Parallel acceleration and transport of ions from polar ionosphere to plasma sheet
The effect of the convection electric field in accelerating ions that escape from the polar ionosphere is investigated. It is shown that at high altitudes the velocity component of the ions along the magnetic field may be increased by more than an order of magnitude. The highest velocities are acqui...
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Veröffentlicht in: | Geophysical research letters 1986-09, Vol.13 (9), p.893-896 |
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description | The effect of the convection electric field in accelerating ions that escape from the polar ionosphere is investigated. It is shown that at high altitudes the velocity component of the ions along the magnetic field may be increased by more than an order of magnitude. The highest velocities are acquired by ions that escape from the region of the ionosphere that is connected along magnetic field lines to the dayside cusps. During disturbed times, ions from that region intercept the center plane of the magnetotail in one to two hours at radial distances exceeding about 6 earth radii. Investigation of the resulting O(+) properties in the center plane, viz., their locations, number densities, and energies, indicates that the polar ionosphere near the cusps is the principal source of the O(+) observed in the plasma sheet. Moreover, a study of the ion motion at quiet and disturbed times indicates that the increase of O(+) in the plasma sheet with increasing AE values (Lennartsson and Shelley, 1986) is due mainly to an increase in the source of O(+) rather than alteration of its transport path. |
doi_str_mv | 10.1029/GL013i009p00893 |
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B.</creator><creatorcontrib>Cladis, J. B.</creatorcontrib><description>The effect of the convection electric field in accelerating ions that escape from the polar ionosphere is investigated. It is shown that at high altitudes the velocity component of the ions along the magnetic field may be increased by more than an order of magnitude. The highest velocities are acquired by ions that escape from the region of the ionosphere that is connected along magnetic field lines to the dayside cusps. During disturbed times, ions from that region intercept the center plane of the magnetotail in one to two hours at radial distances exceeding about 6 earth radii. Investigation of the resulting O(+) properties in the center plane, viz., their locations, number densities, and energies, indicates that the polar ionosphere near the cusps is the principal source of the O(+) observed in the plasma sheet. Moreover, a study of the ion motion at quiet and disturbed times indicates that the increase of O(+) in the plasma sheet with increasing AE values (Lennartsson and Shelley, 1986) is due mainly to an increase in the source of O(+) rather than alteration of its transport path.</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/GL013i009p00893</identifier><identifier>CODEN: GPRLAJ</identifier><language>eng</language><publisher>Legacy CDMS: Blackwell Publishing Ltd</publisher><subject>Convection ; Cusps ; Density ; Earth, ocean, space ; Exact sciences and technology ; External geophysics ; Geophysics ; Interaction between ionosphere and magnetosphere ; Ionosphere ; Magnetic fields ; Magnetic properties ; Physics of the ionosphere ; Planes ; Transport</subject><ispartof>Geophysical research letters, 1986-09, Vol.13 (9), p.893-896</ispartof><rights>Copyright 1986 by the American Geophysical Union.</rights><rights>1987 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c5500-2a2d297bcafbeee07fd55796015c9b628b29f2e945a94bd7a66c3096e04d0c713</citedby><cites>FETCH-LOGICAL-c5500-2a2d297bcafbeee07fd55796015c9b628b29f2e945a94bd7a66c3096e04d0c713</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2FGL013i009p00893$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2FGL013i009p00893$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,780,784,1417,27924,27925,45574,45575</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=7856945$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Cladis, J. B.</creatorcontrib><title>Parallel acceleration and transport of ions from polar ionosphere to plasma sheet</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>The effect of the convection electric field in accelerating ions that escape from the polar ionosphere is investigated. It is shown that at high altitudes the velocity component of the ions along the magnetic field may be increased by more than an order of magnitude. The highest velocities are acquired by ions that escape from the region of the ionosphere that is connected along magnetic field lines to the dayside cusps. During disturbed times, ions from that region intercept the center plane of the magnetotail in one to two hours at radial distances exceeding about 6 earth radii. Investigation of the resulting O(+) properties in the center plane, viz., their locations, number densities, and energies, indicates that the polar ionosphere near the cusps is the principal source of the O(+) observed in the plasma sheet. Moreover, a study of the ion motion at quiet and disturbed times indicates that the increase of O(+) in the plasma sheet with increasing AE values (Lennartsson and Shelley, 1986) is due mainly to an increase in the source of O(+) rather than alteration of its transport path.</description><subject>Convection</subject><subject>Cusps</subject><subject>Density</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Geophysics</subject><subject>Interaction between ionosphere and magnetosphere</subject><subject>Ionosphere</subject><subject>Magnetic fields</subject><subject>Magnetic properties</subject><subject>Physics of the ionosphere</subject><subject>Planes</subject><subject>Transport</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1986</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNqFkc1v1DAQxSMEEkvLmQsHHxDiEjq24zg-0gJppRWlfJSjNXEmasAbp3Yq6H-PV6l64EBPtmd-72nmuShecHjLQZijdgtcjgBmBmiMfFRsuKmqsgHQj4tNrue70PXT4llKPwFAguSb4uIzRvSePEPnyFPEZQwTw6lnS8QpzSEuLAwsFxMbYtixOXiM-3dI8xVFYktgs8e0Q5auiJbD4smAPtHzu_Og-P7xw7eT03J73p6dvNuWTimAUqDohdGdw6EjItBDr5Q2NXDlTFeLphNmEGQqhabqeo117SSYmqDqwWkuD4rXq-8cw_UNpcXuxpRX8DhRuElWVAKUaVQG3_wX5EoYI4XSTUaPVtTFkFKkwc5x3GG8tRzsPmX7T8pZ8erOHJNDP-TM3JjuZbpRdV4hY9WK_R493T7katsvWykayLKXq2zChHZaYp7WNHr_eeu45doe00J_7l0x_rK1llrZH59ae_z1_enlRXtpj-Vf4Fyj6A</recordid><startdate>198609</startdate><enddate>198609</enddate><creator>Cladis, J. B.</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><scope>BSCLL</scope><scope>CYE</scope><scope>CYI</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>FR3</scope><scope>H8D</scope><scope>KR7</scope><scope>L7M</scope></search><sort><creationdate>198609</creationdate><title>Parallel acceleration and transport of ions from polar ionosphere to plasma sheet</title><author>Cladis, J. B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c5500-2a2d297bcafbeee07fd55796015c9b628b29f2e945a94bd7a66c3096e04d0c713</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1986</creationdate><topic>Convection</topic><topic>Cusps</topic><topic>Density</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>External geophysics</topic><topic>Geophysics</topic><topic>Interaction between ionosphere and magnetosphere</topic><topic>Ionosphere</topic><topic>Magnetic fields</topic><topic>Magnetic properties</topic><topic>Physics of the ionosphere</topic><topic>Planes</topic><topic>Transport</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Cladis, J. B.</creatorcontrib><collection>Istex</collection><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Civil Engineering Abstracts</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Cladis, J. B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Parallel acceleration and transport of ions from polar ionosphere to plasma sheet</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>1986-09</date><risdate>1986</risdate><volume>13</volume><issue>9</issue><spage>893</spage><epage>896</epage><pages>893-896</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>The effect of the convection electric field in accelerating ions that escape from the polar ionosphere is investigated. It is shown that at high altitudes the velocity component of the ions along the magnetic field may be increased by more than an order of magnitude. The highest velocities are acquired by ions that escape from the region of the ionosphere that is connected along magnetic field lines to the dayside cusps. During disturbed times, ions from that region intercept the center plane of the magnetotail in one to two hours at radial distances exceeding about 6 earth radii. Investigation of the resulting O(+) properties in the center plane, viz., their locations, number densities, and energies, indicates that the polar ionosphere near the cusps is the principal source of the O(+) observed in the plasma sheet. Moreover, a study of the ion motion at quiet and disturbed times indicates that the increase of O(+) in the plasma sheet with increasing AE values (Lennartsson and Shelley, 1986) is due mainly to an increase in the source of O(+) rather than alteration of its transport path.</abstract><cop>Legacy CDMS</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/GL013i009p00893</doi><tpages>4</tpages></addata></record> |
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issn | 0094-8276 1944-8007 |
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source | Access via Wiley Online Library; NASA Technical Reports Server |
subjects | Convection Cusps Density Earth, ocean, space Exact sciences and technology External geophysics Geophysics Interaction between ionosphere and magnetosphere Ionosphere Magnetic fields Magnetic properties Physics of the ionosphere Planes Transport |
title | Parallel acceleration and transport of ions from polar ionosphere to plasma sheet |
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