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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZsFDuKxG/EGLMo
Repositorysid.inpe.br/marciana/2005/01.07.15.39   (restricted access)
Last Update2005:06.13.03.00.00 (UTC) jefferson
Metadata Repositorysid.inpe.br/marciana/2005/01.07.15.39.26
Metadata Last Update2018:06.05.01.21.24 (UTC) administrator
Secondary KeyINPE-12555-PRE/7852
ISSN0273-1177
Citation KeyPugachevaGusJaySchSpj:2004:TrAnPr
TitleTrapped antiprotons produced by cosmic rays in the eartth's magnetosphere
Year2004
Access Date2024, May 06
Secondary TypePRE PI
Number of Files1
Size280 KiB
2. Context
Author1 Pugacheva, G.
2 Gusev, A. A.
3 Jayanthi, Udaya Bhaskaram
4 Schuch, Nelson Jorge
5 Spjeldvik, W. N.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JJAE
4 8JMKD3MGP5W/3C9JHUD
Group1 RSU-INPE-MCT-BR
2 DAS-INPE-MCT-BR
3 RSU-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espacais, Divisão de Astrofisica(INPE,DAS)
2 Instituto Nacional de Pesquisas Espacais, Unidade Regional Sul de Pesquisas Espaciais
3 Russian Acad Sci, Space Res Inst, Moscow, Russia
4 Soutthern Regional Space Research Center - CRSPE/INPE - MCT, Santa Maria, Brazil
5 Weber State Univ, Ogden, UT 84408 USA
JournalAdvances in Space Research
Volume34
Number6
Pages1433-1437
History (UTC)2006-06-14 22:52:16 :: jefferson -> administrator ::
2008-06-10 22:28:55 :: administrator -> jefferson ::
2011-05-28 18:10:13 :: jefferson -> administrator ::
2012-10-21 21:50:22 :: administrator -> jefferson :: 2004
2013-02-27 12:48:59 :: jefferson -> administrator :: 2004
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
Version Typepublisher
Keywordsantiprotons
cosmic rays
Earth's magnetosphere
trapped particles/PROTON
AbstractThe existence of significant fluxes of antiparticles in the Earth magnetosphere has been predicted on theoretical considerations in this article. These antiparticles (positrons or antiprotons) at several hundred kilometers of altitudes, we believe are not of direct extraterrestrial origin, but are the natural products of nuclear reactions of the high energy primary cosmic rays (CR) and trapped protons (TP) confined in the terrestrial radiation belt, with the constituents of terrestrial atmosphere. Extraterrestrial positrons and antiprotons born in nuclear reactions of the same CR particles passing through only 5-7 g/cm(2) of interstellar matter, exhibit lower fluxes compared to the antiprotons born at hundreds of g/cm(2) in the atmosphere, which when confined in the magnetic field of the Earth (in any other planet), get accumulated. We present the results of the computations of the antiproton fluxes at 10 MeV to several GeV energies due to CR particle interactions with the matter in the interstellar space, and also with the residual atmosphere at altitudes of similar to1000 km over the Earth's surface. The estimates show that the magnetospheric antiproton fluxes are greater by two orders of magnitude compared to the extraterrestrial fluxes measured at energies < 1-2 GeV. (C) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
AreaCEA
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doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filetrapped.pdf
User Groupadministrator
jefferson
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
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
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