E-Fields Parallel-to-B Effects on Plasma Shear Across Magnetic Flux Tubes
Necessary conditions are derived if very long plasma filaments (striations) are to remain magnetic flux tube aligned in distorted geomagnetic fields subsequent to nuclear burst. Special E fields are required, unrelated to resistive effects. It is not yet clear if such special E fields can appear in...
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creator | Kilb, R W |
description | Necessary conditions are derived if very long plasma filaments (striations) are to remain magnetic flux tube aligned in distorted geomagnetic fields subsequent to nuclear burst. Special E fields are required, unrelated to resistive effects. It is not yet clear if such special E fields can appear in reality. If such special E fields cannot exist, long nuclear bursts striations in the magnetosphere will gradually shear across magnetic flux tubes, break up into several shorter segments, descend into the lower ionosphere, and be consumed faster there by molecular deionization. |
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fullrecord | <record><control><sourceid>dtic_1RU</sourceid><recordid>TN_cdi_dtic_stinet_ADA141339</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>ADA141339</sourcerecordid><originalsourceid>FETCH-dtic_stinet_ADA1413393</originalsourceid><addsrcrecordid>eNrjZPB01XXLTM1JKVYISCxKzMlJzdEtydd1UnBNS0tNLilWyM9TCMhJLM5NVAjOSE0sUnBMLsovLlbwTUzPSy3JTFZwyymtUAgpTUot5mFgTUvMKU7lhdLcDDJuriHOHropQHXxxSWZQA3xji6OhiaGxsaWxgSkAf5MMA4</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>report</recordtype></control><display><type>report</type><title>E-Fields Parallel-to-B Effects on Plasma Shear Across Magnetic Flux Tubes</title><source>DTIC Technical Reports</source><creator>Kilb, R W</creator><creatorcontrib>Kilb, R W ; MISSION RESEARCH CORP SANTA BARBARA CA</creatorcontrib><description>Necessary conditions are derived if very long plasma filaments (striations) are to remain magnetic flux tube aligned in distorted geomagnetic fields subsequent to nuclear burst. Special E fields are required, unrelated to resistive effects. It is not yet clear if such special E fields can appear in reality. If such special E fields cannot exist, long nuclear bursts striations in the magnetosphere will gradually shear across magnetic flux tubes, break up into several shorter segments, descend into the lower ionosphere, and be consumed faster there by molecular deionization.</description><language>eng</language><subject>ELECTRIC FIELDS ; ELECTRON DENSITY ; IONOSPHERE ; MAGNETIC FIELDS ; MAGNETOSPHERE ; NUCLEAR EXPLOSIONS ; PE62715H ; PLASMA DIAGNOSTICS ; Plasma Physics and Magnetohydrodynamics ; PLASMAS(PHYSICS) ; STRIATIONS ; WU55</subject><creationdate>1983</creationdate><rights>Approved for public release; distribution is unlimited.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,780,885,27567,27568</link.rule.ids><linktorsrc>$$Uhttps://apps.dtic.mil/sti/citations/ADA141339$$EView_record_in_DTIC$$FView_record_in_$$GDTIC$$Hfree_for_read</linktorsrc></links><search><creatorcontrib>Kilb, R W</creatorcontrib><creatorcontrib>MISSION RESEARCH CORP SANTA BARBARA CA</creatorcontrib><title>E-Fields Parallel-to-B Effects on Plasma Shear Across Magnetic Flux Tubes</title><description>Necessary conditions are derived if very long plasma filaments (striations) are to remain magnetic flux tube aligned in distorted geomagnetic fields subsequent to nuclear burst. Special E fields are required, unrelated to resistive effects. It is not yet clear if such special E fields can appear in reality. If such special E fields cannot exist, long nuclear bursts striations in the magnetosphere will gradually shear across magnetic flux tubes, break up into several shorter segments, descend into the lower ionosphere, and be consumed faster there by molecular deionization.</description><subject>ELECTRIC FIELDS</subject><subject>ELECTRON DENSITY</subject><subject>IONOSPHERE</subject><subject>MAGNETIC FIELDS</subject><subject>MAGNETOSPHERE</subject><subject>NUCLEAR EXPLOSIONS</subject><subject>PE62715H</subject><subject>PLASMA DIAGNOSTICS</subject><subject>Plasma Physics and Magnetohydrodynamics</subject><subject>PLASMAS(PHYSICS)</subject><subject>STRIATIONS</subject><subject>WU55</subject><fulltext>true</fulltext><rsrctype>report</rsrctype><creationdate>1983</creationdate><recordtype>report</recordtype><sourceid>1RU</sourceid><recordid>eNrjZPB01XXLTM1JKVYISCxKzMlJzdEtydd1UnBNS0tNLilWyM9TCMhJLM5NVAjOSE0sUnBMLsovLlbwTUzPSy3JTFZwyymtUAgpTUot5mFgTUvMKU7lhdLcDDJuriHOHropQHXxxSWZQA3xji6OhiaGxsaWxgSkAf5MMA4</recordid><startdate>19831026</startdate><enddate>19831026</enddate><creator>Kilb, R W</creator><scope>1RU</scope><scope>BHM</scope></search><sort><creationdate>19831026</creationdate><title>E-Fields Parallel-to-B Effects on Plasma Shear Across Magnetic Flux Tubes</title><author>Kilb, R W</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-dtic_stinet_ADA1413393</frbrgroupid><rsrctype>reports</rsrctype><prefilter>reports</prefilter><language>eng</language><creationdate>1983</creationdate><topic>ELECTRIC FIELDS</topic><topic>ELECTRON DENSITY</topic><topic>IONOSPHERE</topic><topic>MAGNETIC FIELDS</topic><topic>MAGNETOSPHERE</topic><topic>NUCLEAR EXPLOSIONS</topic><topic>PE62715H</topic><topic>PLASMA DIAGNOSTICS</topic><topic>Plasma Physics and Magnetohydrodynamics</topic><topic>PLASMAS(PHYSICS)</topic><topic>STRIATIONS</topic><topic>WU55</topic><toplevel>online_resources</toplevel><creatorcontrib>Kilb, R W</creatorcontrib><creatorcontrib>MISSION RESEARCH CORP SANTA BARBARA CA</creatorcontrib><collection>DTIC Technical Reports</collection><collection>DTIC STINET</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Kilb, R W</au><aucorp>MISSION RESEARCH CORP SANTA BARBARA CA</aucorp><format>book</format><genre>unknown</genre><ristype>RPRT</ristype><btitle>E-Fields Parallel-to-B Effects on Plasma Shear Across Magnetic Flux Tubes</btitle><date>1983-10-26</date><risdate>1983</risdate><abstract>Necessary conditions are derived if very long plasma filaments (striations) are to remain magnetic flux tube aligned in distorted geomagnetic fields subsequent to nuclear burst. Special E fields are required, unrelated to resistive effects. It is not yet clear if such special E fields can appear in reality. If such special E fields cannot exist, long nuclear bursts striations in the magnetosphere will gradually shear across magnetic flux tubes, break up into several shorter segments, descend into the lower ionosphere, and be consumed faster there by molecular deionization.</abstract><oa>free_for_read</oa></addata></record> |
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subjects | ELECTRIC FIELDS ELECTRON DENSITY IONOSPHERE MAGNETIC FIELDS MAGNETOSPHERE NUCLEAR EXPLOSIONS PE62715H PLASMA DIAGNOSTICS Plasma Physics and Magnetohydrodynamics PLASMAS(PHYSICS) STRIATIONS WU55 |
title | E-Fields Parallel-to-B Effects on Plasma Shear Across Magnetic Flux Tubes |
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