%0 Journal Article
%@mirrorrepository sid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
%3 2009JA014788.pdf
%4 sid.inpe.br/mtc-m19@80/2010/07.29.12.22
%8 Mar.
%@issn 0926-9851
%A Muella, M. T. A. H,
%A Kherani, E. A.,
%A Paula, E. R,
%A Cerruti, A. P,
%A Kintner, P. M,
%A Kantor, I. J.,
%A Mitchell, C. N.,
%A Batista, I. S,
%A Abdu, Mangalathayil Ali,
%@secondarytype PRE PI
%B Journal of Applied Geophysics
%D 2010
%F self-archiving-INPE-MCTIC-GOV-BR
%@secondarykey INPE--PRE/
%@archivingpolicy denypublisher denyfinaldraft24
%K total electron-content, l-band scintillations, 20 november 2003, spread-f, low-latitude, ionospheric scintillation, horizontal gradients, density gradients, neutral wind, zonal drifts.
%N A03301
%P 19
%@secondarymark A2_ENGENHARIAS_I A2_ENGENHARIAS_III B1_GEOCIÊNCIAS B1_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
%T Scintillation-producing Fresnel-scale irregularities associated with the regions of steepest TEC gradients adjacent to the equatorial ionization anomaly
%V 115
%X Using ground-based GPS and digital ionosonde instruments, we have built up at latitudes of the equatorial ionization anomaly (EIA), in the Brazilian sector, a time-evolving picture of total electron content (TEC), L-band amplitude scintillations, and F region heights, and we have investigated likely reasons for the occurrence or suppression of equatorial scintillations during the disturbed period of 18-23 November 2003. During the prestorm quiet nights, scintillations are occurring postsunset, as expected; however, during the storm time period, their spatial-temporal characteristics and intensity modify significantly owing to the dramatic changes in the ionospheric plasma density distribution and in the temporal evolution of TEC. The two-dimensional maps showing both TEC and amplitude scintillations revealed strong evidence of turbulences at the Fresnel length (causing scintillations) concurrent with those regions of steepest TEC gradients adjacent to the crests of the EIA. The largest density gradients have been found to occur in an environment of increased background electron density, and their spatial distribution and location during the disturbed period may differ significantly from the magnetic quiet night pattern. However, in terms of magnitude the gradients at equatorial and low latitudes appear to not change during both magnetic quiet and disturbed conditions. The scenarios for the formation or suppression of scintillation-producing Fresnel-scale irregularities during the prestorm quiet nights and disturbed nights are discussed in view of different competing effects computed from numerical simulation techniques.
%@area CEA
%@documentstage not transferred
%@group
%@group DAE-CEA-INPE-MCT-BR
%@group DAE-CEA-INPE-MCT-BR
%@group
%@group
%@group DAE-CEA-INPE-MCT-BR
%@group
%@group DAE-CEA-INPE-MCT-BR
%@group DAE-CEA-INPE-MCT-BR
%@usergroup administrator
%@usergroup banon
%@usergroup marciana
%@nexthigherunit 8JMKD3MGPCW/3ETL868
%@affiliation Cornell Univ, Sch Elect & Comp Engn, Ithaca, NY 14853 USA.
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Cornell Univ, Sch Elect & Comp Engn, Ithaca, NY 14853 USA.
%@affiliation
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Univ Bath, Dept Elect & Elect Engn, Bath BA2 7AY, Avon, England.
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@versiontype publisher
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@doi 10.1029/2009JA014788
%2 sid.inpe.br/mtc-m19@80/2010/07.29.12.22.49