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Cited by 520

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

The Clementine Bistatic Radar Experiment

Open access
Nozette, S., Lichtenberg, C. L., Spudis, P., Bonner, R., Ort, W., Malaret, E., Robinson, M., Shoemaker, E. M.·1996·Science

Abstract

During the Clementine 1 mission, a bistatic radar experiment measured the magnitude and polarization of the radar echo versus bistatic angle, β, for selected lunar areas. Observations of the lunar south pole yield a same-sense polarization enhancement around β = 0. Analysis shows that the observed enhancement is localized to the permanently shadowed regions of the lunar south pole. Radar observations of periodically solar-illuminated lunar surfaces, including the north pole, yielded no such enhancement. A probable explanation for these differences is the presence of low-loss volume scatterers, such as water ice, in the permanently shadowed region at the south pole.

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Crossref · 10.1126/science.274.5292.1495

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Metadata

Authors
Nozette, S., Lichtenberg, C. L., Spudis, P., Bonner, R., Ort, W., Malaret, E., Robinson, M., & Shoemaker, E. M.
Venue
Science
Published
1996-11-29
Volume
274
Issue
5292
Pages
1495-1498
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2037460055
Cited by
520
References
1
FWCI
18.49
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The Clementine Bistatic Radar Experiment. https://app.cochat.ai/papers/10.1126/science.274.5292.1495
The paper
Nozette, S., Lichtenberg, C. L., Spudis, P., Bonner, R., Ort, W., Malaret, E., Robinson, M., & Shoemaker, E. M. (1996). The Clementine Bistatic Radar Experiment. Science. https://doi.org/10.1126/science.274.5292.1495

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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