Loading…

Obtain martian magnetic pileup boundary by spectrum of low energy electrons

The electron spectrometer of Mars Express (MEX) provides the flux of low energy electrons (〈20 keV) near Mars. 96 pieces of continuously measured data are analyzed, and the crossings of the magnetic pileup boundary (MPB) can be determined by fitting the energy spectrum of the low energy electrons. T...

Full description

Saved in:
Bibliographic Details
Published in:Science China. Technological sciences 2013-09, Vol.56 (9), p.2349-2354
Main Authors: Li, ChenFang, Zou, Hong, Chen, HongFei, Shi, WeiHong, Yu, XiangQian
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c314t-a820b5d978462bb41c55468673df9b8dc2876b24498e3e055caea4c84294b6623
cites cdi_FETCH-LOGICAL-c314t-a820b5d978462bb41c55468673df9b8dc2876b24498e3e055caea4c84294b6623
container_end_page 2354
container_issue 9
container_start_page 2349
container_title Science China. Technological sciences
container_volume 56
creator Li, ChenFang
Zou, Hong
Chen, HongFei
Shi, WeiHong
Yu, XiangQian
description The electron spectrometer of Mars Express (MEX) provides the flux of low energy electrons (〈20 keV) near Mars. 96 pieces of continuously measured data are analyzed, and the crossings of the magnetic pileup boundary (MPB) can be determined by fitting the energy spectrum of the low energy electrons. The shape and position of the MPB can be gained from these crossings, and they are in good agreement with the results obtained by the Mars Global Surveyor (MGS) and Phobos-2. In addition, we classify these crossings based on the crustal magnetic field nearby. It turns out that the position of MPB near the strong (〉50 nT) crustal magnetic field is higher than the position of the MPB near the weak (〈10 nT) crustal magnetic field. This re- sult reflects the effect of the crustal magnetic field on the interaction between the Martian atmosphere and solar wind.
doi_str_mv 10.1007/s11431-013-5300-8
format article
fullrecord <record><control><sourceid>crossref_sprin</sourceid><recordid>TN_cdi_crossref_primary_10_1007_s11431_013_5300_8</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cqvip_id>46901303</cqvip_id><sourcerecordid>10_1007_s11431_013_5300_8</sourcerecordid><originalsourceid>FETCH-LOGICAL-c314t-a820b5d978462bb41c55468673df9b8dc2876b24498e3e055caea4c84294b6623</originalsourceid><addsrcrecordid>eNp9kMtOwzAQRS0EElXpB7AzH2DwK46zRBUvUakbWFu244RUqR3sRCh_j6NWLJnNjEZz584cAG4JvicYlw-JEM4IwoShgmGM5AVYESkqRCqML3MtSo5KRsk12KR0wDmYrDDhK_C-N6PuPDzqOHZ6ya13Y2fh0PVuGqAJk691nKGZYRqcHeN0hKGBffiBzrvYztD1Szv4dAOuGt0ntznnNfh8fvrYvqLd_uVt-7hDlhE-Ii0pNkVdlZILagwntii4kKJkdVMZWVsqS2Eo55V0zOGisNppbiWnFTdCULYG5LTXxpBSdI0aYpcfmBXBagGiTkBUBqIWIEpmDT1pUp71rYvqEKbo85n_iu7ORl_Bt99Z9-fERebHMGO__GZuCQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Obtain martian magnetic pileup boundary by spectrum of low energy electrons</title><source>Springer Nature</source><creator>Li, ChenFang ; Zou, Hong ; Chen, HongFei ; Shi, WeiHong ; Yu, XiangQian</creator><creatorcontrib>Li, ChenFang ; Zou, Hong ; Chen, HongFei ; Shi, WeiHong ; Yu, XiangQian</creatorcontrib><description>The electron spectrometer of Mars Express (MEX) provides the flux of low energy electrons (〈20 keV) near Mars. 96 pieces of continuously measured data are analyzed, and the crossings of the magnetic pileup boundary (MPB) can be determined by fitting the energy spectrum of the low energy electrons. The shape and position of the MPB can be gained from these crossings, and they are in good agreement with the results obtained by the Mars Global Surveyor (MGS) and Phobos-2. In addition, we classify these crossings based on the crustal magnetic field nearby. It turns out that the position of MPB near the strong (〉50 nT) crustal magnetic field is higher than the position of the MPB near the weak (〈10 nT) crustal magnetic field. This re- sult reflects the effect of the crustal magnetic field on the interaction between the Martian atmosphere and solar wind.</description><identifier>ISSN: 1674-7321</identifier><identifier>EISSN: 1869-1900</identifier><identifier>DOI: 10.1007/s11431-013-5300-8</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Engineering ; 低能电子 ; 堆积 ; 火星大气 ; 电子能谱仪 ; 相互作用 ; 磁场 ; 边界 ; 频谱</subject><ispartof>Science China. Technological sciences, 2013-09, Vol.56 (9), p.2349-2354</ispartof><rights>Science China Press and Springer-Verlag Berlin Heidelberg 2013</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c314t-a820b5d978462bb41c55468673df9b8dc2876b24498e3e055caea4c84294b6623</citedby><cites>FETCH-LOGICAL-c314t-a820b5d978462bb41c55468673df9b8dc2876b24498e3e055caea4c84294b6623</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Uhttp://image.cqvip.com/vip1000/qk/60110X/60110X.jpg</thumbnail><link.rule.ids>314,777,781,27905,27906</link.rule.ids></links><search><creatorcontrib>Li, ChenFang</creatorcontrib><creatorcontrib>Zou, Hong</creatorcontrib><creatorcontrib>Chen, HongFei</creatorcontrib><creatorcontrib>Shi, WeiHong</creatorcontrib><creatorcontrib>Yu, XiangQian</creatorcontrib><title>Obtain martian magnetic pileup boundary by spectrum of low energy electrons</title><title>Science China. Technological sciences</title><addtitle>Sci. China Technol. Sci</addtitle><addtitle>SCIENCE CHINA Technological Sciences</addtitle><description>The electron spectrometer of Mars Express (MEX) provides the flux of low energy electrons (〈20 keV) near Mars. 96 pieces of continuously measured data are analyzed, and the crossings of the magnetic pileup boundary (MPB) can be determined by fitting the energy spectrum of the low energy electrons. The shape and position of the MPB can be gained from these crossings, and they are in good agreement with the results obtained by the Mars Global Surveyor (MGS) and Phobos-2. In addition, we classify these crossings based on the crustal magnetic field nearby. It turns out that the position of MPB near the strong (〉50 nT) crustal magnetic field is higher than the position of the MPB near the weak (〈10 nT) crustal magnetic field. This re- sult reflects the effect of the crustal magnetic field on the interaction between the Martian atmosphere and solar wind.</description><subject>Engineering</subject><subject>低能电子</subject><subject>堆积</subject><subject>火星大气</subject><subject>电子能谱仪</subject><subject>相互作用</subject><subject>磁场</subject><subject>边界</subject><subject>频谱</subject><issn>1674-7321</issn><issn>1869-1900</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNp9kMtOwzAQRS0EElXpB7AzH2DwK46zRBUvUakbWFu244RUqR3sRCh_j6NWLJnNjEZz584cAG4JvicYlw-JEM4IwoShgmGM5AVYESkqRCqML3MtSo5KRsk12KR0wDmYrDDhK_C-N6PuPDzqOHZ6ya13Y2fh0PVuGqAJk691nKGZYRqcHeN0hKGBffiBzrvYztD1Szv4dAOuGt0ntznnNfh8fvrYvqLd_uVt-7hDlhE-Ii0pNkVdlZILagwntii4kKJkdVMZWVsqS2Eo55V0zOGisNppbiWnFTdCULYG5LTXxpBSdI0aYpcfmBXBagGiTkBUBqIWIEpmDT1pUp71rYvqEKbo85n_iu7ORl_Bt99Z9-fERebHMGO__GZuCQ</recordid><startdate>20130901</startdate><enddate>20130901</enddate><creator>Li, ChenFang</creator><creator>Zou, Hong</creator><creator>Chen, HongFei</creator><creator>Shi, WeiHong</creator><creator>Yu, XiangQian</creator><general>Springer Berlin Heidelberg</general><scope>2RA</scope><scope>92L</scope><scope>CQIGP</scope><scope>W92</scope><scope>~WA</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20130901</creationdate><title>Obtain martian magnetic pileup boundary by spectrum of low energy electrons</title><author>Li, ChenFang ; Zou, Hong ; Chen, HongFei ; Shi, WeiHong ; Yu, XiangQian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c314t-a820b5d978462bb41c55468673df9b8dc2876b24498e3e055caea4c84294b6623</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Engineering</topic><topic>低能电子</topic><topic>堆积</topic><topic>火星大气</topic><topic>电子能谱仪</topic><topic>相互作用</topic><topic>磁场</topic><topic>边界</topic><topic>频谱</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Li, ChenFang</creatorcontrib><creatorcontrib>Zou, Hong</creatorcontrib><creatorcontrib>Chen, HongFei</creatorcontrib><creatorcontrib>Shi, WeiHong</creatorcontrib><creatorcontrib>Yu, XiangQian</creatorcontrib><collection>维普_期刊</collection><collection>中文科技期刊数据库-CALIS站点</collection><collection>中文科技期刊数据库-7.0平台</collection><collection>中文科技期刊数据库-工程技术</collection><collection>中文科技期刊数据库- 镜像站点</collection><collection>CrossRef</collection><jtitle>Science China. Technological sciences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Li, ChenFang</au><au>Zou, Hong</au><au>Chen, HongFei</au><au>Shi, WeiHong</au><au>Yu, XiangQian</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Obtain martian magnetic pileup boundary by spectrum of low energy electrons</atitle><jtitle>Science China. Technological sciences</jtitle><stitle>Sci. China Technol. Sci</stitle><addtitle>SCIENCE CHINA Technological Sciences</addtitle><date>2013-09-01</date><risdate>2013</risdate><volume>56</volume><issue>9</issue><spage>2349</spage><epage>2354</epage><pages>2349-2354</pages><issn>1674-7321</issn><eissn>1869-1900</eissn><abstract>The electron spectrometer of Mars Express (MEX) provides the flux of low energy electrons (〈20 keV) near Mars. 96 pieces of continuously measured data are analyzed, and the crossings of the magnetic pileup boundary (MPB) can be determined by fitting the energy spectrum of the low energy electrons. The shape and position of the MPB can be gained from these crossings, and they are in good agreement with the results obtained by the Mars Global Surveyor (MGS) and Phobos-2. In addition, we classify these crossings based on the crustal magnetic field nearby. It turns out that the position of MPB near the strong (〉50 nT) crustal magnetic field is higher than the position of the MPB near the weak (〈10 nT) crustal magnetic field. This re- sult reflects the effect of the crustal magnetic field on the interaction between the Martian atmosphere and solar wind.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/s11431-013-5300-8</doi><tpages>6</tpages></addata></record>
fulltext fulltext
identifier ISSN: 1674-7321
ispartof Science China. Technological sciences, 2013-09, Vol.56 (9), p.2349-2354
issn 1674-7321
1869-1900
language eng
recordid cdi_crossref_primary_10_1007_s11431_013_5300_8
source Springer Nature
subjects Engineering
低能电子
堆积
火星大气
电子能谱仪
相互作用
磁场
边界
频谱
title Obtain martian magnetic pileup boundary by spectrum of low energy electrons
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-18T18%3A24%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_sprin&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Obtain%20martian%20magnetic%20pileup%20boundary%20by%20spectrum%20of%20low%20energy%20electrons&rft.jtitle=Science%20China.%20Technological%20sciences&rft.au=Li,%20ChenFang&rft.date=2013-09-01&rft.volume=56&rft.issue=9&rft.spage=2349&rft.epage=2354&rft.pages=2349-2354&rft.issn=1674-7321&rft.eissn=1869-1900&rft_id=info:doi/10.1007/s11431-013-5300-8&rft_dat=%3Ccrossref_sprin%3E10_1007_s11431_013_5300_8%3C/crossref_sprin%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c314t-a820b5d978462bb41c55468673df9b8dc2876b24498e3e055caea4c84294b6623%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rft_cqvip_id=46901303&rfr_iscdi=true