Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars

The results of high latitude ionospheric modification experiments utilising the EISCAT heating facility at Tromsø are presented. As a result of the interaction between the high power pump waves and upper hybrid waves in the ionosphere, field-aligned electron density irregularities are artificially e...

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Published in:Annales Geophysicae
Main Authors: Wright, D. M., Davies, J. A., Yeoman, T. K., Robinson, T. R., Shergill, H.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-24-543-2006
https://angeo.copernicus.org/articles/24/543/2006/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo35756 2023-05-15T16:04:29+02:00 Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars Wright, D. M. Davies, J. A. Yeoman, T. K. Robinson, T. R. Shergill, H. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-24-543-2006 https://angeo.copernicus.org/articles/24/543/2006/ eng eng doi:10.5194/angeo-24-543-2006 https://angeo.copernicus.org/articles/24/543/2006/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-24-543-2006 2020-07-20T16:27:17Z The results of high latitude ionospheric modification experiments utilising the EISCAT heating facility at Tromsø are presented. As a result of the interaction between the high power pump waves and upper hybrid waves in the ionosphere, field-aligned electron density irregularities are artificially excited. Observations of these structures with the CUTLASS coherent HF radars and the EISCAT incoherent UHF radar exhibit hysteresis effects as the heater output power is varied. These are explained in terms of the two-stage mechanism which leads to the growth of the irregularities. Experiments which involve preconditioning of the ionosphere also indicate that hysteresis could be exploited to maximise the intensity of the field-aligned irregularities, especially where the available heater power is limited. In addition, the saturation of the irregularity amplitude is considered. Although, the rate of irregularity growth becomes less rapid at high heater powers it does not seem to fully saturate, indicating that the amplification would continue beyond the capabilities of the Tromsø heater - currently the most powerful of its kind. It is shown that the CUTLASS radars are sensitive to irregularities produced by very low heater powers (effective radiated powers <4 MW). This fact is discussed from the perspective of a new heating facility, SPEAR, located on Spitzbergen and capable of transmitting high frequency radio waves with an effective radiated power ~10% of that of the Tromsø heater (28MW). Text EISCAT Spitzbergen Tromsø Copernicus Publications: E-Journals Tromsø Annales Geophysicae 24 2 543 553
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The results of high latitude ionospheric modification experiments utilising the EISCAT heating facility at Tromsø are presented. As a result of the interaction between the high power pump waves and upper hybrid waves in the ionosphere, field-aligned electron density irregularities are artificially excited. Observations of these structures with the CUTLASS coherent HF radars and the EISCAT incoherent UHF radar exhibit hysteresis effects as the heater output power is varied. These are explained in terms of the two-stage mechanism which leads to the growth of the irregularities. Experiments which involve preconditioning of the ionosphere also indicate that hysteresis could be exploited to maximise the intensity of the field-aligned irregularities, especially where the available heater power is limited. In addition, the saturation of the irregularity amplitude is considered. Although, the rate of irregularity growth becomes less rapid at high heater powers it does not seem to fully saturate, indicating that the amplification would continue beyond the capabilities of the Tromsø heater - currently the most powerful of its kind. It is shown that the CUTLASS radars are sensitive to irregularities produced by very low heater powers (effective radiated powers <4 MW). This fact is discussed from the perspective of a new heating facility, SPEAR, located on Spitzbergen and capable of transmitting high frequency radio waves with an effective radiated power ~10% of that of the Tromsø heater (28MW).
format Text
author Wright, D. M.
Davies, J. A.
Yeoman, T. K.
Robinson, T. R.
Shergill, H.
spellingShingle Wright, D. M.
Davies, J. A.
Yeoman, T. K.
Robinson, T. R.
Shergill, H.
Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars
author_facet Wright, D. M.
Davies, J. A.
Yeoman, T. K.
Robinson, T. R.
Shergill, H.
author_sort Wright, D. M.
title Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars
title_short Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars
title_full Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars
title_fullStr Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars
title_full_unstemmed Saturation and hysteresis effects in ionospheric modification experiments observed by the CUTLASS and EISCAT radars
title_sort saturation and hysteresis effects in ionospheric modification experiments observed by the cutlass and eiscat radars
publishDate 2018
url https://doi.org/10.5194/angeo-24-543-2006
https://angeo.copernicus.org/articles/24/543/2006/
geographic Tromsø
geographic_facet Tromsø
genre EISCAT
Spitzbergen
Tromsø
genre_facet EISCAT
Spitzbergen
Tromsø
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-24-543-2006
https://angeo.copernicus.org/articles/24/543/2006/
op_doi https://doi.org/10.5194/angeo-24-543-2006
container_title Annales Geophysicae
container_volume 24
container_issue 2
container_start_page 543
op_container_end_page 553
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