THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS

In the propagation of VLF pulses in earth-ionosphere waveguide, the spectrums of pulses vary and frequency components of 2-4 kHz are absorbed seriously. According to the principle that the VLF pulse spectrums change with propagation distance, a new method is proposed to determine if whistler waves u...

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Bibliographic Details
Main Authors: ZHOU, HB, SUN, CL, XIAO, Z
Other Authors: CHINESE ACAD SCI,CTR SPACE SCI & APPL RES,BEIJING,PEOPLES R CHINA., BEIJING UNIV,DEPT GEOPHYS,BEIJING,PEOPLES R CHINA.
Format: Journal/Newspaper
Language:English
Published: acta geophysica sinica 1990
Subjects:
WHISTLER
EXIT POINT
SPECTRUM ANALYSIS
WAVE-GUIDE PROPAGATION
South Pole
South pole
Online Access:https://hdl.handle.net/20.500.11897/403564
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spelling ftpekinguniv:oai:localhost:20.500.11897/403564 2023-05-15T18:22:09+02:00 THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS ZHOU, HB SUN, CL XIAO, Z CHINESE ACAD SCI,CTR SPACE SCI & APPL RES,BEIJING,PEOPLES R CHINA. BEIJING UNIV,DEPT GEOPHYS,BEIJING,PEOPLES R CHINA. 1990 https://hdl.handle.net/20.500.11897/403564 en eng acta geophysica sinica ACTA GEOPHYSICA SINICA.1990,33,(3),367-371. 1028350 0001-5733 http://hdl.handle.net/20.500.11897/403564 WOS:A1990EQ15100015 SCI WHISTLER EXIT POINT SPECTRUM ANALYSIS WAVE-GUIDE PROPAGATION Journal 1990 ftpekinguniv https://doi.org/20.500.11897/403564 2021-08-01T10:27:27Z In the propagation of VLF pulses in earth-ionosphere waveguide, the spectrums of pulses vary and frequency components of 2-4 kHz are absorbed seriously. According to the principle that the VLF pulse spectrums change with propagation distance, a new method is proposed to determine if whistler waves undergo waveguide propagation before they are picked up. By analysing whistler spectrum of the South Pole, we can determine whistler exit points from this method. The results are in good agreement with that of other experimental method. Geochemistry & Geophysics SCI(E) 0 NOTE 3 367-371 33 Journal/Newspaper South pole Peking University Institutional Repository (PKU IR) South Pole
institution Open Polar
collection Peking University Institutional Repository (PKU IR)
op_collection_id ftpekinguniv
language English
topic WHISTLER
EXIT POINT
SPECTRUM ANALYSIS
WAVE-GUIDE PROPAGATION
spellingShingle WHISTLER
EXIT POINT
SPECTRUM ANALYSIS
WAVE-GUIDE PROPAGATION
ZHOU, HB
SUN, CL
XIAO, Z
THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS
topic_facet WHISTLER
EXIT POINT
SPECTRUM ANALYSIS
WAVE-GUIDE PROPAGATION
description In the propagation of VLF pulses in earth-ionosphere waveguide, the spectrums of pulses vary and frequency components of 2-4 kHz are absorbed seriously. According to the principle that the VLF pulse spectrums change with propagation distance, a new method is proposed to determine if whistler waves undergo waveguide propagation before they are picked up. By analysing whistler spectrum of the South Pole, we can determine whistler exit points from this method. The results are in good agreement with that of other experimental method. Geochemistry & Geophysics SCI(E) 0 NOTE 3 367-371 33
author2 CHINESE ACAD SCI,CTR SPACE SCI & APPL RES,BEIJING,PEOPLES R CHINA.
BEIJING UNIV,DEPT GEOPHYS,BEIJING,PEOPLES R CHINA.
format Journal/Newspaper
author ZHOU, HB
SUN, CL
XIAO, Z
author_facet ZHOU, HB
SUN, CL
XIAO, Z
author_sort ZHOU, HB
title THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS
title_short THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS
title_full THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS
title_fullStr THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS
title_full_unstemmed THE DETERMINATION OF WHISTLER EXIT POINTS FROM SPECTRUM ANALYSIS
title_sort determination of whistler exit points from spectrum analysis
publisher acta geophysica sinica
publishDate 1990
url https://hdl.handle.net/20.500.11897/403564
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source SCI
op_relation ACTA GEOPHYSICA SINICA.1990,33,(3),367-371.
1028350
0001-5733
http://hdl.handle.net/20.500.11897/403564
WOS:A1990EQ15100015
op_doi https://doi.org/20.500.11897/403564
_version_ 1766201523984924672

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