Charged particle motion in electromagnetic fields varying moderately rapidly in space

Electromagnetic fields are considered which vary on the space scale of the geometric mean of the Larmor radius and the much larger scale length of variation of the magnetic field lines. It is first shown that the magnetic moment is an adiabatic invariant, even though the usual arguments for its exis...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physics of plasmas 2011-10, Vol.18 (10), p.104510-104510-4
Hauptverfasser: Jagannath, Aukosh, Weitzner, Harold
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 104510-4
container_issue 10
container_start_page 104510
container_title Physics of plasmas
container_volume 18
creator Jagannath, Aukosh
Weitzner, Harold
description Electromagnetic fields are considered which vary on the space scale of the geometric mean of the Larmor radius and the much larger scale length of variation of the magnetic field lines. It is first shown that the magnetic moment is an adiabatic invariant, even though the usual arguments for its existence fail. The motion of the guiding center is then examined. For perpendicular drifts in magnitude comparable with the particle speed, the subsequent motion is dominated by electrostatic effects. The motion of particles along the field lines occurs on a much slower time scale than the perpendicular drift time scale. When the guiding center motion is approximately periodic in time, a second adiabatic invariant exists, the magnetic flux enclosed by the almost periodic orbit. When the perpendicular drift is small compared with the particle speed, the parallel motion and the perpendicular drift occur on the same, slow timescale.
doi_str_mv 10.1063/1.3652850
format Article
fullrecord <record><control><sourceid>scitation_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22047022</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>pop</sourcerecordid><originalsourceid>FETCH-LOGICAL-c272t-bc1704e1267fd5d97d169fe9532d184d3b97628a312e500dac5d682a95b7e8043</originalsourceid><addsrcrecordid>eNp1kE1LAzEQhoMoWKsH_8GCJw9bJ9lNsnsRpPgFBS8WvIU0mW0j-0UShP57s2w9epqBeeZl5iHklsKKgige6KoQnFUczsiCQlXnUsjyfOol5EKUX5fkKoRvACgFrxZkuz5ov0ebjdpHZ1rMuiG6oc9cn2GLJvqh0_se0yxrHLY2ZD_aH12_T6BFryO2x8zr0dlU01IYtcFrctHoNuDNqS7J9uX5c_2Wbz5e39dPm9wwyWK-M1RCiZQJ2Vhua2mpqBusecEsrUpb7GopWKULypADWG24FRXTNd9JrKAsluRuzh1CdCoYF9EczND36XDFGJQSGEvU_UwZP4TgsVGjd136QlFQkzVF1claYh9ndgrTk4n_YXVyp_7cqW4ofgFD7XRj</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Charged particle motion in electromagnetic fields varying moderately rapidly in space</title><source>AIP Journals Complete</source><source>AIP Digital Archive</source><source>Alma/SFX Local Collection</source><creator>Jagannath, Aukosh ; Weitzner, Harold</creator><creatorcontrib>Jagannath, Aukosh ; Weitzner, Harold</creatorcontrib><description>Electromagnetic fields are considered which vary on the space scale of the geometric mean of the Larmor radius and the much larger scale length of variation of the magnetic field lines. It is first shown that the magnetic moment is an adiabatic invariant, even though the usual arguments for its existence fail. The motion of the guiding center is then examined. For perpendicular drifts in magnitude comparable with the particle speed, the subsequent motion is dominated by electrostatic effects. The motion of particles along the field lines occurs on a much slower time scale than the perpendicular drift time scale. When the guiding center motion is approximately periodic in time, a second adiabatic invariant exists, the magnetic flux enclosed by the almost periodic orbit. When the perpendicular drift is small compared with the particle speed, the parallel motion and the perpendicular drift occur on the same, slow timescale.</description><identifier>ISSN: 1070-664X</identifier><identifier>EISSN: 1089-7674</identifier><identifier>DOI: 10.1063/1.3652850</identifier><identifier>CODEN: PHPAEN</identifier><language>eng</language><publisher>United States: American Institute of Physics</publisher><subject>70 PLASMA PHYSICS AND FUSION TECHNOLOGY ; CHARGED PARTICLES ; ELECTROMAGNETIC FIELDS ; ELECTROMAGNETIC RADIATION ; ELECTROSTATICS ; LARMOR RADIUS ; LENGTH ; MAGNETIC FIELDS ; MAGNETIC FLUX ; MAGNETIC MOMENTS ; ORBITS ; PERIODICITY ; PLASMA</subject><ispartof>Physics of plasmas, 2011-10, Vol.18 (10), p.104510-104510-4</ispartof><rights>2011 American Institute of Physics</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c272t-bc1704e1267fd5d97d169fe9532d184d3b97628a312e500dac5d682a95b7e8043</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/pop/article-lookup/doi/10.1063/1.3652850$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>230,314,776,780,790,881,1553,4498,27901,27902,76126,76132</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22047022$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Jagannath, Aukosh</creatorcontrib><creatorcontrib>Weitzner, Harold</creatorcontrib><title>Charged particle motion in electromagnetic fields varying moderately rapidly in space</title><title>Physics of plasmas</title><description>Electromagnetic fields are considered which vary on the space scale of the geometric mean of the Larmor radius and the much larger scale length of variation of the magnetic field lines. It is first shown that the magnetic moment is an adiabatic invariant, even though the usual arguments for its existence fail. The motion of the guiding center is then examined. For perpendicular drifts in magnitude comparable with the particle speed, the subsequent motion is dominated by electrostatic effects. The motion of particles along the field lines occurs on a much slower time scale than the perpendicular drift time scale. When the guiding center motion is approximately periodic in time, a second adiabatic invariant exists, the magnetic flux enclosed by the almost periodic orbit. When the perpendicular drift is small compared with the particle speed, the parallel motion and the perpendicular drift occur on the same, slow timescale.</description><subject>70 PLASMA PHYSICS AND FUSION TECHNOLOGY</subject><subject>CHARGED PARTICLES</subject><subject>ELECTROMAGNETIC FIELDS</subject><subject>ELECTROMAGNETIC RADIATION</subject><subject>ELECTROSTATICS</subject><subject>LARMOR RADIUS</subject><subject>LENGTH</subject><subject>MAGNETIC FIELDS</subject><subject>MAGNETIC FLUX</subject><subject>MAGNETIC MOMENTS</subject><subject>ORBITS</subject><subject>PERIODICITY</subject><subject>PLASMA</subject><issn>1070-664X</issn><issn>1089-7674</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp1kE1LAzEQhoMoWKsH_8GCJw9bJ9lNsnsRpPgFBS8WvIU0mW0j-0UShP57s2w9epqBeeZl5iHklsKKgige6KoQnFUczsiCQlXnUsjyfOol5EKUX5fkKoRvACgFrxZkuz5ov0ebjdpHZ1rMuiG6oc9cn2GLJvqh0_se0yxrHLY2ZD_aH12_T6BFryO2x8zr0dlU01IYtcFrctHoNuDNqS7J9uX5c_2Wbz5e39dPm9wwyWK-M1RCiZQJ2Vhua2mpqBusecEsrUpb7GopWKULypADWG24FRXTNd9JrKAsluRuzh1CdCoYF9EczND36XDFGJQSGEvU_UwZP4TgsVGjd136QlFQkzVF1claYh9ndgrTk4n_YXVyp_7cqW4ofgFD7XRj</recordid><startdate>20111001</startdate><enddate>20111001</enddate><creator>Jagannath, Aukosh</creator><creator>Weitzner, Harold</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>20111001</creationdate><title>Charged particle motion in electromagnetic fields varying moderately rapidly in space</title><author>Jagannath, Aukosh ; Weitzner, Harold</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c272t-bc1704e1267fd5d97d169fe9532d184d3b97628a312e500dac5d682a95b7e8043</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>70 PLASMA PHYSICS AND FUSION TECHNOLOGY</topic><topic>CHARGED PARTICLES</topic><topic>ELECTROMAGNETIC FIELDS</topic><topic>ELECTROMAGNETIC RADIATION</topic><topic>ELECTROSTATICS</topic><topic>LARMOR RADIUS</topic><topic>LENGTH</topic><topic>MAGNETIC FIELDS</topic><topic>MAGNETIC FLUX</topic><topic>MAGNETIC MOMENTS</topic><topic>ORBITS</topic><topic>PERIODICITY</topic><topic>PLASMA</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Jagannath, Aukosh</creatorcontrib><creatorcontrib>Weitzner, Harold</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Physics of plasmas</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Jagannath, Aukosh</au><au>Weitzner, Harold</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Charged particle motion in electromagnetic fields varying moderately rapidly in space</atitle><jtitle>Physics of plasmas</jtitle><date>2011-10-01</date><risdate>2011</risdate><volume>18</volume><issue>10</issue><spage>104510</spage><epage>104510-4</epage><pages>104510-104510-4</pages><issn>1070-664X</issn><eissn>1089-7674</eissn><coden>PHPAEN</coden><abstract>Electromagnetic fields are considered which vary on the space scale of the geometric mean of the Larmor radius and the much larger scale length of variation of the magnetic field lines. It is first shown that the magnetic moment is an adiabatic invariant, even though the usual arguments for its existence fail. The motion of the guiding center is then examined. For perpendicular drifts in magnitude comparable with the particle speed, the subsequent motion is dominated by electrostatic effects. The motion of particles along the field lines occurs on a much slower time scale than the perpendicular drift time scale. When the guiding center motion is approximately periodic in time, a second adiabatic invariant exists, the magnetic flux enclosed by the almost periodic orbit. When the perpendicular drift is small compared with the particle speed, the parallel motion and the perpendicular drift occur on the same, slow timescale.</abstract><cop>United States</cop><pub>American Institute of Physics</pub><doi>10.1063/1.3652850</doi></addata></record>
fulltext fulltext
identifier ISSN: 1070-664X
ispartof Physics of plasmas, 2011-10, Vol.18 (10), p.104510-104510-4
issn 1070-664X
1089-7674
language eng
recordid cdi_osti_scitechconnect_22047022
source AIP Journals Complete; AIP Digital Archive; Alma/SFX Local Collection
subjects 70 PLASMA PHYSICS AND FUSION TECHNOLOGY
CHARGED PARTICLES
ELECTROMAGNETIC FIELDS
ELECTROMAGNETIC RADIATION
ELECTROSTATICS
LARMOR RADIUS
LENGTH
MAGNETIC FIELDS
MAGNETIC FLUX
MAGNETIC MOMENTS
ORBITS
PERIODICITY
PLASMA
title Charged particle motion in electromagnetic fields varying moderately rapidly in space
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-10T18%3A26%3A35IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-scitation_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Charged%20particle%20motion%20in%20electromagnetic%20fields%20varying%20moderately%20rapidly%20in%20space&rft.jtitle=Physics%20of%20plasmas&rft.au=Jagannath,%20Aukosh&rft.date=2011-10-01&rft.volume=18&rft.issue=10&rft.spage=104510&rft.epage=104510-4&rft.pages=104510-104510-4&rft.issn=1070-664X&rft.eissn=1089-7674&rft.coden=PHPAEN&rft_id=info:doi/10.1063/1.3652850&rft_dat=%3Cscitation_osti_%3Epop%3C/scitation_osti_%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