Signatures of nonlinear charged particle dynamics in Geotail comprehensive plasma instrument observations
In this paper we present simulation results and observational data from the Geotail comprehensive plasma instrument of an ion distribution function signature which arises due to nonlinear particle dynamics in the quiet time magnetotail. The signature manifests itself as peaks and valleys in the ion...
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Veröffentlicht in: | Journal of Geophysical Research 1999-02, Vol.104 (A2), p.2479-2485 |
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creator | Holland, D. L. Paterson, W. R. Frank, L. A. Kokubun, S. Yamamoto, Y. |
description | In this paper we present simulation results and observational data from the Geotail comprehensive plasma instrument of an ion distribution function signature which arises due to nonlinear particle dynamics in the quiet time magnetotail. The signature manifests itself as peaks and valleys in the ion distribution function whose separation scales as the fourth root of the particle energy. The Geotail observations represent the first independent corroboration of this signature since it was seen in ISEE 1 data by Chen et al. [1990]. The simulations demonstrate that the signature is present in the pitch‐angle‐resolved distribution even in the case of perfectly symmetric particle sources in the northern and southern hemispheres. When combined with magnetometer data, we show how the peaks and valleys may be used to determine the current sheet thickness using a single satellite. The current sheet thickness determined in this fashion is less than but consistent with other measurements of the current sheet. |
doi_str_mv | 10.1029/1998JA900040 |
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L. ; Paterson, W. R. ; Frank, L. A. ; Kokubun, S. ; Yamamoto, Y.</creator><creatorcontrib>Holland, D. L. ; Paterson, W. R. ; Frank, L. A. ; Kokubun, S. ; Yamamoto, Y.</creatorcontrib><description>In this paper we present simulation results and observational data from the Geotail comprehensive plasma instrument of an ion distribution function signature which arises due to nonlinear particle dynamics in the quiet time magnetotail. The signature manifests itself as peaks and valleys in the ion distribution function whose separation scales as the fourth root of the particle energy. The Geotail observations represent the first independent corroboration of this signature since it was seen in ISEE 1 data by Chen et al. [1990]. The simulations demonstrate that the signature is present in the pitch‐angle‐resolved distribution even in the case of perfectly symmetric particle sources in the northern and southern hemispheres. When combined with magnetometer data, we show how the peaks and valleys may be used to determine the current sheet thickness using a single satellite. The current sheet thickness determined in this fashion is less than but consistent with other measurements of the current sheet.</description><identifier>ISSN: 0148-0227</identifier><identifier>EISSN: 2156-2202</identifier><identifier>DOI: 10.1029/1998JA900040</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Earth, ocean, space ; Exact sciences and technology ; External geophysics ; Physics of the magnetosphere ; Trapped particles</subject><ispartof>Journal of Geophysical Research, 1999-02, Vol.104 (A2), p.2479-2485</ispartof><rights>Copyright 1999 by the American Geophysical Union.</rights><rights>1999 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4441-368d2be3d74204de05c56aa6af14f65885074043c521163f924a85ddabb426d33</citedby><cites>FETCH-LOGICAL-c4441-368d2be3d74204de05c56aa6af14f65885074043c521163f924a85ddabb426d33</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%2F1998JA900040$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F1998JA900040$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,1427,11493,27901,27902,45550,45551,46384,46443,46808,46867</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=1685495$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Holland, D. L.</creatorcontrib><creatorcontrib>Paterson, W. R.</creatorcontrib><creatorcontrib>Frank, L. A.</creatorcontrib><creatorcontrib>Kokubun, S.</creatorcontrib><creatorcontrib>Yamamoto, Y.</creatorcontrib><title>Signatures of nonlinear charged particle dynamics in Geotail comprehensive plasma instrument observations</title><title>Journal of Geophysical Research</title><addtitle>J. Geophys. Res</addtitle><description>In this paper we present simulation results and observational data from the Geotail comprehensive plasma instrument of an ion distribution function signature which arises due to nonlinear particle dynamics in the quiet time magnetotail. The signature manifests itself as peaks and valleys in the ion distribution function whose separation scales as the fourth root of the particle energy. The Geotail observations represent the first independent corroboration of this signature since it was seen in ISEE 1 data by Chen et al. [1990]. The simulations demonstrate that the signature is present in the pitch‐angle‐resolved distribution even in the case of perfectly symmetric particle sources in the northern and southern hemispheres. When combined with magnetometer data, we show how the peaks and valleys may be used to determine the current sheet thickness using a single satellite. The current sheet thickness determined in this fashion is less than but consistent with other measurements of the current sheet.</description><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Physics of the magnetosphere</subject><subject>Trapped particles</subject><issn>0148-0227</issn><issn>2156-2202</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1999</creationdate><recordtype>article</recordtype><recordid>eNqFkE1vEzEURS0EElHbHT_AC8SKof4ezzKqIKWqigSFSt1YL543rcFjD_akkH9PolTAClZvcc-5T7qEvODsDWeiO-VdZy-WHWNMsSdkIbg2jRBMPCULxpVtmBDtc3JS61e2Z7RRjC9I-BTuEsybgpXmgaacYkgIhfp7KHfY0wnKHHxE2m8TjMFXGhJdYZ4hROrzOBW8x1TDA9IpQh1hl9e5bEZMM83riuUB5pBTPSbPBogVTx7vEfn87u312Xlz-WH1_mx52XilFG-ksb1Yo-xbJZjqkWmvDYCBgavBaGs1axVT0mvBuZFDJxRY3fewXitheimPyKtD71Ty9w3W2Y2heowREuZNdaLlvLVG_xfkllkrdLcDXx9AX3KtBQc3lTBC2TrO3H579_f2O_zlYy9UD3EokHyofxxjter27-UB-xEibv9Z6S5WH5dcSc13VnOwQp3x528LyjdnWtlqd3O1crfttT3_cnXjbuUvPo2iPg</recordid><startdate>19990201</startdate><enddate>19990201</enddate><creator>Holland, D. 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A.</creatorcontrib><creatorcontrib>Kokubun, S.</creatorcontrib><creatorcontrib>Yamamoto, Y.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of Geophysical Research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Holland, D. L.</au><au>Paterson, W. R.</au><au>Frank, L. A.</au><au>Kokubun, S.</au><au>Yamamoto, Y.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Signatures of nonlinear charged particle dynamics in Geotail comprehensive plasma instrument observations</atitle><jtitle>Journal of Geophysical Research</jtitle><addtitle>J. Geophys. Res</addtitle><date>1999-02-01</date><risdate>1999</risdate><volume>104</volume><issue>A2</issue><spage>2479</spage><epage>2485</epage><pages>2479-2485</pages><issn>0148-0227</issn><eissn>2156-2202</eissn><abstract>In this paper we present simulation results and observational data from the Geotail comprehensive plasma instrument of an ion distribution function signature which arises due to nonlinear particle dynamics in the quiet time magnetotail. The signature manifests itself as peaks and valleys in the ion distribution function whose separation scales as the fourth root of the particle energy. The Geotail observations represent the first independent corroboration of this signature since it was seen in ISEE 1 data by Chen et al. [1990]. The simulations demonstrate that the signature is present in the pitch‐angle‐resolved distribution even in the case of perfectly symmetric particle sources in the northern and southern hemispheres. When combined with magnetometer data, we show how the peaks and valleys may be used to determine the current sheet thickness using a single satellite. The current sheet thickness determined in this fashion is less than but consistent with other measurements of the current sheet.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/1998JA900040</doi><tpages>7</tpages><oa>free_for_read</oa></addata></record> |
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source | Wiley-Blackwell AGU Digital Library; Wiley Online Library Journals Frontfile Complete; Wiley Online Library Free Content; Alma/SFX Local Collection |
subjects | Earth, ocean, space Exact sciences and technology External geophysics Physics of the magnetosphere Trapped particles |
title | Signatures of nonlinear charged particle dynamics in Geotail comprehensive plasma instrument observations |
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