Loading…

Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images

The Clementine mission to the Moon returned global imaging data collected by the ultraviolet visible (UVVIS) camera. This data set is now in a final state of calibration, and a five‐band multispectral digital image model (DIM) of the lunar surface will soon be available to the science community. We...

Full description

Saved in:
Bibliographic Details
Published in:Journal of Geophysical Research 2000-08, Vol.105 (E8), p.20297-20305
Main Authors: Lucey, Paul G., Blewett, David T., Jolliff, Bradley L.
Format: Article
Language:English
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-a4728-488d514f98b89270aea63362461c0417a0e16353296698a2e1e37d9aec2ce5263
cites cdi_FETCH-LOGICAL-a4728-488d514f98b89270aea63362461c0417a0e16353296698a2e1e37d9aec2ce5263
container_end_page 20305
container_issue E8
container_start_page 20297
container_title Journal of Geophysical Research
container_volume 105
creator Lucey, Paul G.
Blewett, David T.
Jolliff, Bradley L.
description The Clementine mission to the Moon returned global imaging data collected by the ultraviolet visible (UVVIS) camera. This data set is now in a final state of calibration, and a five‐band multispectral digital image model (DIM) of the lunar surface will soon be available to the science community. We have used observations of the lunar sample‐return sites and stations extracted from the final DIM in conjunction with compositional information for returned lunar soils to revise our previously published algorithms for the spectral determination of the FeO and TiO2 content of the lunar surface. The algorithms successfully normalize the effects of space weathering so that composition may be determined without regard to a surface's state of maturity. These algorithms permit anyone with access to the standard archived DIM to construct high spatial resolution maps of FeO and TiO2 abundance. Such maps will be of great utility in a variety of lunar geologic studies.
doi_str_mv 10.1029/1999JE001117
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_27558634</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>27558634</sourcerecordid><originalsourceid>FETCH-LOGICAL-a4728-488d514f98b89270aea63362461c0417a0e16353296698a2e1e37d9aec2ce5263</originalsourceid><addsrcrecordid>eNp9kEtv1DAUhS0EEqO2O36AV6wI-BU_lmg6nTIaFQmBpjvrTnIzuHWcYict_fdNNVXFiru5m-87OjqEfODsM2fCfeHOuc2KMc65eUMWgte6EoKJt2TBuLIVE8K8J2el3LD5VK0V4wsybKcEmYY8JAqppWMYIYWpp7CfUgupQQrxMOQw_u4L3UPBls5oFxJEepeHBksJ6UCHji4j9pjGkJBOccxwH4aIY3UfSthHpKGHA5ZT8q6DWPDs5Z-QXxern8vLavt9_W35dVuBMsJWytq25qpzdm-dMAwQtJRaKM0bprgBhlzLWgqntbMgkKM0rQNsRIO10PKEfDzmzh3_TFhG34fSYIyQcJiKF6aurZZqBj8dwSYPpWTs_F2eq-ZHz5l_Htb_O-yMiyP-ECI-_pf1m_WPFefCzlJ1lEIZ8e-rBPnWayNN7XdXa39-fbG73u3O_ZV8AldTiVc</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>27558634</pqid></control><display><type>article</type><title>Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images</title><source>Wiley-Blackwell AGU Digital Archive</source><creator>Lucey, Paul G. ; Blewett, David T. ; Jolliff, Bradley L.</creator><creatorcontrib>Lucey, Paul G. ; Blewett, David T. ; Jolliff, Bradley L.</creatorcontrib><description>The Clementine mission to the Moon returned global imaging data collected by the ultraviolet visible (UVVIS) camera. This data set is now in a final state of calibration, and a five‐band multispectral digital image model (DIM) of the lunar surface will soon be available to the science community. We have used observations of the lunar sample‐return sites and stations extracted from the final DIM in conjunction with compositional information for returned lunar soils to revise our previously published algorithms for the spectral determination of the FeO and TiO2 content of the lunar surface. The algorithms successfully normalize the effects of space weathering so that composition may be determined without regard to a surface's state of maturity. These algorithms permit anyone with access to the standard archived DIM to construct high spatial resolution maps of FeO and TiO2 abundance. Such maps will be of great utility in a variety of lunar geologic studies.</description><identifier>ISSN: 0148-0227</identifier><identifier>EISSN: 2156-2202</identifier><identifier>DOI: 10.1029/1999JE001117</identifier><language>eng</language><publisher>Blackwell Publishing Ltd</publisher><ispartof>Journal of Geophysical Research, 2000-08, Vol.105 (E8), p.20297-20305</ispartof><rights>Copyright 2000 by the American Geophysical Union.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a4728-488d514f98b89270aea63362461c0417a0e16353296698a2e1e37d9aec2ce5263</citedby><cites>FETCH-LOGICAL-a4728-488d514f98b89270aea63362461c0417a0e16353296698a2e1e37d9aec2ce5263</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F1999JE001117$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F1999JE001117$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,780,784,11514,27924,27925,46468,46892</link.rule.ids></links><search><creatorcontrib>Lucey, Paul G.</creatorcontrib><creatorcontrib>Blewett, David T.</creatorcontrib><creatorcontrib>Jolliff, Bradley L.</creatorcontrib><title>Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images</title><title>Journal of Geophysical Research</title><addtitle>J. Geophys. Res</addtitle><description>The Clementine mission to the Moon returned global imaging data collected by the ultraviolet visible (UVVIS) camera. This data set is now in a final state of calibration, and a five‐band multispectral digital image model (DIM) of the lunar surface will soon be available to the science community. We have used observations of the lunar sample‐return sites and stations extracted from the final DIM in conjunction with compositional information for returned lunar soils to revise our previously published algorithms for the spectral determination of the FeO and TiO2 content of the lunar surface. The algorithms successfully normalize the effects of space weathering so that composition may be determined without regard to a surface's state of maturity. These algorithms permit anyone with access to the standard archived DIM to construct high spatial resolution maps of FeO and TiO2 abundance. Such maps will be of great utility in a variety of lunar geologic studies.</description><issn>0148-0227</issn><issn>2156-2202</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><recordid>eNp9kEtv1DAUhS0EEqO2O36AV6wI-BU_lmg6nTIaFQmBpjvrTnIzuHWcYict_fdNNVXFiru5m-87OjqEfODsM2fCfeHOuc2KMc65eUMWgte6EoKJt2TBuLIVE8K8J2el3LD5VK0V4wsybKcEmYY8JAqppWMYIYWpp7CfUgupQQrxMOQw_u4L3UPBls5oFxJEepeHBksJ6UCHji4j9pjGkJBOccxwH4aIY3UfSthHpKGHA5ZT8q6DWPDs5Z-QXxern8vLavt9_W35dVuBMsJWytq25qpzdm-dMAwQtJRaKM0bprgBhlzLWgqntbMgkKM0rQNsRIO10PKEfDzmzh3_TFhG34fSYIyQcJiKF6aurZZqBj8dwSYPpWTs_F2eq-ZHz5l_Htb_O-yMiyP-ECI-_pf1m_WPFefCzlJ1lEIZ8e-rBPnWayNN7XdXa39-fbG73u3O_ZV8AldTiVc</recordid><startdate>20000825</startdate><enddate>20000825</enddate><creator>Lucey, Paul G.</creator><creator>Blewett, David T.</creator><creator>Jolliff, Bradley L.</creator><general>Blackwell Publishing Ltd</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20000825</creationdate><title>Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images</title><author>Lucey, Paul G. ; Blewett, David T. ; Jolliff, Bradley L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a4728-488d514f98b89270aea63362461c0417a0e16353296698a2e1e37d9aec2ce5263</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Lucey, Paul G.</creatorcontrib><creatorcontrib>Blewett, David T.</creatorcontrib><creatorcontrib>Jolliff, Bradley L.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of Geophysical Research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lucey, Paul G.</au><au>Blewett, David T.</au><au>Jolliff, Bradley L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images</atitle><jtitle>Journal of Geophysical Research</jtitle><addtitle>J. Geophys. Res</addtitle><date>2000-08-25</date><risdate>2000</risdate><volume>105</volume><issue>E8</issue><spage>20297</spage><epage>20305</epage><pages>20297-20305</pages><issn>0148-0227</issn><eissn>2156-2202</eissn><abstract>The Clementine mission to the Moon returned global imaging data collected by the ultraviolet visible (UVVIS) camera. This data set is now in a final state of calibration, and a five‐band multispectral digital image model (DIM) of the lunar surface will soon be available to the science community. We have used observations of the lunar sample‐return sites and stations extracted from the final DIM in conjunction with compositional information for returned lunar soils to revise our previously published algorithms for the spectral determination of the FeO and TiO2 content of the lunar surface. The algorithms successfully normalize the effects of space weathering so that composition may be determined without regard to a surface's state of maturity. These algorithms permit anyone with access to the standard archived DIM to construct high spatial resolution maps of FeO and TiO2 abundance. Such maps will be of great utility in a variety of lunar geologic studies.</abstract><pub>Blackwell Publishing Ltd</pub><doi>10.1029/1999JE001117</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0148-0227
ispartof Journal of Geophysical Research, 2000-08, Vol.105 (E8), p.20297-20305
issn 0148-0227
2156-2202
language eng
recordid cdi_proquest_miscellaneous_27558634
source Wiley-Blackwell AGU Digital Archive
title Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T00%3A04%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Lunar%20iron%20and%20titanium%20abundance%20algorithms%20based%20on%20final%20processing%20of%20Clementine%20ultraviolet-visible%20images&rft.jtitle=Journal%20of%20Geophysical%20Research&rft.au=Lucey,%20Paul%20G.&rft.date=2000-08-25&rft.volume=105&rft.issue=E8&rft.spage=20297&rft.epage=20305&rft.pages=20297-20305&rft.issn=0148-0227&rft.eissn=2156-2202&rft_id=info:doi/10.1029/1999JE001117&rft_dat=%3Cproquest_cross%3E27558634%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a4728-488d514f98b89270aea63362461c0417a0e16353296698a2e1e37d9aec2ce5263%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=27558634&rft_id=info:pmid/&rfr_iscdi=true