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1. Identity statement
Reference TypeJournal Article
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/GUMmd
Repositorysid.inpe.br/iris@1905/2005/07.29.23.55
Last Update2017:12.18.18.08.57 (UTC) marciana
Metadata Repositorysid.inpe.br/iris@1905/2005/07.29.23.55.25
Metadata Last Update2018:06.06.04.04.04 (UTC) administrator
Secondary KeyINPE-8690-PRE/4426
ISSN0148-0227
2156-2202
Label9626
Citation KeyPintoPintMend:1996:XRaMi
TitleX ray microbursts in the South Atlantic magnetic anomaly
Year1996
MonthMay
Access Date2024, May 01
Secondary TypePRE PI
Number of Files1
Size437 KiB
2. Context
Author1 Pinto, Osmar
2 Pinto, Iara Regina Cardoso de Almeida
3 Mendes Jr., Odim
Group1 DGE-INPE-MCT-BR
JournalJournal of Geophysical Research
Volume101
Number(A5)
Pages10909-10917
History (UTC)2014-09-29 15:13:44 :: administrator -> marciana :: 1996
2017-12-18 18:08:57 :: marciana -> administrator :: 1996
2018-06-06 04:04:04 :: administrator -> marciana :: 1996
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGEOFÍSICA ESPACIAL
raios x
microexlorações (meteorologia)
medição
anomalias magnéticas
x ray
microburst (meteorogy)
measurement
magnetic anomalies
AbstractBalloon-borne X ray measurements with high time resolution were carried out in the South Atlantic magnetic anomaly to investigate the fine structure of the precipitation in this region. Measurements were obtained on two balloon flights launched from Cachoeira Paulista, Sao Paulo, Brazil, on January 26 and February 1, 1994, and were supported by onboard electric field and geomagnetic field ground data. In one flight, we have found that rapid changes do occur in times of about 0.05 s during periods of a few seconds. They should be considered as the first evidence of the presence of microbursts in the low L value region of the South Atlantic anomaly. These microbursts were not correlated with sferic signatures in the same hemisphere and may be correlated with magnetic fluctuations in the geomagnetic field. Energy-time features of the microbursts are examined in order to identify possible responsible mechanisms.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > X ray microbursts...
doc Directory Contentaccess
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4. Conditions of access and use
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zipped data URLhttp://urlib.net/zip/6qtX3pFwXQZ3r59YCT/GUMmd
Target File8690.pdf
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Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
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5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.22.11 1
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2001/04.03.15.36
6. Notes
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