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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3NTG6AE
Repositorysid.inpe.br/mtc-m21b/2017/05.19.12.56
Last Update2017:05.19.12.56.29 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21b/2017/05.19.12.56.29
Metadata Last Update2018:06.04.02.27.28 (UTC) administrator
DOI10.1002/2017GL072817
ISSN0094-8276
Citation KeyLopezGonz:2017:MaBaSo
TitleMagnetospheric balance of solar wind dynamic pressure
Year2017
MonthApr.
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size773 KiB
2. Context
Author1 Lopez, Ramon E.
2 Gonzalez Alarcon, Walter Demétrio
Resume Identifier1
2 8JMKD3MGP5W/3C9JJC4
Group1
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 University of Texas at Arlington
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1 relopez@uta.edu
2 walter.gonzalez@inpe.br
JournalGeophysical Research Letters
Volume44
Number7
Pages2991-2999
Secondary MarkA1_INTERDISCIPLINAR A1_GEOGRAFIA A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ENGENHARIAS_I A1_CIÊNCIAS_AMBIENTAIS A1_CIÊNCIAS_AGRÁRIAS_I A1_BIODIVERSIDADE A2_QUÍMICA A2_ENGENHARIAS_IV A2_ENGENHARIAS_II A2_CIÊNCIAS_BIOLÓGICAS_I B1_ASTRONOMIA_/_FÍSICA B2_ENSINO
History (UTC)2017-05-19 12:56:29 :: simone -> administrator ::
2017-05-19 12:56:30 :: administrator -> simone :: 2017
2017-05-19 12:56:51 :: simone -> administrator :: 2017
2018-06-04 02:27:28 :: administrator -> simone :: 2017
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsmagnetopause
bow shock
currents
AbstractThe magnetopause is the boundary established by pressure balance between the solar wind flow in the magnetosheath and the magnetosphere. Generally, this pressure balance is represented to be between the solar wind, the dynamic pressure, and the magnetic pressure of Earth's dipole field. The plasma actually in contact with the magnetosphere is the slowed, compressed, and heated solar wind downstream of the shock. The force exerted on the magnetosheath plasma is the JxB force produced by the Chapman-Ferraro current that flows on the magnetopause. Under typical solar wind conditions of relatively high magnetosonic Mach number flow (>6), this simple picture is a reasonable description of the situation. However, under conditions of low solar wind magnetosonic Mach number flow (similar to 2) the force on the solar wind plasma is not exerted at the magnetopause and must be exerted at the bow shock by currents that connect to the Region 1 currents. In this paper we present observations from two magnetopause crossings observed by the Time History of Events and Macroscale Interactions during Substorms spacecraft to compare and contrast the force balance with the solar wind for two situations with very different solar wind magnetosonic Mach numbers. Plain Language Summary When the solar wind hits Earth's magnetic field, the magnetic field pushes back on the solar wind. Typically, this force is exerted at the boundary between Earth's magnetic field and the solar wind. However, when the supersonic solar wind has a low Mach number (about 2, as opposed to the typical value of >6), the place where the force is exerted on the solar wind is at the bow shock wave in front of Earth. This force is produced by an electric current that flows on the bow shock and which connects to currents that flow directly into Earth's ionosphere in the polar regions. This paper presents spacecraft observations documenting this unusual situation.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Magnetospheric balance of...
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4. Conditions of access and use
data URLhttp://mtc-m21b.sid.inpe.br/ibi/8JMKD3MGP3W34P/3NTG6AE
zipped data URLhttp://mtc-m21b.sid.inpe.br/zip/8JMKD3MGP3W34P/3NTG6AE
Languageen
Target Filelopez_magnetospheric.pdf
User Groupsimone
Reader Groupadministrator
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Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.22.11 3
sid.inpe.br/mtc-m21/2012/07.13.15.01.50 3
DisseminationWEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS.
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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