The trimpi effect in antarctica: observations and models

LEP (lightning electron precipitation) bursts can be detected on the ground because they cause transient perturbations (known as ‘Trimpi events’) in the received amplitude and phase of subionospherically propagating radio waves, typically at VLF. The occurrence of mid-latitude Trimpis at Halley (eve...

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Published in:Journal of Atmospheric and Terrestrial Physics
Main Authors: Smith, A.J., Cotton, P.D.
Format: Article in Journal/Newspaper
Language:unknown
Published: Elsevier 1990
Subjects:
Online Access:http://nora.nerc.ac.uk/id/eprint/520874/
https://doi.org/10.1016/0021-9169(90)90103-T
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spelling ftnerc:oai:nora.nerc.ac.uk:520874 2023-05-15T13:49:35+02:00 The trimpi effect in antarctica: observations and models Smith, A.J. Cotton, P.D. 1990-05 http://nora.nerc.ac.uk/id/eprint/520874/ https://doi.org/10.1016/0021-9169(90)90103-T unknown Elsevier Smith, A.J.; Cotton, P.D. 1990 The trimpi effect in antarctica: observations and models. Journal of Atmospheric and Terrestrial Physics, 52 (5). 341-355. https://doi.org/10.1016/0021-9169(90)90103-T <https://doi.org/10.1016/0021-9169(90)90103-T> Publication - Article PeerReviewed 1990 ftnerc https://doi.org/10.1016/0021-9169(90)90103-T 2023-02-04T19:47:02Z LEP (lightning electron precipitation) bursts can be detected on the ground because they cause transient perturbations (known as ‘Trimpi events’) in the received amplitude and phase of subionospherically propagating radio waves, typically at VLF. The occurrence of mid-latitude Trimpis at Halley (events observed on five nights per month at equinox) is similar to other ( L$̃4 ) stations e.g. Siple and Eights, and much less than for lower latitude stations such as Palmer or Faraday ( L$̃2.5 ), nearer to the active LEP belt at 2 ⩽ L ⩽ 3. Activity is mainly on approximately north— south paths from NSS and NAA. In one case study of simultaneous Trimpi activity on the NSS-Halley and NAA-Halley paths, events were not synchronised, implying precipitation regions ⩽ 200–300 km in east-west extent. The maximum amplitude and phase excursions of a sequence of events on the NSS-Halley path oscillated sinusoidally in quadrature this was consistent with the echo Trimpi model of Dowden and Adams, assuming an echo signal 15 dB down on the direct signal, with the velocity of the precipitation region perpendicular to the propagation path changing the phase path difference between direct and echo signals by one wavelength (14 km at 21.4 kHz) in about 23 min. Burst precipitation of energetic electrons at high latitudes, close to, and poleward of, the plasmapause, can be well studied by means of the Trimpi effect using the Siple VLF transmitter and a network of VLF receivers in Antarctica (Siple, Faraday/Palmer, Halley, and South Pole). A high-latitude, low VLF waveguide mode propagation computer model for use in such studies has been developed, and tested against observations of controlled transmissions from a dipole antenna of variable (simulated) orientation. Published observations of Trimpi events in this high-latitude region are well reproduced by the model. A new experiment— OPALnet— designed to investigate LEP through its effects on the phase and amplitude of signals from the Omega VLF navigational network, is described. Its ... Article in Journal/Newspaper Antarc* Antarctica South pole South pole Natural Environment Research Council: NERC Open Research Archive South Pole Siple ENVELOPE(-83.917,-83.917,-75.917,-75.917) Faraday ENVELOPE(-64.256,-64.256,-65.246,-65.246) Trimpi ENVELOPE(-72.782,-72.782,-75.345,-75.345) Journal of Atmospheric and Terrestrial Physics 52 5 341 355
institution Open Polar
collection Natural Environment Research Council: NERC Open Research Archive
op_collection_id ftnerc
language unknown
description LEP (lightning electron precipitation) bursts can be detected on the ground because they cause transient perturbations (known as ‘Trimpi events’) in the received amplitude and phase of subionospherically propagating radio waves, typically at VLF. The occurrence of mid-latitude Trimpis at Halley (events observed on five nights per month at equinox) is similar to other ( L$̃4 ) stations e.g. Siple and Eights, and much less than for lower latitude stations such as Palmer or Faraday ( L$̃2.5 ), nearer to the active LEP belt at 2 ⩽ L ⩽ 3. Activity is mainly on approximately north— south paths from NSS and NAA. In one case study of simultaneous Trimpi activity on the NSS-Halley and NAA-Halley paths, events were not synchronised, implying precipitation regions ⩽ 200–300 km in east-west extent. The maximum amplitude and phase excursions of a sequence of events on the NSS-Halley path oscillated sinusoidally in quadrature this was consistent with the echo Trimpi model of Dowden and Adams, assuming an echo signal 15 dB down on the direct signal, with the velocity of the precipitation region perpendicular to the propagation path changing the phase path difference between direct and echo signals by one wavelength (14 km at 21.4 kHz) in about 23 min. Burst precipitation of energetic electrons at high latitudes, close to, and poleward of, the plasmapause, can be well studied by means of the Trimpi effect using the Siple VLF transmitter and a network of VLF receivers in Antarctica (Siple, Faraday/Palmer, Halley, and South Pole). A high-latitude, low VLF waveguide mode propagation computer model for use in such studies has been developed, and tested against observations of controlled transmissions from a dipole antenna of variable (simulated) orientation. Published observations of Trimpi events in this high-latitude region are well reproduced by the model. A new experiment— OPALnet— designed to investigate LEP through its effects on the phase and amplitude of signals from the Omega VLF navigational network, is described. Its ...
format Article in Journal/Newspaper
author Smith, A.J.
Cotton, P.D.
spellingShingle Smith, A.J.
Cotton, P.D.
The trimpi effect in antarctica: observations and models
author_facet Smith, A.J.
Cotton, P.D.
author_sort Smith, A.J.
title The trimpi effect in antarctica: observations and models
title_short The trimpi effect in antarctica: observations and models
title_full The trimpi effect in antarctica: observations and models
title_fullStr The trimpi effect in antarctica: observations and models
title_full_unstemmed The trimpi effect in antarctica: observations and models
title_sort trimpi effect in antarctica: observations and models
publisher Elsevier
publishDate 1990
url http://nora.nerc.ac.uk/id/eprint/520874/
https://doi.org/10.1016/0021-9169(90)90103-T
long_lat ENVELOPE(-83.917,-83.917,-75.917,-75.917)
ENVELOPE(-64.256,-64.256,-65.246,-65.246)
ENVELOPE(-72.782,-72.782,-75.345,-75.345)
geographic South Pole
Siple
Faraday
Trimpi
geographic_facet South Pole
Siple
Faraday
Trimpi
genre Antarc*
Antarctica
South pole
South pole
genre_facet Antarc*
Antarctica
South pole
South pole
op_relation Smith, A.J.; Cotton, P.D. 1990 The trimpi effect in antarctica: observations and models. Journal of Atmospheric and Terrestrial Physics, 52 (5). 341-355. https://doi.org/10.1016/0021-9169(90)90103-T <https://doi.org/10.1016/0021-9169(90)90103-T>
op_doi https://doi.org/10.1016/0021-9169(90)90103-T
container_title Journal of Atmospheric and Terrestrial Physics
container_volume 52
container_issue 5
container_start_page 341
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