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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3SB3T28
Repositorysid.inpe.br/mtc-m21c/2018/12.03.15.19
Last Update2019:01.09.17.45.11 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2018/12.03.15.19.28
Metadata Last Update2019:01.14.17.06.39 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeySilveiraSiLeGoKoSo:2018:FlTrEv
TitleFlux transfer events observed in the dayside magnetopause by MMS mission
Year2018
Access Date2024, May 19
Secondary TypePRE CI
Number of Files1
Size116 KiB
2. Context
Author1 Silveira, Marcos D.
2 Sibeck, David G.
3 Lee, Sun-Hee
4 Gonzalez Alarcon, Walter Demétrio
5 Koga, Daiki
6 Souza, Vitor Moura Cardoso e Silva
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJC4
Group1
2
3
4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
5 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
6 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Catholic University of America
2 NASA Goddard Space Flight Center
3 NASA Goddard Space Flight Center
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4 walter.gonzalez@inpe.br
5 daiki.koga@inpe.br
6 vitor.souza@inpe.br
Conference NameAGU Fall Meeting
Conference LocationWashington, D. C.
Date10-14 dec.
History (UTC)2018-12-03 15:19:28 :: simone -> administrator ::
2019-01-14 17:06:39 :: administrator -> simone :: 2018
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractFlux transfer events (FTE) have been interpreted to be results from transient magnetic reconnection and can be observed in the vicinity of the Earths magnetopause, as well in other planets. FTE acts as a flux tube connecting the magnetosheath to the magnetosphere allowing the transference of particles, energy and momentum in both sides magnetopause. Their main signatures in satellite data are bipolar variation in the magnetic field component normal to the magnetopause, centered in an enhanced magnetic field strength. Other signatures such as pressure imbalance, bulk flow jets, and particle anisotropy distribution can be observed inside the those structures. We surveyed FTEs observed by MMS on the vicinity of the magnetopause (from x = 0 to 13Re and y = -12 to 12Re). Taking advantage of the MMS tetrahedron configuration we will employed timing analysis to determine the FTEs direction of motion and scale lengths. We will present information about occurrence related with IMF clock angle and other parameters, amplitude of the perturbations induced by the FTEs in the environment magnetic field and plasma; characteristic time and structure scale size. Using data from ACE, Wind and Artemis we can evaluate which is the best solar wind monitor for each FTE observed and then employ the appropriated lag time corresponding to FTE location and magnetic field orientation. The objective is to investigate the mechanisms of generation of FTEs comparing characteristics of the events observed on the dayside region and on the magnetopause flanks determining the motion and speed of FTEs.
AreaCEA
ArrangementFlux transfer events...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
agreement.html 03/12/2018 13:19 1.0 KiB 
4. Conditions of access and use
data URLhttp://mtc-m21c.sid.inpe.br/ibi/8JMKD3MGP3W34R/3SB3T28
zipped data URLhttp://mtc-m21c.sid.inpe.br/zip/8JMKD3MGP3W34R/3SB3T28
Languageen
Target Filesilveira_flux.pdf
User Groupself-uploading-INPE-MCTI-GOV-BR
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.15.01.50 4
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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