Microwave brightness of Saturn's rings
It is shown that a lower limit exists on the microwave brightness of the rings of Saturn, if they are assumed to be composed of Mie scatterers of geological composition. The lower limit (about 15°K) is due to scattering of planetary microwave emission. Significant variation of brightness with azimut...
Gespeichert in:
Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 1974-06, Vol.22 (2), p.149-158 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 158 |
---|---|
container_issue | 2 |
container_start_page | 149 |
container_title | Icarus (New York, N.Y. 1962) |
container_volume | 22 |
creator | Cuzzi, Jeffrey N. Van Blerkom, David |
description | It is shown that a lower limit exists on the microwave brightness of the rings of Saturn, if they are assumed to be composed of Mie scatterers of geological composition. The lower limit (about 15°K) is due to scattering of planetary microwave emission. Significant variation of brightness with azimuth along the rings is expected if the particles are typically of 2–3cm radius. Implications for the multiple-scattering hypothesis of the radar cross section of the rings are noted. |
doi_str_mv | 10.1016/0019-1035(74)90114-6 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_22157399</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>0019103574901146</els_id><sourcerecordid>22157399</sourcerecordid><originalsourceid>FETCH-LOGICAL-a358t-194e97acbc43ec166e3e0c861965705eaa380f7b4e0a915ea2810f770088ece33</originalsourceid><addsrcrecordid>eNp9kEtPwzAQhC0EEqXwDzjkVOAQ2I0dPy5IqCoPqYgDcLZcd1OM2qTYSRH_npQijpxWI30z2hnGThEuEVBeAaDJEXh5rsSFAUSRyz02QDCQF1LwfTb4Qw7ZUUrvAFBqwwds9Bh8bD7dhrJZDIu3tqaUsqbKnl3bxfosZTHUi3TMDiq3THTye4fs9XbyMr7Pp093D-Obae54qdscjSCjnJ95wcmjlMQJvJZoZKmgJOe4hkrNBIEz2OtCY68VgNbkifMhG-1y17H56Ci1dhWSp-XS1dR0yRYFloob04NiB_bfpxSpsusYVi5-WQS7HcVuG9ttY6uE_RnFyt52vbNRX2ITKNrkA9We5iGSb-28Cf8HfAPPoWbl</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>22157399</pqid></control><display><type>article</type><title>Microwave brightness of Saturn's rings</title><source>Elsevier ScienceDirect Journals</source><creator>Cuzzi, Jeffrey N. ; Van Blerkom, David</creator><creatorcontrib>Cuzzi, Jeffrey N. ; Van Blerkom, David</creatorcontrib><description>It is shown that a lower limit exists on the microwave brightness of the rings of Saturn, if they are assumed to be composed of Mie scatterers of geological composition. The lower limit (about 15°K) is due to scattering of planetary microwave emission. Significant variation of brightness with azimuth along the rings is expected if the particles are typically of 2–3cm radius. Implications for the multiple-scattering hypothesis of the radar cross section of the rings are noted.</description><identifier>ISSN: 0019-1035</identifier><identifier>EISSN: 1090-2643</identifier><identifier>DOI: 10.1016/0019-1035(74)90114-6</identifier><language>eng</language><publisher>Elsevier Inc</publisher><ispartof>Icarus (New York, N.Y. 1962), 1974-06, Vol.22 (2), p.149-158</ispartof><rights>1974</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a358t-194e97acbc43ec166e3e0c861965705eaa380f7b4e0a915ea2810f770088ece33</citedby><cites>FETCH-LOGICAL-a358t-194e97acbc43ec166e3e0c861965705eaa380f7b4e0a915ea2810f770088ece33</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/0019103574901146$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,776,780,3537,27901,27902,65306</link.rule.ids></links><search><creatorcontrib>Cuzzi, Jeffrey N.</creatorcontrib><creatorcontrib>Van Blerkom, David</creatorcontrib><title>Microwave brightness of Saturn's rings</title><title>Icarus (New York, N.Y. 1962)</title><description>It is shown that a lower limit exists on the microwave brightness of the rings of Saturn, if they are assumed to be composed of Mie scatterers of geological composition. The lower limit (about 15°K) is due to scattering of planetary microwave emission. Significant variation of brightness with azimuth along the rings is expected if the particles are typically of 2–3cm radius. Implications for the multiple-scattering hypothesis of the radar cross section of the rings are noted.</description><issn>0019-1035</issn><issn>1090-2643</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1974</creationdate><recordtype>article</recordtype><recordid>eNp9kEtPwzAQhC0EEqXwDzjkVOAQ2I0dPy5IqCoPqYgDcLZcd1OM2qTYSRH_npQijpxWI30z2hnGThEuEVBeAaDJEXh5rsSFAUSRyz02QDCQF1LwfTb4Qw7ZUUrvAFBqwwds9Bh8bD7dhrJZDIu3tqaUsqbKnl3bxfosZTHUi3TMDiq3THTye4fs9XbyMr7Pp093D-Obae54qdscjSCjnJ95wcmjlMQJvJZoZKmgJOe4hkrNBIEz2OtCY68VgNbkifMhG-1y17H56Ci1dhWSp-XS1dR0yRYFloob04NiB_bfpxSpsusYVi5-WQS7HcVuG9ttY6uE_RnFyt52vbNRX2ITKNrkA9We5iGSb-28Cf8HfAPPoWbl</recordid><startdate>19740601</startdate><enddate>19740601</enddate><creator>Cuzzi, Jeffrey N.</creator><creator>Van Blerkom, David</creator><general>Elsevier Inc</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19740601</creationdate><title>Microwave brightness of Saturn's rings</title><author>Cuzzi, Jeffrey N. ; Van Blerkom, David</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a358t-194e97acbc43ec166e3e0c861965705eaa380f7b4e0a915ea2810f770088ece33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1974</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Cuzzi, Jeffrey N.</creatorcontrib><creatorcontrib>Van Blerkom, David</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Icarus (New York, N.Y. 1962)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Cuzzi, Jeffrey N.</au><au>Van Blerkom, David</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Microwave brightness of Saturn's rings</atitle><jtitle>Icarus (New York, N.Y. 1962)</jtitle><date>1974-06-01</date><risdate>1974</risdate><volume>22</volume><issue>2</issue><spage>149</spage><epage>158</epage><pages>149-158</pages><issn>0019-1035</issn><eissn>1090-2643</eissn><abstract>It is shown that a lower limit exists on the microwave brightness of the rings of Saturn, if they are assumed to be composed of Mie scatterers of geological composition. The lower limit (about 15°K) is due to scattering of planetary microwave emission. Significant variation of brightness with azimuth along the rings is expected if the particles are typically of 2–3cm radius. Implications for the multiple-scattering hypothesis of the radar cross section of the rings are noted.</abstract><pub>Elsevier Inc</pub><doi>10.1016/0019-1035(74)90114-6</doi><tpages>10</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0019-1035 |
ispartof | Icarus (New York, N.Y. 1962), 1974-06, Vol.22 (2), p.149-158 |
issn | 0019-1035 1090-2643 |
language | eng |
recordid | cdi_proquest_miscellaneous_22157399 |
source | Elsevier ScienceDirect Journals |
title | Microwave brightness of Saturn's rings |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-08T01%3A38%3A18IST&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=Microwave%20brightness%20of%20Saturn's%20rings&rft.jtitle=Icarus%20(New%20York,%20N.Y.%201962)&rft.au=Cuzzi,%20Jeffrey%20N.&rft.date=1974-06-01&rft.volume=22&rft.issue=2&rft.spage=149&rft.epage=158&rft.pages=149-158&rft.issn=0019-1035&rft.eissn=1090-2643&rft_id=info:doi/10.1016/0019-1035(74)90114-6&rft_dat=%3Cproquest_cross%3E22157399%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=22157399&rft_id=info:pmid/&rft_els_id=0019103574901146&rfr_iscdi=true |