First wind shear observation in PMSE with the tristatic EISCAT VHF radar

(c) American Geophysical Union, reprinted with permission. Article also available at source: https://doi.org/10.1002/2016JA023080 The Polar Summer Mesosphere has the lowest temperatures that occur in the entire Earth system. Water ice particles below the optically observable size range participate t...

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Published in:Journal of Geophysical Research: Space Physics
Main Authors: Mann, Ingrid, Häggström, I., Tjulin, A, Rostami, S, Anyairo, CC, Dalin, P
Format: Article in Journal/Newspaper
Language:English
Published: 2016
Subjects:
Online Access:https://hdl.handle.net/10037/11280
https://doi.org/10.1002/2016JA023080
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author Mann, Ingrid
Häggström, I.
Tjulin, A
Rostami, S
Anyairo, CC
Dalin, P
author_facet Mann, Ingrid
Häggström, I.
Tjulin, A
Rostami, S
Anyairo, CC
Dalin, P
author_sort Mann, Ingrid
collection University of Tromsø: Munin Open Research Archive
container_issue 11
container_start_page 11,271
container_title Journal of Geophysical Research: Space Physics
container_volume 121
description (c) American Geophysical Union, reprinted with permission. Article also available at source: https://doi.org/10.1002/2016JA023080 The Polar Summer Mesosphere has the lowest temperatures that occur in the entire Earth system. Water ice particles below the optically observable size range participate there in the formation of strong radar echoes (Polar Mesospheric Summer Echoes, PMSE). To study PMSE we carried out observations with the European Incoherent Scatter (EISCAT) VHF and EISCAT UHF radar simultaneously from a site near Tromsø (69.58°N, 19.2272°E) and observed VHF backscattering also with the EISCAT receivers in Kiruna (67.86°N, 20.44°E) and Sodankylä (67.36°N, 26.63°E). This is one of the first tristatic measurements with EISCAT VHF, and we therefore describe the observations and geometry in detail. We present observations made on 26 June 2013 from 7:00 to 13:00 h UT where we found similar PMSE patterns with all three VHF receivers and found signs of wind shear in PMSE. The observations suggest that the PMSE contains sublayers that move in different directions horizontally, and this points to Kelvin-Helmholtz instability possibly playing a role in PMSE formation. We find no signs of PMSE in the UHF data. The electron densities that we derive from observed incoherent scatter at UHF are at PMSE altitudes close to the noise level but possibly indicate reduced electron densities directly above the PMSE.
format Article in Journal/Newspaper
genre EISCAT
Kiruna
Sodankylä
Tromsø
genre_facet EISCAT
Kiruna
Sodankylä
Tromsø
geographic Kiruna
Sodankylä
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geographic_facet Kiruna
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long_lat ENVELOPE(26.600,26.600,67.417,67.417)
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op_doi https://doi.org/10.1002/2016JA023080
op_relation Journal of Geophysical Research - Space Physics
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doi:10.1002/2016JA023080
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spelling ftunivtroemsoe:oai:munin.uit.no:10037/11280 2025-04-13T14:18:05+00:00 First wind shear observation in PMSE with the tristatic EISCAT VHF radar Mann, Ingrid Häggström, I. Tjulin, A Rostami, S Anyairo, CC Dalin, P 2016-11-05 https://hdl.handle.net/10037/11280 https://doi.org/10.1002/2016JA023080 eng eng Journal of Geophysical Research - Space Physics FRIDAID 1431699 doi:10.1002/2016JA023080 https://hdl.handle.net/10037/11280 openAccess VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437 VDP::Mathematics and natural science: 400::Physics: 430::Space and plasma physics: 437 Journal article Tidsskriftartikkel Peer reviewed 2016 ftunivtroemsoe https://doi.org/10.1002/2016JA023080 2025-03-14T05:17:57Z (c) American Geophysical Union, reprinted with permission. Article also available at source: https://doi.org/10.1002/2016JA023080 The Polar Summer Mesosphere has the lowest temperatures that occur in the entire Earth system. Water ice particles below the optically observable size range participate there in the formation of strong radar echoes (Polar Mesospheric Summer Echoes, PMSE). To study PMSE we carried out observations with the European Incoherent Scatter (EISCAT) VHF and EISCAT UHF radar simultaneously from a site near Tromsø (69.58°N, 19.2272°E) and observed VHF backscattering also with the EISCAT receivers in Kiruna (67.86°N, 20.44°E) and Sodankylä (67.36°N, 26.63°E). This is one of the first tristatic measurements with EISCAT VHF, and we therefore describe the observations and geometry in detail. We present observations made on 26 June 2013 from 7:00 to 13:00 h UT where we found similar PMSE patterns with all three VHF receivers and found signs of wind shear in PMSE. The observations suggest that the PMSE contains sublayers that move in different directions horizontally, and this points to Kelvin-Helmholtz instability possibly playing a role in PMSE formation. We find no signs of PMSE in the UHF data. The electron densities that we derive from observed incoherent scatter at UHF are at PMSE altitudes close to the noise level but possibly indicate reduced electron densities directly above the PMSE. Article in Journal/Newspaper EISCAT Kiruna Sodankylä Tromsø University of Tromsø: Munin Open Research Archive Kiruna Sodankylä ENVELOPE(26.600,26.600,67.417,67.417) Tromsø Journal of Geophysical Research: Space Physics 121 11 11,271 11,281
spellingShingle VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
VDP::Mathematics and natural science: 400::Physics: 430::Space and plasma physics: 437
Mann, Ingrid
Häggström, I.
Tjulin, A
Rostami, S
Anyairo, CC
Dalin, P
First wind shear observation in PMSE with the tristatic EISCAT VHF radar
title First wind shear observation in PMSE with the tristatic EISCAT VHF radar
title_full First wind shear observation in PMSE with the tristatic EISCAT VHF radar
title_fullStr First wind shear observation in PMSE with the tristatic EISCAT VHF radar
title_full_unstemmed First wind shear observation in PMSE with the tristatic EISCAT VHF radar
title_short First wind shear observation in PMSE with the tristatic EISCAT VHF radar
title_sort first wind shear observation in pmse with the tristatic eiscat vhf radar
topic VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
VDP::Mathematics and natural science: 400::Physics: 430::Space and plasma physics: 437
topic_facet VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
VDP::Mathematics and natural science: 400::Physics: 430::Space and plasma physics: 437
url https://hdl.handle.net/10037/11280
https://doi.org/10.1002/2016JA023080