Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter
HF radar backscatter, which has been artificially-induced by a high power RF facility such as the EISCAT heater at Tromsø, has provided coherent radar ionospheric electric field data of unprecedented temporal resolution and accuracy. Here such data are used to investigate ULF wave processes...
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2002-09-01
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doaj-0c72f5554d92414c8168884fc557f4182020-11-25T00:24:56ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762002-09-01201487149810.5194/angeo-20-1487-2002Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatterL. J. Baddeley0L. J. Baddeley1L. J. Baddeley2T. K. Yeoman3D. M. Wright4J. A. Davies5K. J. Trattner6J. L. Roeder7Correspondence to: L. J. BaddeleyDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK(Lisa.Baddeley@ion.le.ac.uk)Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UKDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UKDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UKLockheed Martin ATC, Palo Alto, USAThe Aerospace Corporation, Los Angeles, CA, USAHF radar backscatter, which has been artificially-induced by a high power RF facility such as the EISCAT heater at Tromsø, has provided coherent radar ionospheric electric field data of unprecedented temporal resolution and accuracy. Here such data are used to investigate ULF wave processes observed by both the CUTLASS HF radars and the EISCAT UHF radar. Data from the SP-UK-OUCH experiment have revealed small-scale (high azimuthal wave number, <i>m</i> <approx> -45) waves, predominantly in the morning sector, thought to be brought about by the drift-bounce resonance processes. Conjugate observations from the Polar CAM-MICE instrument indicate the presence of a non-Maxwellian ion distribution function. Further statistical analysis has been undertaken, using the Polar TIMAS instrument, to reveal the prevalence and magnitude of the non-Maxwellian energetic particle populations thought to be responsible for generating these wave types.<br><br><b>Key words. </b>Ionosphere (active experiments; wave-particle interactions) Magnetospheric physics (MHD waves and instabilities)https://www.ann-geophys.net/20/1487/2002/angeo-20-1487-2002.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
L. J. Baddeley L. J. Baddeley L. J. Baddeley T. K. Yeoman D. M. Wright J. A. Davies K. J. Trattner J. L. Roeder |
spellingShingle |
L. J. Baddeley L. J. Baddeley L. J. Baddeley T. K. Yeoman D. M. Wright J. A. Davies K. J. Trattner J. L. Roeder Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter Annales Geophysicae |
author_facet |
L. J. Baddeley L. J. Baddeley L. J. Baddeley T. K. Yeoman D. M. Wright J. A. Davies K. J. Trattner J. L. Roeder |
author_sort |
L. J. Baddeley |
title |
Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter |
title_short |
Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter |
title_full |
Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter |
title_fullStr |
Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter |
title_full_unstemmed |
Morning sector drift-bounce resonance driven ULF waves observed in artificially-induced HF radar backscatter |
title_sort |
morning sector drift-bounce resonance driven ulf waves observed in artificially-induced hf radar backscatter |
publisher |
Copernicus Publications |
series |
Annales Geophysicae |
issn |
0992-7689 1432-0576 |
publishDate |
2002-09-01 |
description |
HF radar backscatter,
which has been artificially-induced by a high power RF facility such as the
EISCAT heater at Tromsø, has provided coherent radar ionospheric electric
field data of unprecedented temporal resolution and accuracy. Here such data
are used to investigate ULF wave processes observed by both the CUTLASS HF
radars and the EISCAT UHF radar. Data from the SP-UK-OUCH experiment have
revealed small-scale (high azimuthal wave number, <i>m</i> <approx> -45)
waves, predominantly in the morning sector, thought to be brought about by the
drift-bounce resonance processes. Conjugate observations from the Polar
CAM-MICE instrument indicate the presence of a non-Maxwellian ion distribution
function. Further statistical analysis has been undertaken, using the Polar
TIMAS instrument, to reveal the prevalence and magnitude of the non-Maxwellian
energetic particle populations thought to be responsible for generating these
wave types.<br><br><b>Key words. </b>Ionosphere (active
experiments; wave-particle interactions) Magnetospheric physics (MHD waves and
instabilities) |
url |
https://www.ann-geophys.net/20/1487/2002/angeo-20-1487-2002.pdf |
work_keys_str_mv |
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