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...
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Veröffentlicht in: | Physics of plasmas 2011-10, Vol.18 (10), p.104510-104510-4 |
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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 |
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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> |
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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 |
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