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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZsFDuKxG/CGzmu
Repositorysid.inpe.br/marciana/2004/07.08.15.06   (restricted access)
Last Update2004:07.08.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/07.08.15.06.22
Metadata Last Update2018:06.05.01.20.56 (UTC) administrator
Secondary KeyINPE-10873-PRE/6329
ISSN0016-7169
Citation KeyGusevJayPanPugSch:2004:CoRaTr
TitleCosmic rays and trapped protons as a source of the Earth’s positron radiation belt
Year2004
Access Date2024, May 02
Secondary TypePRE PN
Number of Files1
Size667 KiB
2. Context
Author1 Gusev, Anatoly Alexandrovitch
2 Jayanthi, Udaya Bhaskaram
3 Pankov, V. M.
4 Pugacheva, G. I.
5 Schuch, Nelson Jorge
Resume Identifier1
2 8JMKD3MGP5W/3C9JJAE
3
4
5 8JMKD3MGP5W/3C9JHUD
Group1 DAS-INPE-MCT-BR
2 RSU-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, INPE, São Jose dos Campos, SP, Brasil
2 Space Research Institute of Russian Academy of Science, Moscow, Russia
3 Southern Regional Space Research Center/INPE, Santa Maria, Braz
JournalGeofísica Internacional
Volume43
Number2
Pages241-249
History (UTC)2004-12-14 12:46:04 :: sergio -> administrator ::
2006-09-29 03:08:03 :: administrator -> sergio ::
2008-01-07 12:53:22 :: sergio -> administrator ::
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
KeywordsRayos cósmicos
electrones atrapados
cinturones de radiación. / Cosmic rays
trapped protons
radiation belt
AbstractSe discute la posible existencia de un cinturón de radiación de positrones en la magnetosfera interior, su localización, su flujo y distribución de energías y la razón de e+/e-. Sugerimos que la generación de positrones es debida al decaimiento de piones cargados que nacieron en las reacciones nucleares del cinturón de protones atrapados y de los rayos cósmicos primarios con la atmósfera residual a alturas de 100 a 1000 km sobre la superficie terrestre. Se hace una comparación con datos recientes proporcionados por el experimento AMS a bordo del transbordador espacial. Abstract: The possible existence of a positron radiation belt in the inner magnetosphere of the Earth, its space localization, flux and energy distribution and the ratio of e+/e- flux are considered. We suggest for the positron generation the decay of charged pions born in nuclear reactions of the trapped radiation belt protons and of primary cosmic rays with residual atmosphere at the altitudes of 100 to 1000 km over the surface of the earth. A comparison is attempted with the recent data of AMS experiment on board the space shuttle.
AreaCEA
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4. Conditions of access and use
Languageen
Target FileGUSEV.pdf
User Groupadministrator
sergio
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
8JMKD3MGPCW/3EUFCFP
DisseminationWEBSCI; PORTALCAPES; AGU.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyright creatorhistory descriptionlevel documentstage 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 versiontype
7. Description control
e-Mail (login)marciana
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