Diurnal phase and amplitude variations of 12.1 kHz Omega signal along the auroral zone

The diurnal and seasonal variations in the phase and amplitude of Omega radio navigation signal at 12.1 kHz band (from Aldra in Norway) received at Tjornes in Iceland are analyzed in order to know the propagation mode of the VLF wave signal in high latitudes for a better understanding of the behavio...

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Bibliographic Details
Main Authors: Takashi Araki, Natsuo Sato, Ryoichi Fujii, Takashi Kikuchi
Format: Report
Language:English
Published: Faculty of Education, Hirosaki University/National Institute of Polar Research/National Institute of Polar Research/Hiraiso Solar-Terrestrial Research Center, Communications Research Laboratory 1990
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Online Access:https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=4087
http://id.nii.ac.jp/1291/00004087/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=4087&item_no=1&attribute_id=18&file_no=1
Description
Summary:The diurnal and seasonal variations in the phase and amplitude of Omega radio navigation signal at 12.1 kHz band (from Aldra in Norway) received at Tjornes in Iceland are analyzed in order to know the propagation mode of the VLF wave signal in high latitudes for a better understanding of the behavior of the lower ionosphere. It is found that the diurnal variation of the VLF phase and amplitude is closely correlated with solar zenith angle. A rapid change of VLF phase shift and VLF amplitude occurs at the times of sunrise and sunset during magnetically quiet period.