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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/43H2N8L
Repositorysid.inpe.br/mtc-m21c/2020/11.03.13.51
Last Update2020:11.03.13.51.17 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2020/11.03.13.51.17
Metadata Last Update2022:01.04.01.35.32 (UTC) administrator
DOI10.1029/2020JA027773
ISSN2169-9402
Citation KeyAbduKherSous:2020:SoMiMa
TitleRole of bottom-side density gradient in the development of equatorial plasma bubble/spread F irregularities: solar minimum and maximum conditions
Year2020
MonthOct
Access Date2024, May 20
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size5252 KiB
2. Context
Author1 Abdu, Mangalathayil Ali
2 Kherani, Esfhan Alam
3 Sousasantos, J.
Resume Identifier1 8JMKD3MGP5W/3C9JHNK
ORCID1 0000-0001-5857-5761
2 0000-0003-0182-2252
Group1 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
2 DIDAE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Tecnológico de Aeronáutica (ITA)
Author e-Mail Address1 abdu.manga@gmail.com
2 esfhan.kherani@inpe.br
JournalJournal of Geophysical Research: Space Physics
Volume125
Number10
Pagese2020JA027773
History (UTC)2020-11-03 13:51:17 :: simone -> administrator ::
2020-11-03 13:51:18 :: administrator -> simone :: 2020
2020-11-03 13:51:43 :: simone -> administrator :: 2020
2022-01-04 01:35:32 :: administrator -> simone :: 2020
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractFrom the analysis of Digisonde data over Brazilian equatorial and low‐latitude sites, we investigate the relative importance of the different parameters driving the generation of rising bubble‐type and bottom‐type spread F (SF) irregularities. Data for the complete month of October 2001, a solar maximum epoch (F10.7 = 210), and that of October 2008, an extended solar minimum period (F10.7 = 70), are analyzed to examine the SF intensity and occurrence rate as a function of the evening prereversal vertical drift velocity and the corresponding F layer heights and the bottom‐side density gradient. While the SF at the equatorial site is indicative of both the bottom‐side irregularities and rising bubbles, the SF at the low latitude represents exclusively the latter. Comparison of the results, from the two epochs, reveals a large decrease in the intensity and occurrence rate of plasma bubbles, with a decrease in solar flux. But a notable increase in these characteristics is observed in the case of bottom‐side SF. It is found that a larger (steeper) density gradient of the F layer bottom side that exists in the low solar flux condition is responsible for an enhanced Raleigh‐Taylor instability growth, counterbalancing a reduction in this rate that may arise from a smaller prereversal vertical drift and lower layer height that also characterize the low solar flux condition. Thus, the role of the bottom‐side density gradient in the ESF instability growth has been identified for the first time in terms of its ability to explain the contrasting irregularity features as observed during solar flux maximum and minimum years.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Role of bottom-side...
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34R/43H2N8L
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34R/43H2N8L
Languageen
Target Fileabdu_role.pdf
User Groupsimone
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.54.26 2
sid.inpe.br/bibdigital/2013/09.29.20.43 1
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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