Mapping the Range of Simple Fresh Lunar Crater Ejecta by Analyzing the Scattering Characteristics of the Lunar Regolith Using Mini-RF Data
Lunar crater ejecta can provide important information regarding the impact cratering process and the properties of subsurface materials. However, the mapping of the range of the crater ejecta has been hampered by the degradation of the lunar surface’s morphological features. Polarimetric synthetic a...
Gespeichert in:
Veröffentlicht in: | IEEE geoscience and remote sensing letters 2024, Vol.21, p.1-5 |
---|---|
Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 5 |
---|---|
container_issue | |
container_start_page | 1 |
container_title | IEEE geoscience and remote sensing letters |
container_volume | 21 |
creator | Song, Zhaobo Huang, Zhanchi Shu, Gaofeng Guo, Zhengwei Li, Ning |
description | Lunar crater ejecta can provide important information regarding the impact cratering process and the properties of subsurface materials. However, the mapping of the range of the crater ejecta has been hampered by the degradation of the lunar surface’s morphological features. Polarimetric synthetic aperture radar (SAR) is an effective technique to determine the scattering characteristics of the lunar surface and subsurface, and for distinguishing the fresh crater ejecta from surrounding regions. This letter uses a three-component compact decomposition to process the mini-radio frequency (Mini-RF) data to identify the scattering characteristics of the crater floor, crater wall, crater ejecta of the simple fresh crater, and lunar background regolith. Then, a method for mapping the range of crater ejecta is proposed to obtain the boundary between the crater ejecta and other regions by analyzing the differences in polarimetric scattering characteristics. Using this method, the crater ejecta of six craters were extracted and verified with the range of the ejecta obtained through visual interpretation on SAR imagery, the accuracy of the ejecta range obtained by the proposed method is 82%–95%. The results show that the proposed method can effectively depict the range of the simple fresh lunar crater ejecta. |
doi_str_mv | 10.1109/LGRS.2024.3356201 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2921290791</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2921290791</sourcerecordid><originalsourceid>FETCH-LOGICAL-c225t-c2b3b51d29af1c975549280f59e39cb91941265edcfa2ae15e98a66a7474c4003</originalsourceid><addsrcrecordid>eNo1kEFOwzAQRS0EEqVwAHaWWKfYTpzEyyrQgpQKKaUSO2viOk2qNAm2uyhH4NTEatnMzNe8-dJ8hB4pmVFKxHO-LNYzRlg0C0MeM0Kv0IRyngaEJ_TazxEPuEi_btGdtXsykmmaTNDvCoah6XbY1RoX0O007iu8bg5Dq_HCaFvj_NiBwZkBpw1-3WvlAJcnPO-gPf38n64VuHHvZVaDAeWFdY2y3s8TZ5tC7_q2cTXeWM-umq4JigV-AQf36KaC1uqHS5-izeL1M3sL8o_lezbPA8UYd2Mtw5LTLRNQUSUSziPBUlJxoUOhSkFFRFnM9VZVwEBTrkUKcQxJlEQqIiScoqez72D676O2Tu77oxm_sZIJRpkgiaAjRc-UMr21RldyMM0BzElSIn3k0kcufeTyEnn4Bx2-dGc</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2921290791</pqid></control><display><type>article</type><title>Mapping the Range of Simple Fresh Lunar Crater Ejecta by Analyzing the Scattering Characteristics of the Lunar Regolith Using Mini-RF Data</title><source>IEEE Electronic Library (IEL)</source><creator>Song, Zhaobo ; Huang, Zhanchi ; Shu, Gaofeng ; Guo, Zhengwei ; Li, Ning</creator><creatorcontrib>Song, Zhaobo ; Huang, Zhanchi ; Shu, Gaofeng ; Guo, Zhengwei ; Li, Ning</creatorcontrib><description>Lunar crater ejecta can provide important information regarding the impact cratering process and the properties of subsurface materials. However, the mapping of the range of the crater ejecta has been hampered by the degradation of the lunar surface’s morphological features. Polarimetric synthetic aperture radar (SAR) is an effective technique to determine the scattering characteristics of the lunar surface and subsurface, and for distinguishing the fresh crater ejecta from surrounding regions. This letter uses a three-component compact decomposition to process the mini-radio frequency (Mini-RF) data to identify the scattering characteristics of the crater floor, crater wall, crater ejecta of the simple fresh crater, and lunar background regolith. Then, a method for mapping the range of crater ejecta is proposed to obtain the boundary between the crater ejecta and other regions by analyzing the differences in polarimetric scattering characteristics. Using this method, the crater ejecta of six craters were extracted and verified with the range of the ejecta obtained through visual interpretation on SAR imagery, the accuracy of the ejecta range obtained by the proposed method is 82%–95%. The results show that the proposed method can effectively depict the range of the simple fresh lunar crater ejecta.</description><identifier>ISSN: 1545-598X</identifier><identifier>EISSN: 1558-0571</identifier><identifier>DOI: 10.1109/LGRS.2024.3356201</identifier><language>eng</language><publisher>Piscataway: The Institute of Electrical and Electronics Engineers, Inc. (IEEE)</publisher><subject>Ejecta ; Lunar craters ; Lunar regolith ; Lunar surface ; Mapping ; Mental task performance ; Polarimetry ; Radio frequency ; Regolith ; SAR (radar) ; Scattering ; Synthetic aperture radar ; Visual system</subject><ispartof>IEEE geoscience and remote sensing letters, 2024, Vol.21, p.1-5</ispartof><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. (IEEE) 2024</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c225t-c2b3b51d29af1c975549280f59e39cb91941265edcfa2ae15e98a66a7474c4003</cites><orcidid>0000-0002-4358-6449 ; 0000-0002-7098-7029</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,4010,27900,27901,27902</link.rule.ids></links><search><creatorcontrib>Song, Zhaobo</creatorcontrib><creatorcontrib>Huang, Zhanchi</creatorcontrib><creatorcontrib>Shu, Gaofeng</creatorcontrib><creatorcontrib>Guo, Zhengwei</creatorcontrib><creatorcontrib>Li, Ning</creatorcontrib><title>Mapping the Range of Simple Fresh Lunar Crater Ejecta by Analyzing the Scattering Characteristics of the Lunar Regolith Using Mini-RF Data</title><title>IEEE geoscience and remote sensing letters</title><description>Lunar crater ejecta can provide important information regarding the impact cratering process and the properties of subsurface materials. However, the mapping of the range of the crater ejecta has been hampered by the degradation of the lunar surface’s morphological features. Polarimetric synthetic aperture radar (SAR) is an effective technique to determine the scattering characteristics of the lunar surface and subsurface, and for distinguishing the fresh crater ejecta from surrounding regions. This letter uses a three-component compact decomposition to process the mini-radio frequency (Mini-RF) data to identify the scattering characteristics of the crater floor, crater wall, crater ejecta of the simple fresh crater, and lunar background regolith. Then, a method for mapping the range of crater ejecta is proposed to obtain the boundary between the crater ejecta and other regions by analyzing the differences in polarimetric scattering characteristics. Using this method, the crater ejecta of six craters were extracted and verified with the range of the ejecta obtained through visual interpretation on SAR imagery, the accuracy of the ejecta range obtained by the proposed method is 82%–95%. The results show that the proposed method can effectively depict the range of the simple fresh lunar crater ejecta.</description><subject>Ejecta</subject><subject>Lunar craters</subject><subject>Lunar regolith</subject><subject>Lunar surface</subject><subject>Mapping</subject><subject>Mental task performance</subject><subject>Polarimetry</subject><subject>Radio frequency</subject><subject>Regolith</subject><subject>SAR (radar)</subject><subject>Scattering</subject><subject>Synthetic aperture radar</subject><subject>Visual system</subject><issn>1545-598X</issn><issn>1558-0571</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNo1kEFOwzAQRS0EEqVwAHaWWKfYTpzEyyrQgpQKKaUSO2viOk2qNAm2uyhH4NTEatnMzNe8-dJ8hB4pmVFKxHO-LNYzRlg0C0MeM0Kv0IRyngaEJ_TazxEPuEi_btGdtXsykmmaTNDvCoah6XbY1RoX0O007iu8bg5Dq_HCaFvj_NiBwZkBpw1-3WvlAJcnPO-gPf38n64VuHHvZVaDAeWFdY2y3s8TZ5tC7_q2cTXeWM-umq4JigV-AQf36KaC1uqHS5-izeL1M3sL8o_lezbPA8UYd2Mtw5LTLRNQUSUSziPBUlJxoUOhSkFFRFnM9VZVwEBTrkUKcQxJlEQqIiScoqez72D676O2Tu77oxm_sZIJRpkgiaAjRc-UMr21RldyMM0BzElSIn3k0kcufeTyEnn4Bx2-dGc</recordid><startdate>2024</startdate><enddate>2024</enddate><creator>Song, Zhaobo</creator><creator>Huang, Zhanchi</creator><creator>Shu, Gaofeng</creator><creator>Guo, Zhengwei</creator><creator>Li, Ning</creator><general>The Institute of Electrical and Electronics Engineers, Inc. (IEEE)</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7SC</scope><scope>7SP</scope><scope>7TG</scope><scope>7UA</scope><scope>8FD</scope><scope>C1K</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>JQ2</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope><scope>L~C</scope><scope>L~D</scope><orcidid>https://orcid.org/0000-0002-4358-6449</orcidid><orcidid>https://orcid.org/0000-0002-7098-7029</orcidid></search><sort><creationdate>2024</creationdate><title>Mapping the Range of Simple Fresh Lunar Crater Ejecta by Analyzing the Scattering Characteristics of the Lunar Regolith Using Mini-RF Data</title><author>Song, Zhaobo ; Huang, Zhanchi ; Shu, Gaofeng ; Guo, Zhengwei ; Li, Ning</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c225t-c2b3b51d29af1c975549280f59e39cb91941265edcfa2ae15e98a66a7474c4003</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Ejecta</topic><topic>Lunar craters</topic><topic>Lunar regolith</topic><topic>Lunar surface</topic><topic>Mapping</topic><topic>Mental task performance</topic><topic>Polarimetry</topic><topic>Radio frequency</topic><topic>Regolith</topic><topic>SAR (radar)</topic><topic>Scattering</topic><topic>Synthetic aperture radar</topic><topic>Visual system</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Song, Zhaobo</creatorcontrib><creatorcontrib>Huang, Zhanchi</creatorcontrib><creatorcontrib>Shu, Gaofeng</creatorcontrib><creatorcontrib>Guo, Zhengwei</creatorcontrib><creatorcontrib>Li, Ning</creatorcontrib><collection>CrossRef</collection><collection>Computer and Information Systems Abstracts</collection><collection>Electronics & Communications Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>Technology Research Database</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>ProQuest Computer Science Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Computer and Information Systems Abstracts Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><jtitle>IEEE geoscience and remote sensing letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Song, Zhaobo</au><au>Huang, Zhanchi</au><au>Shu, Gaofeng</au><au>Guo, Zhengwei</au><au>Li, Ning</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Mapping the Range of Simple Fresh Lunar Crater Ejecta by Analyzing the Scattering Characteristics of the Lunar Regolith Using Mini-RF Data</atitle><jtitle>IEEE geoscience and remote sensing letters</jtitle><date>2024</date><risdate>2024</risdate><volume>21</volume><spage>1</spage><epage>5</epage><pages>1-5</pages><issn>1545-598X</issn><eissn>1558-0571</eissn><abstract>Lunar crater ejecta can provide important information regarding the impact cratering process and the properties of subsurface materials. However, the mapping of the range of the crater ejecta has been hampered by the degradation of the lunar surface’s morphological features. Polarimetric synthetic aperture radar (SAR) is an effective technique to determine the scattering characteristics of the lunar surface and subsurface, and for distinguishing the fresh crater ejecta from surrounding regions. This letter uses a three-component compact decomposition to process the mini-radio frequency (Mini-RF) data to identify the scattering characteristics of the crater floor, crater wall, crater ejecta of the simple fresh crater, and lunar background regolith. Then, a method for mapping the range of crater ejecta is proposed to obtain the boundary between the crater ejecta and other regions by analyzing the differences in polarimetric scattering characteristics. Using this method, the crater ejecta of six craters were extracted and verified with the range of the ejecta obtained through visual interpretation on SAR imagery, the accuracy of the ejecta range obtained by the proposed method is 82%–95%. The results show that the proposed method can effectively depict the range of the simple fresh lunar crater ejecta.</abstract><cop>Piscataway</cop><pub>The Institute of Electrical and Electronics Engineers, Inc. (IEEE)</pub><doi>10.1109/LGRS.2024.3356201</doi><tpages>5</tpages><orcidid>https://orcid.org/0000-0002-4358-6449</orcidid><orcidid>https://orcid.org/0000-0002-7098-7029</orcidid></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1545-598X |
ispartof | IEEE geoscience and remote sensing letters, 2024, Vol.21, p.1-5 |
issn | 1545-598X 1558-0571 |
language | eng |
recordid | cdi_proquest_journals_2921290791 |
source | IEEE Electronic Library (IEL) |
subjects | Ejecta Lunar craters Lunar regolith Lunar surface Mapping Mental task performance Polarimetry Radio frequency Regolith SAR (radar) Scattering Synthetic aperture radar Visual system |
title | Mapping the Range of Simple Fresh Lunar Crater Ejecta by Analyzing the Scattering Characteristics of the Lunar Regolith Using Mini-RF Data |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-03T05%3A36%3A09IST&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=Mapping%20the%20Range%20of%20Simple%20Fresh%20Lunar%20Crater%20Ejecta%20by%20Analyzing%20the%20Scattering%20Characteristics%20of%20the%20Lunar%20Regolith%20Using%20Mini-RF%20Data&rft.jtitle=IEEE%20geoscience%20and%20remote%20sensing%20letters&rft.au=Song,%20Zhaobo&rft.date=2024&rft.volume=21&rft.spage=1&rft.epage=5&rft.pages=1-5&rft.issn=1545-598X&rft.eissn=1558-0571&rft_id=info:doi/10.1109/LGRS.2024.3356201&rft_dat=%3Cproquest_cross%3E2921290791%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2921290791&rft_id=info:pmid/&rfr_iscdi=true |