ARCB/GSSR M RADIO TELESC DERIVED RADAR MODEL UNIT MAP V1.0

A model for Mars depolarized radar echo power that (1) matches the observed variation of total radar cross section with longitude and (2) produces model spectra that have the broad features of spectra published for Goldstone Solar System Radar and for Arecibo Observatory 1980 to 1982 observations. This model assumes that different geologic units on Mars backscatter in a uniformly bright manner, where radar echo power is A * Cosine (angle of incidence), where A varies across the planet. This model assigns depolarized radar echo power on a degree-by-degree basis in latitude and longitude.

Data and Resources

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Additional Info

Field Value
Maintainer Thomas Morgan
Last Updated July 17, 2025, 17:41 (UTC)
Created April 1, 2025, 02:13 (UTC)
accessLevel public
accrualPeriodicity irregular
bureauCode {026:00}
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harvest_object_id 358518ee-5e0f-4b8f-9d47-be539d0207db
harvest_source_id 61638e72-b36c-4866-9d28-551a3062f158
harvest_source_title DNG Legacy Data
identifier urn:nasa:pds:context_pds3:data_set:data_set.arcb-gssr-m-rtls-5-model-v1.0_wqhr-f7dd
issued 2018-06-26
landingPage https://pds.nasa.gov/ds-view/pds/viewDataset.jsp?dsid=ARCB%2FGSSR-M-RTLS-5-MODEL-V1.0
modified 2023-01-26
programCode {026:005}
publisher National Aeronautics and Space Administration
references {https://pds.nasa.gov}
resource-type Dataset
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source_hash 68e51cb03d721fd1bdaaffd836e988ce4134e9726288451859a512cb053cd7b7
source_schema_version 1.1
theme {"Earth Science"}