md5:b2e154ac64494de244674abeaeb53c79
12.9 MB Download
md5:f32776a50df07f724f207d316a3c224a
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md5:74cc15493362b9ec9d53f74b6b9ba4ec
12.9 MB Download
md5:4ac52b26923f4ebaa4106b112dabad32
12.9 MB Download
md5:0c4538a6de08f6bc0db60cc0dab5121d
12.9 MB Download
md5:8282e3bf3ae8f2ce3b2259d00769502e
12.9 MB Download
md5:c63f71853710b9c2a6c97a176ed15778
12.9 MB Download