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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3SNHMP2
Repositorysid.inpe.br/mtc-m21c/2019/02.12.10.39   (restricted access)
Last Update2019:02.12.10.39.11 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21c/2019/02.12.10.39.11
Metadata Last Update2020:01.06.11.42.09 (UTC) administrator
DOI10.1186/s40645-019-0258-1
ISSN2197-4284
Citation KeyAbdu:2019:DaShVa
TitleDay-to-day and short-term variabilities in the equatorial plasma bubble/spread F irregularity seeding and development
Year2019
MonthDec.
Access Date2024, May 06
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2459 KiB
2. Context
AuthorAbdu, Mangalathayil Ali
Resume Identifier8JMKD3MGP5W/3C9JHNK
ORCID0000-0001-9970-0258
GroupDIDAE-CGCEA-INPE-MCTIC-GOV-BR
AffiliationInstituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Addressabdu.managa@gmail.com
JournalProgress in Earth and Planetary Science
Volume6
Number1
Pagese11
History (UTC)2019-02-12 10:39:26 :: simone -> administrator :: 2019
2020-01-06 11:42:09 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsEquatorial ionosphere
Plasma bubbles/spread F irregularities
Prereversal vertical drift
Prompt penetration electric field
Gravity waves
Trans-equatorial wind
Planetary/Kelvin waves
ESF/EPB short-term variability
AbstractThe background ionospheric conditions shaped by sunset electrodynamic processes are responsible for the development of equatorial plasma bubble (EPB)/equatorial spread F (ESF) irregularities of the post-sunset ionosphere. Distinct conditions exist for the EPB/ESF development also at later hours of the night. The plasma instability growth leading to EPB generation is dependent on the basic precursor conditions defined by the well-known parameters: the evening prereversal enhancement in vertical plasma drift (PRE), wave structure in plasma density and polarization electric field required to initiate/seed the instability, and the F layer bottom side density gradient, as a significant factor in controlling the growth rate. Competing roles of the zonal versus meridional thermospheric winds additionally control their development. Statistical as well as case studies have addressed aspects of the EPB development and occurrence under different geophysical conditions, generally focusing attention on any one of the above specific parameters. Little is known regarding the relative importance of concurrent presence of the precursor parameters (mentioned above) in shaping a given event. A large degree of day-to-day variability in these parameters arise from different sources of forcing, such as upward propagating atmospheric waves, and magnetic disturbance time electric fields in the form of prompt penetration and disturbance dynamo electric fields that often contribute to the widely observed short-term variabilities in EPB development and dynamics. In this paper, we will present and discuss some important aspects of the EPB/ ESF short-term variability, focusing attention on their enhanced development, or suppression and, wherever possible, highlighting also the relative roles of the precursor parameters in such variability.
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4. Conditions of access and use
Languageen
Target Fileabdu_day.pdf
User Groupsimone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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