昭和基地における遠距離VLF信号強度の測定結果
The measurement of NAA-17.8 kHz signal strength was made at Syowa Station, Antarctica, for one year from February 1970 to January 1971. The diurnal and seasonal variations of the signal strength are shown. The data were compared with other observational data associated with auroral phenomena and sol...
Main Authors: | , , , |
---|---|
Format: | Report |
Language: | Japanese |
Published: |
研究論文
1976
|
Subjects: | |
Online Access: | https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=7848 http://id.nii.ac.jp/1291/00007848/ https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=7848&item_no=1&attribute_id=18&file_no=1 |
Summary: | The measurement of NAA-17.8 kHz signal strength was made at Syowa Station, Antarctica, for one year from February 1970 to January 1971. The diurnal and seasonal variations of the signal strength are shown. The data were compared with other observational data associated with auroral phenomena and solar flares. A significant positive correlation between VLF signal strength and radio aurora occurrences was found during the nighttime. Sudden enhancements of the signal were detected, which appear to be related to the solar flares. |
---|