Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region

The electron rate of recombination and collision frequency of electrons with neutrals depend on the electron temperature, which is, at E-region heights, greater than the neutral temperature even for geomagnetically quiet conditions; therefore in order to perform theoretical computations of electron...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Duhau, S., De La Vega, M., Azpiazu, M.C.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00320633_v35_n1_p1_Duhau
Aporte de:
id todo:paper_00320633_v35_n1_p1_Duhau
record_format dspace
spelling todo:paper_00320633_v35_n1_p1_Duhau2023-10-03T14:44:42Z Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region Duhau, S. De La Vega, M. Azpiazu, M.C. The electron rate of recombination and collision frequency of electrons with neutrals depend on the electron temperature, which is, at E-region heights, greater than the neutral temperature even for geomagnetically quiet conditions; therefore in order to perform theoretical computations of electron number and electric current densities, the usual hypothesis that both temperatures are equal at those heights is removed in the present paper. Instead, an empirical model of E-region electron temperature is used and all the data were carefully selected so that they correspond to equivalent ionospheric and solar conditions. It is found that: the electron number density, depends strongly on the electron temperature, being well predicted by the present model; the shape of the vertical profile of the electrical conductivity is mainly determined by the electron number density profile, and the shape of the vertical current density thus calculated is in good agreement with the measured one. At the dip equator, a discrepancy between the intensity of the measured and computed current densities around the height of the electrojet peak still remains, which could be due to an anomalous reduction of the electric field there, as is suggested by the agreement found a few degrees beyond the dip. © 1987. Fil:Duhau, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:De La Vega, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Azpiazu, M.C. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00320633_v35_n1_p1_Duhau
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description The electron rate of recombination and collision frequency of electrons with neutrals depend on the electron temperature, which is, at E-region heights, greater than the neutral temperature even for geomagnetically quiet conditions; therefore in order to perform theoretical computations of electron number and electric current densities, the usual hypothesis that both temperatures are equal at those heights is removed in the present paper. Instead, an empirical model of E-region electron temperature is used and all the data were carefully selected so that they correspond to equivalent ionospheric and solar conditions. It is found that: the electron number density, depends strongly on the electron temperature, being well predicted by the present model; the shape of the vertical profile of the electrical conductivity is mainly determined by the electron number density profile, and the shape of the vertical current density thus calculated is in good agreement with the measured one. At the dip equator, a discrepancy between the intensity of the measured and computed current densities around the height of the electrojet peak still remains, which could be due to an anomalous reduction of the electric field there, as is suggested by the agreement found a few degrees beyond the dip. © 1987.
format JOUR
author Duhau, S.
De La Vega, M.
Azpiazu, M.C.
spellingShingle Duhau, S.
De La Vega, M.
Azpiazu, M.C.
Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region
author_facet Duhau, S.
De La Vega, M.
Azpiazu, M.C.
author_sort Duhau, S.
title Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region
title_short Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region
title_full Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region
title_fullStr Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region
title_full_unstemmed Effect of the electron temperature in the electron number density and dynamics of the equatorial E-region
title_sort effect of the electron temperature in the electron number density and dynamics of the equatorial e-region
url http://hdl.handle.net/20.500.12110/paper_00320633_v35_n1_p1_Duhau
work_keys_str_mv AT duhaus effectoftheelectrontemperatureintheelectronnumberdensityanddynamicsoftheequatorialeregion
AT delavegam effectoftheelectrontemperatureintheelectronnumberdensityanddynamicsoftheequatorialeregion
AT azpiazumc effectoftheelectrontemperatureintheelectronnumberdensityanddynamicsoftheequatorialeregion
_version_ 1807316904439709696