Conjugacy of ELF emission spectra and powers

P(論文) Conjugate observations of ELF emissions were carried out at Syowa Station in Antarctica and Husafell in Iceland from July 29 to September 18,1977. The conjugacy of ELF emissions depends on the emission types and local time. The intensity of auroral chorus is always much stronger at Husafell th...

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Main Authors: Sato, Masahiko, Maezawa, Kiyoshi, Fukunishi, Hiroshi, Sato, Natsuo
Language:English
Published: 1983
Subjects:
Online Access:https://nipr.repo.nii.ac.jp/record/1412/files/KJ00000012046.pdf
id ftnipr:oai:nipr.repo.nii.ac.jp:00001412
record_format openpolar
spelling ftnipr:oai:nipr.repo.nii.ac.jp:00001412 2024-09-09T19:08:31+00:00 Conjugacy of ELF emission spectra and powers Sato, Masahiko Maezawa, Kiyoshi Fukunishi, Hiroshi Sato, Natsuo 1983-03 application/pdf https://nipr.repo.nii.ac.jp/record/1412/files/KJ00000012046.pdf eng eng Memoirs of National Institute of Polar Research. Special issue 26 91 102 AA00733561 https://nipr.repo.nii.ac.jp/record/1412/files/KJ00000012046.pdf 1983 ftnipr 2024-06-17T04:00:39Z P(論文) Conjugate observations of ELF emissions were carried out at Syowa Station in Antarctica and Husafell in Iceland from July 29 to September 18,1977. The conjugacy of ELF emissions depends on the emission types and local time. The intensity of auroral chorus is always much stronger at Husafell than at Syowa. Frequency-time (f-t) spectral patterns of polar chorus emissions depend on local time at conjugate-pair stations. In the morning sector (06-09 MLT) the lower frequency band at Syowa is stronger than that at Husafell. The conjugacy of emission patterns in f-t spectra is more complex in the daytime sector (09-14MLT), but the following tendencies are found : i) Differences in the center frequency of each event at the conjugate stations are less than 0.2kHz in the interval of 09-11 MLT, and in the interval of 11-14 MLT these become larger up to 0.5kHz. ii) The power of emissions in the frequency range higher than 0.8kHz at Husafell is about 10 dB stronger than that at Syowa. iii) Higher cutoff frequency of polar chorus is about 1kHz at Syowa, while that at Husafell extends over 1.5kHz. Statistically, polar chorus emissions are more often observed at Husafell in the whole local time. Furthermore, occurrences of polar chorus at the conjugate stations depend on geomagnetic activity. When geomagnetic activity is quiet (Kp≤1) emissions are often observed at Syowa, but emissions are more often observed at Husafell in the moderate and disturbed periods (Kp≥2). departmental bulletin paper Other/Unknown Material Antarc* Antarctica Iceland Memoirs of National Institute of Polar Research Polar Research National Institute of Polar Research Repository, Japan Husafell ENVELOPE(-20.893,-20.893,64.700,64.700) Syowa Station
institution Open Polar
collection National Institute of Polar Research Repository, Japan
op_collection_id ftnipr
language English
description P(論文) Conjugate observations of ELF emissions were carried out at Syowa Station in Antarctica and Husafell in Iceland from July 29 to September 18,1977. The conjugacy of ELF emissions depends on the emission types and local time. The intensity of auroral chorus is always much stronger at Husafell than at Syowa. Frequency-time (f-t) spectral patterns of polar chorus emissions depend on local time at conjugate-pair stations. In the morning sector (06-09 MLT) the lower frequency band at Syowa is stronger than that at Husafell. The conjugacy of emission patterns in f-t spectra is more complex in the daytime sector (09-14MLT), but the following tendencies are found : i) Differences in the center frequency of each event at the conjugate stations are less than 0.2kHz in the interval of 09-11 MLT, and in the interval of 11-14 MLT these become larger up to 0.5kHz. ii) The power of emissions in the frequency range higher than 0.8kHz at Husafell is about 10 dB stronger than that at Syowa. iii) Higher cutoff frequency of polar chorus is about 1kHz at Syowa, while that at Husafell extends over 1.5kHz. Statistically, polar chorus emissions are more often observed at Husafell in the whole local time. Furthermore, occurrences of polar chorus at the conjugate stations depend on geomagnetic activity. When geomagnetic activity is quiet (Kp≤1) emissions are often observed at Syowa, but emissions are more often observed at Husafell in the moderate and disturbed periods (Kp≥2). departmental bulletin paper
author Sato, Masahiko
Maezawa, Kiyoshi
Fukunishi, Hiroshi
Sato, Natsuo
spellingShingle Sato, Masahiko
Maezawa, Kiyoshi
Fukunishi, Hiroshi
Sato, Natsuo
Conjugacy of ELF emission spectra and powers
author_facet Sato, Masahiko
Maezawa, Kiyoshi
Fukunishi, Hiroshi
Sato, Natsuo
author_sort Sato, Masahiko
title Conjugacy of ELF emission spectra and powers
title_short Conjugacy of ELF emission spectra and powers
title_full Conjugacy of ELF emission spectra and powers
title_fullStr Conjugacy of ELF emission spectra and powers
title_full_unstemmed Conjugacy of ELF emission spectra and powers
title_sort conjugacy of elf emission spectra and powers
publishDate 1983
url https://nipr.repo.nii.ac.jp/record/1412/files/KJ00000012046.pdf
long_lat ENVELOPE(-20.893,-20.893,64.700,64.700)
geographic Husafell
Syowa Station
geographic_facet Husafell
Syowa Station
genre Antarc*
Antarctica
Iceland
Memoirs of National Institute of Polar Research
Polar Research
genre_facet Antarc*
Antarctica
Iceland
Memoirs of National Institute of Polar Research
Polar Research
op_relation Memoirs of National Institute of Polar Research. Special issue
26
91
102
AA00733561
https://nipr.repo.nii.ac.jp/record/1412/files/KJ00000012046.pdf
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