On TID Observation program in the Auroral Zone

On TID Observation program in the Auroral Zone

A future plan of TID observation at Syowa Station by means of the HF Doppler technique is proposed. The purpose of the observation is to locate the generation source of the medium-scale TID, and also to estimate the temperature of the neutral atmosphere at the ionospheric heights by observing the di...

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Bibliographic Details
Main Authors: Tai-ichi KITAMURA, Tohru OGAWA
Format: Article
Language:English
Published: National Institute of Polar Research 1979-03-01
Series:Antarctic Record
Online Access:https://doi.org/10.15094/00008057
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spelling doaj-54825bd760ff4e88966a3bbeb61954922020-11-25T00:30:00ZengNational Institute of Polar ResearchAntarctic Record0085-72892432-079X1979-03-0165758010.15094/00008057On TID Observation program in the Auroral ZoneTai-ichi KITAMURA0Tohru OGAWA1Department of Physics, Kyushu UniversityIonospheric Research Laboratory, Kyoto UniversityA future plan of TID observation at Syowa Station by means of the HF Doppler technique is proposed. The purpose of the observation is to locate the generation source of the medium-scale TID, and also to estimate the temperature of the neutral atmosphere at the ionospheric heights by observing the dispersion of the gravity waves. A network of observation stations (one receiving station (Syowa Station) and three transmitting stations), assuming the distance between paired stations to be 80 km to 300 km, is necessary to carry out the above purpose. The electric power at a station is expected to be supplied by the windmill generator.https://doi.org/10.15094/00008057
collection DOAJ
language English
format Article
sources DOAJ
author Tai-ichi KITAMURA
Tohru OGAWA
spellingShingle Tai-ichi KITAMURA
Tohru OGAWA
On TID Observation program in the Auroral Zone
Antarctic Record
author_facet Tai-ichi KITAMURA
Tohru OGAWA
author_sort Tai-ichi KITAMURA
title On TID Observation program in the Auroral Zone
title_short On TID Observation program in the Auroral Zone
title_full On TID Observation program in the Auroral Zone
title_fullStr On TID Observation program in the Auroral Zone
title_full_unstemmed On TID Observation program in the Auroral Zone
title_sort on tid observation program in the auroral zone
publisher National Institute of Polar Research
series Antarctic Record
issn 0085-7289
2432-079X
publishDate 1979-03-01
description A future plan of TID observation at Syowa Station by means of the HF Doppler technique is proposed. The purpose of the observation is to locate the generation source of the medium-scale TID, and also to estimate the temperature of the neutral atmosphere at the ionospheric heights by observing the dispersion of the gravity waves. A network of observation stations (one receiving station (Syowa Station) and three transmitting stations), assuming the distance between paired stations to be 80 km to 300 km, is necessary to carry out the above purpose. The electric power at a station is expected to be supplied by the windmill generator.
url https://doi.org/10.15094/00008057
work_keys_str_mv AT taiichikitamura ontidobservationprogramintheauroralzone
AT tohruogawa ontidobservationprogramintheauroralzone
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