Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica

The measurements of vector electric fields and currents were made with two plastic balloons of 5,000 m^3 launched from Syowa Station (L=8.4), Antarctica, on 28 November and 29 December, 1972. The results give the following. (1) The vertical electric field and current at the altitude of 30km are 0.12...

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Bibliographic Details
Main Authors: Yoshikazu TANAKA, Toshio OGAWA, Masahiro KODAMA
Format: Article in Journal/Newspaper
Language:English
Published: National Institute of Polar Research 1975
Subjects:
geo
Online Access:https://doi.org/10.15094/00007830
https://doaj.org/article/006987ea4a3547dbb6a2fc7c772453c4
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spelling fttriple:oai:gotriple.eu:oai:doaj.org/article:006987ea4a3547dbb6a2fc7c772453c4 2023-05-15T13:38:53+02:00 Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica Yoshikazu TANAKA Toshio OGAWA Masahiro KODAMA 1975-12-01 https://doi.org/10.15094/00007830 https://doaj.org/article/006987ea4a3547dbb6a2fc7c772453c4 en other eng National Institute of Polar Research doi:10.15094/00007830 0085-7289 2432-079X https://doaj.org/article/006987ea4a3547dbb6a2fc7c772453c4 undefined Antarctic Record, Iss 54, Pp 18-33 (1975) geo Journal Article https://vocabularies.coar-repositories.org/resource_types/c_6501/ 1975 fttriple https://doi.org/10.15094/00007830 2023-01-22T19:15:58Z The measurements of vector electric fields and currents were made with two plastic balloons of 5,000 m^3 launched from Syowa Station (L=8.4), Antarctica, on 28 November and 29 December, 1972. The results give the following. (1) The vertical electric field and current at the altitude of 30km are 0.12-0.21 V/m and 1.3-2.2 x10^ A/m^2 respectively, and their diurnal variations are roughly consistent with the expected variation from the average world-wide thunderstorm activity. (2) The electrical conductivities were estimated from the ratio of the electric current to the electric field giving the average value of 1 x 10^ mho/m at the altitude of 30 km. This value is about twice as large as that in Japan. This can be explained by the latitudinal effect of the cosmic ray ionization in the atmosphere. (3) Enhancements of the electric field and current were observed in both vertical and horizontal components of the magnitude of about 80 mV/m and 0.8 x 10^ A/m^2 respectively at an initial stage of a magnetic substorm. The vertical electric field on the ground was also correspondingly enhanced by about 80 V/m at the same time. (4) Comparisons of observed horizontal electric field vectors with the magnetic fields observed at Syowa Station show that the magnetic field variations are caused by the ionospheric Hall current. (5) One hour averages of the horizontal electric field show large scale convection fields consistent with S^p_q in the polar ionosphere and with DP-2 in the equatorial magnetosphere. The average ionospheric and magnetospheric equatorial electric fields were 40 mV/m and 0.98 mV/m respectively, and corresponding plasma convection velocities were estimated to be 700 m/s and 22 km/s respectively. Article in Journal/Newspaper Antarc* Antarctica Unknown Syowa Station
institution Open Polar
collection Unknown
op_collection_id fttriple
language English
topic geo
spellingShingle geo
Yoshikazu TANAKA
Toshio OGAWA
Masahiro KODAMA
Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica
topic_facet geo
description The measurements of vector electric fields and currents were made with two plastic balloons of 5,000 m^3 launched from Syowa Station (L=8.4), Antarctica, on 28 November and 29 December, 1972. The results give the following. (1) The vertical electric field and current at the altitude of 30km are 0.12-0.21 V/m and 1.3-2.2 x10^ A/m^2 respectively, and their diurnal variations are roughly consistent with the expected variation from the average world-wide thunderstorm activity. (2) The electrical conductivities were estimated from the ratio of the electric current to the electric field giving the average value of 1 x 10^ mho/m at the altitude of 30 km. This value is about twice as large as that in Japan. This can be explained by the latitudinal effect of the cosmic ray ionization in the atmosphere. (3) Enhancements of the electric field and current were observed in both vertical and horizontal components of the magnitude of about 80 mV/m and 0.8 x 10^ A/m^2 respectively at an initial stage of a magnetic substorm. The vertical electric field on the ground was also correspondingly enhanced by about 80 V/m at the same time. (4) Comparisons of observed horizontal electric field vectors with the magnetic fields observed at Syowa Station show that the magnetic field variations are caused by the ionospheric Hall current. (5) One hour averages of the horizontal electric field show large scale convection fields consistent with S^p_q in the polar ionosphere and with DP-2 in the equatorial magnetosphere. The average ionospheric and magnetospheric equatorial electric fields were 40 mV/m and 0.98 mV/m respectively, and corresponding plasma convection velocities were estimated to be 700 m/s and 22 km/s respectively.
format Article in Journal/Newspaper
author Yoshikazu TANAKA
Toshio OGAWA
Masahiro KODAMA
author_facet Yoshikazu TANAKA
Toshio OGAWA
Masahiro KODAMA
author_sort Yoshikazu TANAKA
title Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica
title_short Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica
title_full Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica
title_fullStr Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica
title_full_unstemmed Startospheric Electric Fields and Currents Measured at Syowa Station, Antarctica
title_sort startospheric electric fields and currents measured at syowa station, antarctica
publisher National Institute of Polar Research
publishDate 1975
url https://doi.org/10.15094/00007830
https://doaj.org/article/006987ea4a3547dbb6a2fc7c772453c4
geographic Syowa Station
geographic_facet Syowa Station
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source Antarctic Record, Iss 54, Pp 18-33 (1975)
op_relation doi:10.15094/00007830
0085-7289
2432-079X
https://doaj.org/article/006987ea4a3547dbb6a2fc7c772453c4
op_rights undefined
op_doi https://doi.org/10.15094/00007830
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