Sunrise effects on VLF signals propagating over a long north-south path

We present a detailed study of the times of amplitude minima observed on the 12-Mm path from NAA (24 kHz, 1 MW, Cutler, Maine) to Faraday, Antarctica, during the period 1990–1995. (NAA is a naval transmitter call sign.) This study represents the first account of the effect of the sunrise terminator...

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Published in:Radio Science
Main Authors: Clilverd, Mark A., Thomson, Neil R., Rodger, Craig J.
Format: Article in Journal/Newspaper
Language:unknown
Published: American Geophysical Union 1999
Subjects:
Online Access:http://nora.nerc.ac.uk/id/eprint/503087/
https://doi.org/10.1029/1999RS900052
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spelling ftnerc:oai:nora.nerc.ac.uk:503087 2023-05-15T13:48:07+02:00 Sunrise effects on VLF signals propagating over a long north-south path Clilverd, Mark A. Thomson, Neil R. Rodger, Craig J. 1999 http://nora.nerc.ac.uk/id/eprint/503087/ https://doi.org/10.1029/1999RS900052 unknown American Geophysical Union Clilverd, Mark A. orcid:0000-0002-7388-1529 Thomson, Neil R.; Rodger, Craig J. 1999 Sunrise effects on VLF signals propagating over a long north-south path. Radio Science, 34 (4). 939-948. https://doi.org/10.1029/1999RS900052 <https://doi.org/10.1029/1999RS900052> Publication - Article PeerReviewed 1999 ftnerc https://doi.org/10.1029/1999RS900052 2023-02-04T19:37:38Z We present a detailed study of the times of amplitude minima observed on the 12-Mm path from NAA (24 kHz, 1 MW, Cutler, Maine) to Faraday, Antarctica, during the period 1990–1995. (NAA is a naval transmitter call sign.) This study represents the first account of the effect of the sunrise terminator when it is parallel to a propagation path at some times of the year. Since the NAA-Faraday path is within 3° of the north-south meridian, parallel orientation happens close to the equinoxes, while the maximum angle of incidence occurs during the solstices. During the solstices the terminator takes a significant length of time to cross the entire propagation path, so modal conversion effects are observed over a range of hours. During the equinoxes, however, the leading edge of the night-day transition region crosses the whole propagation path within 20 min. The interpretation of the timing of minima is consistent with modal conversion taking place as the sunrise terminator crosses the NAA-Faraday transmission path at specific, consistent locations. The timing of minima is remarkably consistent from year to year. Long wave propagation modeling is used to show that the location of nightside minima at an altitude of 45–75 km in the subionospheric waveguide represents the location of the sunrise terminator on the great circle path when dayside minima occur. Article in Journal/Newspaper Antarc* Antarctica Natural Environment Research Council: NERC Open Research Archive Faraday ENVELOPE(-64.256,-64.256,-65.246,-65.246) Cutler ENVELOPE(-60.981,-60.981,-62.612,-62.612) Radio Science 34 4 939 948
institution Open Polar
collection Natural Environment Research Council: NERC Open Research Archive
op_collection_id ftnerc
language unknown
description We present a detailed study of the times of amplitude minima observed on the 12-Mm path from NAA (24 kHz, 1 MW, Cutler, Maine) to Faraday, Antarctica, during the period 1990–1995. (NAA is a naval transmitter call sign.) This study represents the first account of the effect of the sunrise terminator when it is parallel to a propagation path at some times of the year. Since the NAA-Faraday path is within 3° of the north-south meridian, parallel orientation happens close to the equinoxes, while the maximum angle of incidence occurs during the solstices. During the solstices the terminator takes a significant length of time to cross the entire propagation path, so modal conversion effects are observed over a range of hours. During the equinoxes, however, the leading edge of the night-day transition region crosses the whole propagation path within 20 min. The interpretation of the timing of minima is consistent with modal conversion taking place as the sunrise terminator crosses the NAA-Faraday transmission path at specific, consistent locations. The timing of minima is remarkably consistent from year to year. Long wave propagation modeling is used to show that the location of nightside minima at an altitude of 45–75 km in the subionospheric waveguide represents the location of the sunrise terminator on the great circle path when dayside minima occur.
format Article in Journal/Newspaper
author Clilverd, Mark A.
Thomson, Neil R.
Rodger, Craig J.
spellingShingle Clilverd, Mark A.
Thomson, Neil R.
Rodger, Craig J.
Sunrise effects on VLF signals propagating over a long north-south path
author_facet Clilverd, Mark A.
Thomson, Neil R.
Rodger, Craig J.
author_sort Clilverd, Mark A.
title Sunrise effects on VLF signals propagating over a long north-south path
title_short Sunrise effects on VLF signals propagating over a long north-south path
title_full Sunrise effects on VLF signals propagating over a long north-south path
title_fullStr Sunrise effects on VLF signals propagating over a long north-south path
title_full_unstemmed Sunrise effects on VLF signals propagating over a long north-south path
title_sort sunrise effects on vlf signals propagating over a long north-south path
publisher American Geophysical Union
publishDate 1999
url http://nora.nerc.ac.uk/id/eprint/503087/
https://doi.org/10.1029/1999RS900052
long_lat ENVELOPE(-64.256,-64.256,-65.246,-65.246)
ENVELOPE(-60.981,-60.981,-62.612,-62.612)
geographic Faraday
Cutler
geographic_facet Faraday
Cutler
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation Clilverd, Mark A. orcid:0000-0002-7388-1529
Thomson, Neil R.; Rodger, Craig J. 1999 Sunrise effects on VLF signals propagating over a long north-south path. Radio Science, 34 (4). 939-948. https://doi.org/10.1029/1999RS900052 <https://doi.org/10.1029/1999RS900052>
op_doi https://doi.org/10.1029/1999RS900052
container_title Radio Science
container_volume 34
container_issue 4
container_start_page 939
op_container_end_page 948
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