Lunar South Pole Radar Images and Earthshine Model (85°S to Pole)

The larger map is centered on the south pole and is based on radar images obtained using Arecibo Observatory and Green Bank Telescope (Cornell University/Smithsonian Institution). The inset map shows solar permanently shaded regions (PSRs) larger than 10 km^2 as well as an earthshine model based on...

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Bibliographic Details
Main Authors: Stopar, Julie, orcid:0000-0003-1578-3688
Format: Map
Language:English
Published: Lunar and Planetary Institute, Regional Planetary Image Facility 2020
Subjects:
Online Access:https://hdl.handle.net/20.500.11753/1488
id ftusrahouston:oai:repository.hou.usra.edu:20.500.11753/1488
record_format openpolar
spelling ftusrahouston:oai:repository.hou.usra.edu:20.500.11753/1488 2023-05-15T18:21:50+02:00 Lunar South Pole Radar Images and Earthshine Model (85°S to Pole) Stopar, Julie orcid:0000-0003-1578-3688 Moon 2020-04 2 maps on 1 sheet (49 MB) application/pdf https://hdl.handle.net/20.500.11753/1488 en eng Lunar and Planetary Institute, Regional Planetary Image Facility LPI contribution no. 2347 Stopar J. (2020) Lunar South Pole Radar Images and Earthshine Mode (85°S to Pole), Lunar and Planetary Institute Regional Planetary Image Facility, LPI Contribution 2347. https://hdl.handle.net/20.500.11753/1488 https://hdl.handle.net/20.500.11753/1488 Moon--Maps Map 2020 ftusrahouston https://doi.org/20.500.11753/1488 2022-07-30T17:31:10Z The larger map is centered on the south pole and is based on radar images obtained using Arecibo Observatory and Green Bank Telescope (Cornell University/Smithsonian Institution). The inset map shows solar permanently shaded regions (PSRs) larger than 10 km^2 as well as an earthshine model based on Lunar Reconnaissance Orbiter Laser Altimeter (LOLA) data (NASA Goddard Space Flight Center). Polar stereographic projection is used with scale true at the pole. S-band Earth-based Radar Backscatter Mosaic -- Model of Earthshine Map South pole USRA Houston Repository (Universities Space Research Association) Lola ENVELOPE(-44.700,-44.700,-60.717,-60.717) South Pole
institution Open Polar
collection USRA Houston Repository (Universities Space Research Association)
op_collection_id ftusrahouston
language English
topic Moon--Maps
spellingShingle Moon--Maps
Stopar, Julie
orcid:0000-0003-1578-3688
Lunar South Pole Radar Images and Earthshine Model (85°S to Pole)
topic_facet Moon--Maps
description The larger map is centered on the south pole and is based on radar images obtained using Arecibo Observatory and Green Bank Telescope (Cornell University/Smithsonian Institution). The inset map shows solar permanently shaded regions (PSRs) larger than 10 km^2 as well as an earthshine model based on Lunar Reconnaissance Orbiter Laser Altimeter (LOLA) data (NASA Goddard Space Flight Center). Polar stereographic projection is used with scale true at the pole. S-band Earth-based Radar Backscatter Mosaic -- Model of Earthshine
format Map
author Stopar, Julie
orcid:0000-0003-1578-3688
author_facet Stopar, Julie
orcid:0000-0003-1578-3688
author_sort Stopar, Julie
title Lunar South Pole Radar Images and Earthshine Model (85°S to Pole)
title_short Lunar South Pole Radar Images and Earthshine Model (85°S to Pole)
title_full Lunar South Pole Radar Images and Earthshine Model (85°S to Pole)
title_fullStr Lunar South Pole Radar Images and Earthshine Model (85°S to Pole)
title_full_unstemmed Lunar South Pole Radar Images and Earthshine Model (85°S to Pole)
title_sort lunar south pole radar images and earthshine model (85°s to pole)
publisher Lunar and Planetary Institute, Regional Planetary Image Facility
publishDate 2020
url https://hdl.handle.net/20.500.11753/1488
op_coverage Moon
long_lat ENVELOPE(-44.700,-44.700,-60.717,-60.717)
geographic Lola
South Pole
geographic_facet Lola
South Pole
genre South pole
genre_facet South pole
op_relation LPI contribution
no. 2347
Stopar J. (2020) Lunar South Pole Radar Images and Earthshine Mode (85°S to Pole), Lunar and Planetary Institute Regional Planetary Image Facility, LPI Contribution 2347. https://hdl.handle.net/20.500.11753/1488
https://hdl.handle.net/20.500.11753/1488
op_doi https://doi.org/20.500.11753/1488
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