Resolving the ambiguous direction of arrival of weak meteor radar trail echoes
Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different regimes: a dense and transient plasma region co-moving with the ablating meteoroid and a trail of diffusing plasma left in the atmosphere and moving with the neutral wind. Interferometric radar systems a...
Published in: | Atmospheric Measurement Techniques |
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Main Authors: | , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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Copernicus Publications
2021
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Online Access: | https://doi.org/10.5194/amt-14-3583-2021 https://noa.gwlb.de/receive/cop_mods_00056622 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00056273/amt-14-3583-2021.pdf https://amt.copernicus.org/articles/14/3583/2021/amt-14-3583-2021.pdf |
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author | Kastinen, Daniel Kero, Johan Kozlovsky, Alexander Lester, Mark |
author_facet | Kastinen, Daniel Kero, Johan Kozlovsky, Alexander Lester, Mark |
author_sort | Kastinen, Daniel |
collection | Niedersächsisches Online-Archiv NOA |
container_issue | 5 |
container_start_page | 3583 |
container_title | Atmospheric Measurement Techniques |
container_volume | 14 |
description | Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different regimes: a dense and transient plasma region co-moving with the ablating meteoroid and a trail of diffusing plasma left in the atmosphere and moving with the neutral wind. Interferometric radar systems are used to observe the meteor trails and determine their positions and drift velocities. Depending on the spatial configuration of the receiving antennas and their individual gain patterns, the voltage response can be the same for several different plane wave directions of arrival (DOAs), thereby making it impossible to determine the correct direction. A low signal-to-noise ratio (SNR) can create the same effect probabilistically even if the system contains no theoretical ambiguities. Such is the case for the standard meteor trail echo data products of the Sodankylä Geophysical Observatory SKiYMET all-sky interferometric meteor radar. Meteor trails drift slowly enough in the atmosphere and allow for temporal integration, while meteor head echo targets move too fast. Temporal integration is a common method to increase the SNR of radar signals. For meteor head echoes, we instead propose to use direct Monte Carlo (DMC) simulations to validate DOA measurements. We have implemented two separate temporal integration methods and applied them to 2222 events measured by the Sodankylä meteor radar to simultaneously test the usefulness of such DMC simulations on cases where temporal integration is possible, validate the temporal integration methods, and resolve the ambiguous SKiYMET data products. The two methods are the temporal integration of the signal spatial correlations and matched-filter integration of the individual radar channel signals. The results are compared to Bayesian inference using the DMC simulations and the standard SkiYMET data products. In the examined data set, ∼ 13 % of the events were indicated as ambiguous. Out of these, ∼ 13 % contained anomalous signals. In ∼ 95 % of all ambiguous cases with a nominal ... |
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genre | Sodankylä |
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geographic | Sodankylä |
geographic_facet | Sodankylä |
id | ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00056622 |
institution | Open Polar |
language | English |
long_lat | ENVELOPE(26.600,26.600,67.417,67.417) |
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op_doi | https://doi.org/10.5194/amt-14-3583-2021 |
op_relation | Atmospheric Measurement Techniques -- http://www.bibliothek.uni-regensburg.de/ezeit/?2505596 -- http://www.atmospheric-measurement-techniques.net/ -- 1867-8548 https://doi.org/10.5194/amt-14-3583-2021 https://noa.gwlb.de/receive/cop_mods_00056622 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00056273/amt-14-3583-2021.pdf https://amt.copernicus.org/articles/14/3583/2021/amt-14-3583-2021.pdf |
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publishDate | 2021 |
publisher | Copernicus Publications |
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spelling | ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00056622 2025-01-17T00:48:22+00:00 Resolving the ambiguous direction of arrival of weak meteor radar trail echoes Kastinen, Daniel Kero, Johan Kozlovsky, Alexander Lester, Mark 2021-05 electronic https://doi.org/10.5194/amt-14-3583-2021 https://noa.gwlb.de/receive/cop_mods_00056622 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00056273/amt-14-3583-2021.pdf https://amt.copernicus.org/articles/14/3583/2021/amt-14-3583-2021.pdf eng eng Copernicus Publications Atmospheric Measurement Techniques -- http://www.bibliothek.uni-regensburg.de/ezeit/?2505596 -- http://www.atmospheric-measurement-techniques.net/ -- 1867-8548 https://doi.org/10.5194/amt-14-3583-2021 https://noa.gwlb.de/receive/cop_mods_00056622 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00056273/amt-14-3583-2021.pdf https://amt.copernicus.org/articles/14/3583/2021/amt-14-3583-2021.pdf https://creativecommons.org/licenses/by/4.0/ uneingeschränkt info:eu-repo/semantics/openAccess article Verlagsveröffentlichung article Text doc-type:article 2021 ftnonlinearchiv https://doi.org/10.5194/amt-14-3583-2021 2024-06-26T04:40:00Z Meteor phenomena cause ionized plasmas that can be roughly divided into two distinctly different regimes: a dense and transient plasma region co-moving with the ablating meteoroid and a trail of diffusing plasma left in the atmosphere and moving with the neutral wind. Interferometric radar systems are used to observe the meteor trails and determine their positions and drift velocities. Depending on the spatial configuration of the receiving antennas and their individual gain patterns, the voltage response can be the same for several different plane wave directions of arrival (DOAs), thereby making it impossible to determine the correct direction. A low signal-to-noise ratio (SNR) can create the same effect probabilistically even if the system contains no theoretical ambiguities. Such is the case for the standard meteor trail echo data products of the Sodankylä Geophysical Observatory SKiYMET all-sky interferometric meteor radar. Meteor trails drift slowly enough in the atmosphere and allow for temporal integration, while meteor head echo targets move too fast. Temporal integration is a common method to increase the SNR of radar signals. For meteor head echoes, we instead propose to use direct Monte Carlo (DMC) simulations to validate DOA measurements. We have implemented two separate temporal integration methods and applied them to 2222 events measured by the Sodankylä meteor radar to simultaneously test the usefulness of such DMC simulations on cases where temporal integration is possible, validate the temporal integration methods, and resolve the ambiguous SKiYMET data products. The two methods are the temporal integration of the signal spatial correlations and matched-filter integration of the individual radar channel signals. The results are compared to Bayesian inference using the DMC simulations and the standard SkiYMET data products. In the examined data set, ∼ 13 % of the events were indicated as ambiguous. Out of these, ∼ 13 % contained anomalous signals. In ∼ 95 % of all ambiguous cases with a nominal ... Article in Journal/Newspaper Sodankylä Niedersächsisches Online-Archiv NOA Sodankylä ENVELOPE(26.600,26.600,67.417,67.417) Atmospheric Measurement Techniques 14 5 3583 3596 |
spellingShingle | article Verlagsveröffentlichung Kastinen, Daniel Kero, Johan Kozlovsky, Alexander Lester, Mark Resolving the ambiguous direction of arrival of weak meteor radar trail echoes |
title | Resolving the ambiguous direction of arrival of weak meteor radar trail echoes |
title_full | Resolving the ambiguous direction of arrival of weak meteor radar trail echoes |
title_fullStr | Resolving the ambiguous direction of arrival of weak meteor radar trail echoes |
title_full_unstemmed | Resolving the ambiguous direction of arrival of weak meteor radar trail echoes |
title_short | Resolving the ambiguous direction of arrival of weak meteor radar trail echoes |
title_sort | resolving the ambiguous direction of arrival of weak meteor radar trail echoes |
topic | article Verlagsveröffentlichung |
topic_facet | article Verlagsveröffentlichung |
url | https://doi.org/10.5194/amt-14-3583-2021 https://noa.gwlb.de/receive/cop_mods_00056622 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00056273/amt-14-3583-2021.pdf https://amt.copernicus.org/articles/14/3583/2021/amt-14-3583-2021.pdf |