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...
Saved in:
Published in: | Science China. Technological sciences 2013-09, Vol.56 (9), p.2349-2354 |
---|---|
Main Authors: | , , , , |
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 |