Galactic HZE Propagation through the Earth's Atmosphere
A comprehensive physical model for galactic heavy ion propagation is presented. The nuclear fragmentation model is a simplified physical model but contains the major processes of importance to galactic ions. Comparison is made to measurements of atmospheric ion fluence and the limitations of these c...
Gespeichert in:
| Veröffentlicht in: | Radiation research 1987, Vol.109 (2), p.173-183 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 183 |
|---|---|
| container_issue | 2 |
| container_start_page | 173 |
| container_title | Radiation research |
| container_volume | 109 |
| creator | Wilson, John W. Townsend, Lawrence W. Badavi, Forooz F. |
| description | A comprehensive physical model for galactic heavy ion propagation is presented. The nuclear fragmentation model is a simplified physical model but contains the major processes of importance to galactic ions. Comparison is made to measurements of atmospheric ion fluence and the limitations of these comparisons are discussed. |
| doi_str_mv | 10.2307/3576944 |
| format | Article |
| fullrecord | <record><control><sourceid>jstor_cross</sourceid><recordid>TN_cdi_crossref_primary_10_2307_3576944</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>3576944</jstor_id><sourcerecordid>3576944</sourcerecordid><originalsourceid>FETCH-LOGICAL-c356t-7f409dc0a8bd1520c7c6330f77754e6eaf54874f239532fdd7a8ea4de432b7783</originalsourceid><addsrcrecordid>eNp1z8FLwzAUBvAgiptT_AdEehB2qr40SZMcx5ibMNCDXryUtzRZO7a2JNnB_97Kip48fTz48fE-Qm4pPGYM5BMTMtecn5Ex1UylggM_J2MAxlIplByRqxB20N8015dkRKlgSol8TOQS92hibZLV5yJ5822HW4x12ySx8u1xW_VpkwX6WE1DMouHNnSV9faaXDjcB3sz5IR8PC_e56t0_bp8mc_WqWEij6l0HHRpANWmpCIDI03OGDgppeA2t-gEV5K7jGnBMleWEpVFXlrOso2Uik3I9NRrfBuCt67ofH1A_1VQKH6mF8P0Xt6fZHfcHGz554atPXgYAAaDe-exMXX4dVIwoEB7dndiDQYsmuhDkQFwAKU15X8tuxBb_-833xl7ca0</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Galactic HZE Propagation through the Earth's Atmosphere</title><source>MEDLINE</source><source>JSTOR Archive Collection A-Z Listing</source><source>NASA Technical Reports Server</source><creator>Wilson, John W. ; Townsend, Lawrence W. ; Badavi, Forooz F.</creator><creatorcontrib>Wilson, John W. ; Townsend, Lawrence W. ; Badavi, Forooz F.</creatorcontrib><description>A comprehensive physical model for galactic heavy ion propagation is presented. The nuclear fragmentation model is a simplified physical model but contains the major processes of importance to galactic ions. Comparison is made to measurements of atmospheric ion fluence and the limitations of these comparisons are discussed.</description><identifier>ISSN: 0033-7587</identifier><identifier>EISSN: 1938-5404</identifier><identifier>DOI: 10.2307/3576944</identifier><identifier>PMID: 11538856</identifier><identifier>CODEN: RAREAE</identifier><language>eng</language><publisher>Legacy CDMS: Academic Press, Inc</publisher><subject>Aerospace Medicine ; Applied sciences ; Approximation ; Atmospheric models ; Atmospherics ; Beryllium ; Boron ; Carbon ; Cosmic Radiation ; Cosmic rays ; Earth atmosphere ; Elementary Particles ; Energy ; Exact sciences and technology ; Heavy ions ; Ions ; Linear Energy Transfer ; Lithium ; Mathematics ; Models, Theoretical ; Nuclear Physics ; Nucleons ; Other techniques and industries ; Projectiles ; Radiation Protection</subject><ispartof>Radiation research, 1987, Vol.109 (2), p.173-183</ispartof><rights>Copyright 1987 Academic Press, Inc.</rights><rights>1988 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c356t-7f409dc0a8bd1520c7c6330f77754e6eaf54874f239532fdd7a8ea4de432b7783</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/3576944$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/3576944$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,780,784,803,4024,27923,27924,27925,58017,58250</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=7530101$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/11538856$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Wilson, John W.</creatorcontrib><creatorcontrib>Townsend, Lawrence W.</creatorcontrib><creatorcontrib>Badavi, Forooz F.</creatorcontrib><title>Galactic HZE Propagation through the Earth's Atmosphere</title><title>Radiation research</title><addtitle>Radiat Res</addtitle><description>A comprehensive physical model for galactic heavy ion propagation is presented. The nuclear fragmentation model is a simplified physical model but contains the major processes of importance to galactic ions. Comparison is made to measurements of atmospheric ion fluence and the limitations of these comparisons are discussed.</description><subject>Aerospace Medicine</subject><subject>Applied sciences</subject><subject>Approximation</subject><subject>Atmospheric models</subject><subject>Atmospherics</subject><subject>Beryllium</subject><subject>Boron</subject><subject>Carbon</subject><subject>Cosmic Radiation</subject><subject>Cosmic rays</subject><subject>Earth atmosphere</subject><subject>Elementary Particles</subject><subject>Energy</subject><subject>Exact sciences and technology</subject><subject>Heavy ions</subject><subject>Ions</subject><subject>Linear Energy Transfer</subject><subject>Lithium</subject><subject>Mathematics</subject><subject>Models, Theoretical</subject><subject>Nuclear Physics</subject><subject>Nucleons</subject><subject>Other techniques and industries</subject><subject>Projectiles</subject><subject>Radiation Protection</subject><issn>0033-7587</issn><issn>1938-5404</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1987</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><sourceid>EIF</sourceid><recordid>eNp1z8FLwzAUBvAgiptT_AdEehB2qr40SZMcx5ibMNCDXryUtzRZO7a2JNnB_97Kip48fTz48fE-Qm4pPGYM5BMTMtecn5Ex1UylggM_J2MAxlIplByRqxB20N8015dkRKlgSol8TOQS92hibZLV5yJ5822HW4x12ySx8u1xW_VpkwX6WE1DMouHNnSV9faaXDjcB3sz5IR8PC_e56t0_bp8mc_WqWEij6l0HHRpANWmpCIDI03OGDgppeA2t-gEV5K7jGnBMleWEpVFXlrOso2Uik3I9NRrfBuCt67ofH1A_1VQKH6mF8P0Xt6fZHfcHGz554atPXgYAAaDe-exMXX4dVIwoEB7dndiDQYsmuhDkQFwAKU15X8tuxBb_-833xl7ca0</recordid><startdate>1987</startdate><enddate>1987</enddate><creator>Wilson, John W.</creator><creator>Townsend, Lawrence W.</creator><creator>Badavi, Forooz F.</creator><general>Academic Press, Inc</general><general>Radiation Research Society</general><scope>CYE</scope><scope>CYI</scope><scope>IQODW</scope><scope>CGR</scope><scope>CUY</scope><scope>CVF</scope><scope>ECM</scope><scope>EIF</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>1987</creationdate><title>Galactic HZE Propagation through the Earth's Atmosphere</title><author>Wilson, John W. ; Townsend, Lawrence W. ; Badavi, Forooz F.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c356t-7f409dc0a8bd1520c7c6330f77754e6eaf54874f239532fdd7a8ea4de432b7783</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1987</creationdate><topic>Aerospace Medicine</topic><topic>Applied sciences</topic><topic>Approximation</topic><topic>Atmospheric models</topic><topic>Atmospherics</topic><topic>Beryllium</topic><topic>Boron</topic><topic>Carbon</topic><topic>Cosmic Radiation</topic><topic>Cosmic rays</topic><topic>Earth atmosphere</topic><topic>Elementary Particles</topic><topic>Energy</topic><topic>Exact sciences and technology</topic><topic>Heavy ions</topic><topic>Ions</topic><topic>Linear Energy Transfer</topic><topic>Lithium</topic><topic>Mathematics</topic><topic>Models, Theoretical</topic><topic>Nuclear Physics</topic><topic>Nucleons</topic><topic>Other techniques and industries</topic><topic>Projectiles</topic><topic>Radiation Protection</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wilson, John W.</creatorcontrib><creatorcontrib>Townsend, Lawrence W.</creatorcontrib><creatorcontrib>Badavi, Forooz F.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>Medline</collection><collection>MEDLINE</collection><collection>MEDLINE (Ovid)</collection><collection>MEDLINE</collection><collection>MEDLINE</collection><collection>PubMed</collection><collection>CrossRef</collection><jtitle>Radiation research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wilson, John W.</au><au>Townsend, Lawrence W.</au><au>Badavi, Forooz F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Galactic HZE Propagation through the Earth's Atmosphere</atitle><jtitle>Radiation research</jtitle><addtitle>Radiat Res</addtitle><date>1987</date><risdate>1987</risdate><volume>109</volume><issue>2</issue><spage>173</spage><epage>183</epage><pages>173-183</pages><issn>0033-7587</issn><eissn>1938-5404</eissn><coden>RAREAE</coden><abstract>A comprehensive physical model for galactic heavy ion propagation is presented. The nuclear fragmentation model is a simplified physical model but contains the major processes of importance to galactic ions. Comparison is made to measurements of atmospheric ion fluence and the limitations of these comparisons are discussed.</abstract><cop>Legacy CDMS</cop><pub>Academic Press, Inc</pub><pmid>11538856</pmid><doi>10.2307/3576944</doi><tpages>11</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0033-7587 |
| ispartof | Radiation research, 1987, Vol.109 (2), p.173-183 |
| issn | 0033-7587 1938-5404 |
| language | eng |
| recordid | cdi_crossref_primary_10_2307_3576944 |
| source | MEDLINE; JSTOR Archive Collection A-Z Listing; NASA Technical Reports Server |
| subjects | Aerospace Medicine Applied sciences Approximation Atmospheric models Atmospherics Beryllium Boron Carbon Cosmic Radiation Cosmic rays Earth atmosphere Elementary Particles Energy Exact sciences and technology Heavy ions Ions Linear Energy Transfer Lithium Mathematics Models, Theoretical Nuclear Physics Nucleons Other techniques and industries Projectiles Radiation Protection |
| title | Galactic HZE Propagation through the Earth's Atmosphere |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-21T05%3A26%3A13IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Galactic%20HZE%20Propagation%20through%20the%20Earth's%20Atmosphere&rft.jtitle=Radiation%20research&rft.au=Wilson,%20John%20W.&rft.date=1987&rft.volume=109&rft.issue=2&rft.spage=173&rft.epage=183&rft.pages=173-183&rft.issn=0033-7587&rft.eissn=1938-5404&rft.coden=RAREAE&rft_id=info:doi/10.2307/3576944&rft_dat=%3Cjstor_cross%3E3576944%3C/jstor_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/11538856&rft_jstor_id=3576944&rfr_iscdi=true |