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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZsFDuKxG/EGMii
Repositorysid.inpe.br/marciana/2005/01.07.16.01   (restricted access)
Last Update2005:06.13.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2005/01.07.16.01.59
Metadata Last Update2018:06.05.01.21.24 (UTC) administrator
Secondary KeyINPE-12553-PRE/7850
ISSN0103-9733
Citation KeyPugachevaGusJaySchCho:2004:SeCuRa
TitleSeasonal cusp radiation belts on dayside magnetosphere
Year2004
MonthDec.
Access Date2024, Apr. 27
Secondary TypePRE PN
Number of Files1
Size554 KiB
2. Context
Author1 Pugacheva, G. I.
2 Gusev, A. A.
3 Jayanthi, Udaya Bhaskaram
4 Schuch, Nelson Jorge
5 Choque, K. T.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JJAE
4 8JMKD3MGP5W/3C9JHUD
Group1 RSU-INPE-MCT-BR
2 DAS-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Unidade de Santa Maria
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofisica(INPE,DAS)
JournalBrazilian Journal of Physics
Volume34
Number4A
Pages1478-1485
History (UTC)2006-03-17 18:07:43 :: jefferson -> administrator ::
2018-06-05 01:21:24 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsMAGNETIC-FIELD
MODEL
PARTICLES
SHEET
AbstractThe possibility of quasi-stable trapping of charged particles of hundreds keV to MeV energy on the frontside Earth magnetosphere is explored in by numerical modeling of the single particle orbits in the geomagnetic field utilizing empirical Tsyganenko magnetic field model. Due to solar wind pressure the remote magnetic field lines on the frontside of the magnetosphere exhibit two minima in the geomagnetic field strength along the field line in high latitudes on the both sides of the equator. These minima may result in stable confinement structures, a kind of radiation belts, in the northern or/and the southern hemispheres, providing energetic particle trapping for times from several minutes to duration of seasonal scale. Simulation of energetic proton orbits passing through the regions of the magnetic field minima with different disturbance level and the Earth's tilt reveals conditions in which these trapped radiation zones could result. It is shown that the existence of the adiabatic confinement zones strongly depends on the seasonal inclination of the Earth's rotation axis. As a result the northern cusp confinement zone appears only in a summer solstice and similarly the southern cusp capture zone appears only in a winter solstice. In equinox time the confinement zones exist in both hemispheres in the disturbed magnetospheric conditions, however, they are less pronounced. The zones are essentially restricted to the sunlit magnetosphere. They form a kind of cusp radiation ring/belt, where a proton drifts with a period of several minutes, conserving its 1(st) and the 2(nd) adiabatic invariants. The latitudinal width of the ring is very thin, about 2-5 latitudinal degrees. The proton orbits passing through the off-equatorial field minimum opposite to those cusp belts reveal another interesting effect: a bound of the geomagnetic equatorial plane on the day sector. These and other features of the confinement zones in the two minima off-equatorial magnetic field regions are discussed.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Seasonal cusp radiation...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > CRCRS > Seasonal cusp radiation...
doc Directory Contentaccess
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agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileSeasonal cusp radiation.pdf
User Groupadministrator
jefferson
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EUFCFP
DisseminationWEBSCI; PORTALCAPES; SCIELO.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
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7. Description control
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