HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING.
On 12 November 2001, artificial optical annuli were produced using the EISCAT high-frequency (HF) ionospheric Heating facility. This unusual phenomenon was induced using O-mode transmissions at 5.423 MHz with 550 MW effective isotropic radiated power and the pump beam dipped 9 degrees south. The pum...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.626.7752 2023-05-15T16:04:23+02:00 HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING. Mina Ashrafi A M. J. Kosch A F. Honary A The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.626.7752 http://eprints.lancs.ac.uk/6680/1/Ashrafi_ASR_2006.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.626.7752 http://eprints.lancs.ac.uk/6680/1/Ashrafi_ASR_2006.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://eprints.lancs.ac.uk/6680/1/Ashrafi_ASR_2006.pdf text ftciteseerx 2016-01-08T15:15:43Z On 12 November 2001, artificial optical annuli were produced using the EISCAT high-frequency (HF) ionospheric Heating facility. This unusual phenomenon was induced using O-mode transmissions at 5.423 MHz with 550 MW effective isotropic radiated power and the pump beam dipped 9 degrees south. The pump frequency corresponds to the fourth electron gyro-harmonic frequency at 215 km altitude. The EISCAT UHF radar observed a persistent pump-induced enhancement in the ion line data near the HF reflection altitude. The optical and radar signatures of HF pumping started at∼230 km and descended to∼220 km within ∼60 s. This effect has been modelled using the solution to differential equations describing pump-induced electron temperature and density perturbations. The decrease in altitude of the ion line by∼10 km and changes in electron density have been modelled. The results show that an electron temperature enhancement of up to ∼5700 K can be achieved, which is not sufficient to explain the observed optical emissions. Key words: Ionospheric heating; Electron acceleration 1 Text EISCAT Unknown |
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On 12 November 2001, artificial optical annuli were produced using the EISCAT high-frequency (HF) ionospheric Heating facility. This unusual phenomenon was induced using O-mode transmissions at 5.423 MHz with 550 MW effective isotropic radiated power and the pump beam dipped 9 degrees south. The pump frequency corresponds to the fourth electron gyro-harmonic frequency at 215 km altitude. The EISCAT UHF radar observed a persistent pump-induced enhancement in the ion line data near the HF reflection altitude. The optical and radar signatures of HF pumping started at∼230 km and descended to∼220 km within ∼60 s. This effect has been modelled using the solution to differential equations describing pump-induced electron temperature and density perturbations. The decrease in altitude of the ion line by∼10 km and changes in electron density have been modelled. The results show that an electron temperature enhancement of up to ∼5700 K can be achieved, which is not sufficient to explain the observed optical emissions. Key words: Ionospheric heating; Electron acceleration 1 |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Mina Ashrafi A M. J. Kosch A F. Honary A |
spellingShingle |
Mina Ashrafi A M. J. Kosch A F. Honary A HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING. |
author_facet |
Mina Ashrafi A M. J. Kosch A F. Honary A |
author_sort |
Mina Ashrafi A |
title |
HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING. |
title_short |
HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING. |
title_full |
HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING. |
title_fullStr |
HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING. |
title_full_unstemmed |
HEATER-INDUCED ALTITUDE DESCENT OF THE EISCAT UHF ION LINE ENHANCEMENTS: OBSERVATIONS AND MODELLING. |
title_sort |
heater-induced altitude descent of the eiscat uhf ion line enhancements: observations and modelling. |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.626.7752 http://eprints.lancs.ac.uk/6680/1/Ashrafi_ASR_2006.pdf |
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EISCAT |
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EISCAT |
op_source |
http://eprints.lancs.ac.uk/6680/1/Ashrafi_ASR_2006.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.626.7752 http://eprints.lancs.ac.uk/6680/1/Ashrafi_ASR_2006.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766400023337107456 |