Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT

Observations of secondary radiation, stimulated electromagnetic emission (SEE), produced during ionospheric modification experiments using ground-based, high-power, high-frequency (HF) radio waves are considered. The High Frequency Active Auroral Research Program (HAARP) facility is capable of gener...

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Published in:Annales Geophysicae
Main Authors: Fu, H. Y., Scales, W. A., Bernhardt, P. A., Briczinski, S. J., Kosch, M. J., Senior, A., Rietveld, M. T., Yeoman, Timothy Kenneth, Ruohoniemi, J. M.
Format: Article in Journal/Newspaper
Language:English
Published: European Geosciences Union (EGU) 2015
Subjects:
HF
Online Access:http://www.ann-geophys.net/33/983/2015/angeo-33-983-2015.html
http://hdl.handle.net/2381/35968
https://doi.org/10.5194/angeo-33-983-2015
id ftleicester:oai:lra.le.ac.uk:2381/35968
record_format openpolar
spelling ftleicester:oai:lra.le.ac.uk:2381/35968 2023-05-15T16:04:10+02:00 Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT Fu, H. Y. Scales, W. A. Bernhardt, P. A. Briczinski, S. J. Kosch, M. J. Senior, A. Rietveld, M. T. Yeoman, Timothy Kenneth Ruohoniemi, J. M. 2015-11-30T11:34:24Z http://www.ann-geophys.net/33/983/2015/angeo-33-983-2015.html http://hdl.handle.net/2381/35968 https://doi.org/10.5194/angeo-33-983-2015 en eng European Geosciences Union (EGU) Annales Geophysicae, 2015, 33 (8), pp. 983-990 (8) 0992-7689 http://www.ann-geophys.net/33/983/2015/angeo-33-983-2015.html http://hdl.handle.net/2381/35968 doi:10.5194/angeo-33-983-2015 1432-0576 Copyright © Author(s) 2015. This work is distributed under the Creative Commons Attribution 3.0 License ( http://creativecommons.org/licenses/by/3.0/ ), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. CC-BY Science & Technology Physical Sciences Astronomy & Astrophysics Geosciences Multidisciplinary Meteorology & Atmospheric Sciences Geology Ionosphere active experiments particle acceleration plasma waves and instabilities ELECTROMAGNETIC EMISSION-SPECTRUM ION GYROHARMONIC STRUCTURES IONOSPHERIC PLASMA PUMP FREQUENCIES DOWNSHIFTED PEAK HF RADIATION INSTABILITY FEATURES CUTLASS Journal Article Article;Journal 2015 ftleicester https://doi.org/10.5194/angeo-33-983-2015 2019-03-22T20:21:14Z Observations of secondary radiation, stimulated electromagnetic emission (SEE), produced during ionospheric modification experiments using ground-based, high-power, high-frequency (HF) radio waves are considered. The High Frequency Active Auroral Research Program (HAARP) facility is capable of generating narrowband SEE in the form of stimulated Brillouin scatter (SBS) and stimulated ion Bernstein scatter (SIBS) in the SEE spectrum. Such narrowband SEE spectral lines have not been reported using the European Incoherent Scatter (EISCAT) heater facility before. This work reports the first EISCAT results of narrowband SEE spectra and compares them to SEE previously observed at HAARP during electron gyro-harmonic heating. An analysis of experimental SEE data shows observations of emission lines within 100 Hz of the pump frequency, interpreted as SBS, during the 2012 July EISCAT campaign. Experimental results indicate that SBS strengthens as the pump frequency approaches the third electron gyro-harmonic. Also, for different heater antenna beam angles, the CUTLASS radar backscatter induced by HF radio pumping is suppressed near electron gyro-harmonics, whereas electron temperature enhancement weakens as measured by EISCAT/UHF radar. The main features of these new narrowband EISCAT observations are generally consistent with previous SBS measurements at HAARP. Peer-reviewed Publisher Version Article in Journal/Newspaper EISCAT University of Leicester: Leicester Research Archive (LRA) Annales Geophysicae 33 8 983 990
institution Open Polar
collection University of Leicester: Leicester Research Archive (LRA)
op_collection_id ftleicester
language English
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
Geosciences
Multidisciplinary
Meteorology & Atmospheric Sciences
Geology
Ionosphere
active experiments
particle acceleration
plasma waves and instabilities
ELECTROMAGNETIC EMISSION-SPECTRUM
ION GYROHARMONIC STRUCTURES
IONOSPHERIC PLASMA
PUMP FREQUENCIES
DOWNSHIFTED PEAK
HF
RADIATION
INSTABILITY
FEATURES
CUTLASS
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
Geosciences
Multidisciplinary
Meteorology & Atmospheric Sciences
Geology
Ionosphere
active experiments
particle acceleration
plasma waves and instabilities
ELECTROMAGNETIC EMISSION-SPECTRUM
ION GYROHARMONIC STRUCTURES
IONOSPHERIC PLASMA
PUMP FREQUENCIES
DOWNSHIFTED PEAK
HF
RADIATION
INSTABILITY
FEATURES
CUTLASS
Fu, H. Y.
Scales, W. A.
Bernhardt, P. A.
Briczinski, S. J.
Kosch, M. J.
Senior, A.
Rietveld, M. T.
Yeoman, Timothy Kenneth
Ruohoniemi, J. M.
Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT
topic_facet Science & Technology
Physical Sciences
Astronomy & Astrophysics
Geosciences
Multidisciplinary
Meteorology & Atmospheric Sciences
Geology
Ionosphere
active experiments
particle acceleration
plasma waves and instabilities
ELECTROMAGNETIC EMISSION-SPECTRUM
ION GYROHARMONIC STRUCTURES
IONOSPHERIC PLASMA
PUMP FREQUENCIES
DOWNSHIFTED PEAK
HF
RADIATION
INSTABILITY
FEATURES
CUTLASS
description Observations of secondary radiation, stimulated electromagnetic emission (SEE), produced during ionospheric modification experiments using ground-based, high-power, high-frequency (HF) radio waves are considered. The High Frequency Active Auroral Research Program (HAARP) facility is capable of generating narrowband SEE in the form of stimulated Brillouin scatter (SBS) and stimulated ion Bernstein scatter (SIBS) in the SEE spectrum. Such narrowband SEE spectral lines have not been reported using the European Incoherent Scatter (EISCAT) heater facility before. This work reports the first EISCAT results of narrowband SEE spectra and compares them to SEE previously observed at HAARP during electron gyro-harmonic heating. An analysis of experimental SEE data shows observations of emission lines within 100 Hz of the pump frequency, interpreted as SBS, during the 2012 July EISCAT campaign. Experimental results indicate that SBS strengthens as the pump frequency approaches the third electron gyro-harmonic. Also, for different heater antenna beam angles, the CUTLASS radar backscatter induced by HF radio pumping is suppressed near electron gyro-harmonics, whereas electron temperature enhancement weakens as measured by EISCAT/UHF radar. The main features of these new narrowband EISCAT observations are generally consistent with previous SBS measurements at HAARP. Peer-reviewed Publisher Version
format Article in Journal/Newspaper
author Fu, H. Y.
Scales, W. A.
Bernhardt, P. A.
Briczinski, S. J.
Kosch, M. J.
Senior, A.
Rietveld, M. T.
Yeoman, Timothy Kenneth
Ruohoniemi, J. M.
author_facet Fu, H. Y.
Scales, W. A.
Bernhardt, P. A.
Briczinski, S. J.
Kosch, M. J.
Senior, A.
Rietveld, M. T.
Yeoman, Timothy Kenneth
Ruohoniemi, J. M.
author_sort Fu, H. Y.
title Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT
title_short Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT
title_full Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT
title_fullStr Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT
title_full_unstemmed Stimulated Brillouin scattering during electron gyro-harmonic heating at EISCAT
title_sort stimulated brillouin scattering during electron gyro-harmonic heating at eiscat
publisher European Geosciences Union (EGU)
publishDate 2015
url http://www.ann-geophys.net/33/983/2015/angeo-33-983-2015.html
http://hdl.handle.net/2381/35968
https://doi.org/10.5194/angeo-33-983-2015
genre EISCAT
genre_facet EISCAT
op_relation Annales Geophysicae, 2015, 33 (8), pp. 983-990 (8)
0992-7689
http://www.ann-geophys.net/33/983/2015/angeo-33-983-2015.html
http://hdl.handle.net/2381/35968
doi:10.5194/angeo-33-983-2015
1432-0576
op_rights Copyright © Author(s) 2015. This work is distributed under the Creative Commons Attribution 3.0 License ( http://creativecommons.org/licenses/by/3.0/ ), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
op_rightsnorm CC-BY
op_doi https://doi.org/10.5194/angeo-33-983-2015
container_title Annales Geophysicae
container_volume 33
container_issue 8
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