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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnJVY/M2Gao
Repositorysid.inpe.br/mtc-m16@80/2006/08.02.13.46   (restricted access)
Last Update2006:08.02.13.46.27 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m16@80/2006/08.02.13.46.28
Metadata Last Update2021:07.18.04.01.22 (UTC) administrator
Secondary KeyINPE-13938--PRE/9118
ISSN1364-6826
Citation KeyRaulinPacKauCorMar:2006:DeSoXr
TitleOn the detectability of solar X-ray flares using very low frequency sudden phase anomalies
Year2006
MonthJune
Access Date2024, May 02
Secondary TypePRE PI
Number of Files1
Size393 KiB
2. Context
Author1 Raulin, Jean-Pierre
2 Pacini, Alessandra Abe
3 Kaufmann, Pierre
4 Correia, Emília
5 Martinez, Maria Aparecida G.
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JH2C
Group1
2 DAS-INPE-MCT-BR
3
4 DAS-INPE-MCT-BR
Affiliation1 Centro de Rádio Astronomia e Astrofísica Mackenzie, Universidade Presbiteriana Mackenzie
2 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS)
3 Centro de Rádio Astronomia e Astrofísica Mackenzie, Universidade Presbiteriana Mackenzie
4 Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS)
5 Programa de Pós-graduação em Engenharia Elétrica, Universidade Presbiteriana Mackenzie
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume68
Number9
Pages1029-1035
History (UTC)2006-08-02 13:46:28 :: simone -> administrator ::
2021-07-18 04:01:22 :: administrator -> marciana :: 2006
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsSolar flares
X-rays
Ionosphere
Solar activity cycle
Very low frequency propagation
AbstractWe have studied ionization excesses produced by enhancements of X-ray emission during solar flares using the very low frequency (VLF) response of the lower edge of the ionospheric D region. We focus on whether or not the X-rays associated with a given solar flare were responsible for a sudden phase anomaly (SPA) event, independently of the characteristics of the SPA. Approximately 1300 and 200 solar events were found to cause an ionospheric event, during periods of high and low solar activity, respectively. The main results of the present work are: (i) definite spectral characteristics are required for a solar flare to produce a measurable SPA; (ii) the probability of SPA occurrence due to faint solar flares, of X-ray class C1C2 or lower, is higher during solar minimum; (iii) the same probability for more intense solar flares (class C3 or higher) does not depend on the solar activity conditions. Our observations suggest that the low ionosphere has different sensitivities depending on the solar activity, being more sensitive when the Sun is less active. These results also constitute an observational confirmation of recent findings showing that the ionospheric reference height is lower (by about 1 km) during solar maximum.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > On the detectability...
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4. Conditions of access and use
Languageen
Target FileOn the detectability of solar x ray.pdf
User Groupadministrator
simone
Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
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 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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