Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil

Detalhes bibliográficos
Autor(a) principal: Muralikrishna,Polinaya
Data de Publicação: 2007
Outros Autores: Vieira,Leandro Paulino
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Revista Brasileira de Geofísica (Online)
Texto Completo: http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600016
Resumo: Several sounding rockets carrying plasma diagnostic experiments were launched from the Brazilian rocket launching stations in Natal (5.9ºS, 35.2ºW Geog. Lat.) and Alcântara (2.31ºS, 44.4ºW Geog. Lat.). Langmuir Probes (LP) were used to measure the height profiles of electron density and electron temperature and High Frequency Capacitance (HFC) probes were used to measure electron density. The LP's were also used to measure the amplitude of electron density fluctuations. A detailed study of the characteristic features of electron density irregularities in the scale size range of less than a meter to a few kilometres, observed by rocket-borne electron density probes under different ionospheric conditions is presented here. The main objective of these studies is the identification of these irregularities from the point of view of the dynamic and electrodynamic processes responsible for their generation. The existing theories of the Rayleigh Taylor Instability (RTI) mechanism applicable for conditions of the geomagnetic equatorial ionosphere over Brazil are critically examined in the light of the observations. The observed characteristics of the irregularities during four rocket launches are compared with the theoretically expected characteristics. These results confirm the operation of a cascade process that is responsible for the generation of a wide spectrum of irregularities. The large-scale irregularities are first generated probably by the RTI mechanism that creates conditions favourable for the operation of the Cross-Field (CFI) or the Gradient Drift Instability (GDI) mechanism. From the k-spectra of irregularities it is possible to obtain the spectral index n corresponding to the height chosen. In most of the cases the estimated spectral indices agree well with those published in the literature for the cases of irregularities generated by the GDI mechanism.
id SBG-3_a3d79d12912f80d42ff126aa8d4be70c
oai_identifier_str oai:scielo:S0102-261X2007000600016
network_acronym_str SBG-3
network_name_str Revista Brasileira de Geofísica (Online)
repository_id_str
spelling Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazilspace plasmaionosphereF-regionRayleigh-Taylor instabilityCross-Field instabilitySeveral sounding rockets carrying plasma diagnostic experiments were launched from the Brazilian rocket launching stations in Natal (5.9ºS, 35.2ºW Geog. Lat.) and Alcântara (2.31ºS, 44.4ºW Geog. Lat.). Langmuir Probes (LP) were used to measure the height profiles of electron density and electron temperature and High Frequency Capacitance (HFC) probes were used to measure electron density. The LP's were also used to measure the amplitude of electron density fluctuations. A detailed study of the characteristic features of electron density irregularities in the scale size range of less than a meter to a few kilometres, observed by rocket-borne electron density probes under different ionospheric conditions is presented here. The main objective of these studies is the identification of these irregularities from the point of view of the dynamic and electrodynamic processes responsible for their generation. The existing theories of the Rayleigh Taylor Instability (RTI) mechanism applicable for conditions of the geomagnetic equatorial ionosphere over Brazil are critically examined in the light of the observations. The observed characteristics of the irregularities during four rocket launches are compared with the theoretically expected characteristics. These results confirm the operation of a cascade process that is responsible for the generation of a wide spectrum of irregularities. The large-scale irregularities are first generated probably by the RTI mechanism that creates conditions favourable for the operation of the Cross-Field (CFI) or the Gradient Drift Instability (GDI) mechanism. From the k-spectra of irregularities it is possible to obtain the spectral index n corresponding to the height chosen. In most of the cases the estimated spectral indices agree well with those published in the literature for the cases of irregularities generated by the GDI mechanism.Sociedade Brasileira de Geofísica2007-01-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600016Revista Brasileira de Geofísica v.25 suppl.2 2007reponame:Revista Brasileira de Geofísica (Online)instname:Sociedade Brasileira de Geofísica (SBG)instacron:SBG10.1590/S0102-261X2007000600016info:eu-repo/semantics/openAccessMuralikrishna,PolinayaVieira,Leandro Paulinoeng2007-11-22T00:00:00Zoai:scielo:S0102-261X2007000600016Revistahttp://www.scielo.br/rbgONGhttps://old.scielo.br/oai/scielo-oai.php||sbgf@sbgf.org.br1809-45110102-261Xopendoar:2007-11-22T00:00Revista Brasileira de Geofísica (Online) - Sociedade Brasileira de Geofísica (SBG)false
dc.title.none.fl_str_mv Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
title Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
spellingShingle Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
Muralikrishna,Polinaya
space plasma
ionosphere
F-region
Rayleigh-Taylor instability
Cross-Field instability
title_short Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
title_full Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
title_fullStr Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
title_full_unstemmed Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
title_sort Equatorial F-region irregularities generated by the Rayleigh-Taylor instability mechanism: rocket observations from Brazil
author Muralikrishna,Polinaya
author_facet Muralikrishna,Polinaya
Vieira,Leandro Paulino
author_role author
author2 Vieira,Leandro Paulino
author2_role author
dc.contributor.author.fl_str_mv Muralikrishna,Polinaya
Vieira,Leandro Paulino
dc.subject.por.fl_str_mv space plasma
ionosphere
F-region
Rayleigh-Taylor instability
Cross-Field instability
topic space plasma
ionosphere
F-region
Rayleigh-Taylor instability
Cross-Field instability
description Several sounding rockets carrying plasma diagnostic experiments were launched from the Brazilian rocket launching stations in Natal (5.9ºS, 35.2ºW Geog. Lat.) and Alcântara (2.31ºS, 44.4ºW Geog. Lat.). Langmuir Probes (LP) were used to measure the height profiles of electron density and electron temperature and High Frequency Capacitance (HFC) probes were used to measure electron density. The LP's were also used to measure the amplitude of electron density fluctuations. A detailed study of the characteristic features of electron density irregularities in the scale size range of less than a meter to a few kilometres, observed by rocket-borne electron density probes under different ionospheric conditions is presented here. The main objective of these studies is the identification of these irregularities from the point of view of the dynamic and electrodynamic processes responsible for their generation. The existing theories of the Rayleigh Taylor Instability (RTI) mechanism applicable for conditions of the geomagnetic equatorial ionosphere over Brazil are critically examined in the light of the observations. The observed characteristics of the irregularities during four rocket launches are compared with the theoretically expected characteristics. These results confirm the operation of a cascade process that is responsible for the generation of a wide spectrum of irregularities. The large-scale irregularities are first generated probably by the RTI mechanism that creates conditions favourable for the operation of the Cross-Field (CFI) or the Gradient Drift Instability (GDI) mechanism. From the k-spectra of irregularities it is possible to obtain the spectral index n corresponding to the height chosen. In most of the cases the estimated spectral indices agree well with those published in the literature for the cases of irregularities generated by the GDI mechanism.
publishDate 2007
dc.date.none.fl_str_mv 2007-01-01
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600016
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0102-261X2007000600016
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 10.1590/S0102-261X2007000600016
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv text/html
dc.publisher.none.fl_str_mv Sociedade Brasileira de Geofísica
publisher.none.fl_str_mv Sociedade Brasileira de Geofísica
dc.source.none.fl_str_mv Revista Brasileira de Geofísica v.25 suppl.2 2007
reponame:Revista Brasileira de Geofísica (Online)
instname:Sociedade Brasileira de Geofísica (SBG)
instacron:SBG
instname_str Sociedade Brasileira de Geofísica (SBG)
instacron_str SBG
institution SBG
reponame_str Revista Brasileira de Geofísica (Online)
collection Revista Brasileira de Geofísica (Online)
repository.name.fl_str_mv Revista Brasileira de Geofísica (Online) - Sociedade Brasileira de Geofísica (SBG)
repository.mail.fl_str_mv ||sbgf@sbgf.org.br
_version_ 1754820936878522368