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...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
1. Verfasser: Kilb, R W
Format: Report
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title
container_volume
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.
format Report
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>
fulltext fulltext_linktorsrc
identifier
ispartof
issn
language eng
recordid cdi_dtic_stinet_ADA141339
source DTIC Technical Reports
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
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T19%3A44%3A26IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-dtic_1RU&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=unknown&rft.btitle=E-Fields%20Parallel-to-B%20Effects%20on%20Plasma%20Shear%20Across%20Magnetic%20Flux%20Tubes&rft.au=Kilb,%20R%20W&rft.aucorp=MISSION%20RESEARCH%20CORP%20SANTA%20BARBARA%20CA&rft.date=1983-10-26&rft_id=info:doi/&rft_dat=%3Cdtic_1RU%3EADA141339%3C/dtic_1RU%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true