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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/marciana/2004/07.08.14.15   (restricted access)
Last Update2004:12.10.02.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/07.08.14.15.45
Metadata Last Update2018:06.05.01.20.56 (UTC) administrator
Secondary KeyINPE-10971-PRE/6427
ISSN0273-1177
Citation KeyPugachevaGonJaySchGus:2004:RiCuIo
TitleRing Current Ion Finite Motion in Disturbed Magnetosphere With Nonequipotential Magnetic Field Lines
Year2004
Access Date2024, May 18
Secondary TypePRE PI
Number of Files1
Size383 KiB
2. Context
Author1 Pugacheva, G.
2 Gonzalez, W.
3 Jayanthi, U.
4 Schuch, Nelson Jorge
5 Gusev, A.
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JHUD
Group1 RSU-INPE-MCT-BR
2 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
JournalAdvances in Space Research
Volume33
Number5
Pages723-728
History (UTC)2006-03-17 18:54:42 :: sergio -> administrator ::
2006-09-28 22:27:46 :: administrator -> sergio ::
2008-01-07 12:53:22 :: sergio -> administrator ::
2012-07-17 12:42:49 :: administrator -> marciana ::
2012-10-03 16:03:54 :: marciana -> administrator :: 2004
2018-06-05 01:20:56 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractSimulations of the transport of ring current particles in the magnetosphere during disturbances are attempted using a three-dimensional single particle code. The simulations considered, for the magnetospheric field both the dipole and Tsyganenko models. The convection electric field is described in equatorial plane by the model of Volland-Stern with dependence on geomagnetic activity and is assumed to be the same out of the equatorial plane. It implies nonequipotentiality of the geomagnetic field lines that is possible for L > 6 in disturbed magnetosphere conditions. The energetic protons of several tens of keV start on the night side at L=4 and have motion confined to the equatorial plane mostly under gradient magnetospheric drift. However, soon after crossing the noon-night meridian, at some point in their ExB transport trajectory, the protons are observed to abruptly depart from the equatorial plane and move towards high latitude regions. This latter motion is essentially confined to a plane perpendicular to the equator and is characterized by finite periodic motion. The calculations further indicated sudden violation of the first adiabatic invariant at the point of departure from the equatorial region, with slow variation latter along the orbit. The greater the convection electric field the higher is the energy of the protons participating in this off equatorial flow. These numerical calculations indicated that this perpendicular flow can significantly contribute to the morning-evening component of the magnetic field perturbation at storm time, populating the high latitude region by protons with energy around tens of keV. The more energetic ions, however, continue their magnetic drift around the Earth uninterruptedly and form the symmetric ring current population.
AreaCEA
Arrangement 1urlib.net > DIDAS > Ring Current Ion...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Ring Current Ion...
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4. Conditions of access and use
Languageen
Target Filescience.pdf
User Groupadministrator
marciana
sergio
Reader Groupadministrator
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Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EUFCFP
Citing Item Listsid.inpe.br/bibdigital/2013/10.04.21.53 3
sid.inpe.br/mtc-m21/2012/07.13.14.57.02 1
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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