Effect of wave polarization on ionospheric Ohmic heating and optimal polarization

The paper starts from the polarization of the electromagnetic wave launched by the transmitter, develops an ionospheric heating model for a wide range of launching angles and polarizations of powerful heating radio waves. The electric field polarization is characterized by Q and ϕ, where Q character...

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Published in:Physics of Plasmas
Main Authors: Li, Yong, Li, Hui, Wu, Jian, Lyu, Xingbao, Yuan, Chengxun, Li, Ce, Zhou, Zhongxiang
Other Authors: Fundamental Research Funds for the Central Universities
Format: Article in Journal/Newspaper
Language:English
Published: AIP Publishing 2023
Subjects:
Online Access:http://dx.doi.org/10.1063/5.0158960
https://pubs.aip.org/aip/pop/article-pdf/doi/10.1063/5.0158960/18191359/102902_1_5.0158960.pdf
id craippubl:10.1063/5.0158960
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spelling craippubl:10.1063/5.0158960 2024-02-11T10:03:29+01:00 Effect of wave polarization on ionospheric Ohmic heating and optimal polarization Li, Yong Li, Hui Wu, Jian Lyu, Xingbao Yuan, Chengxun Li, Ce Zhou, Zhongxiang Fundamental Research Funds for the Central Universities 2023 http://dx.doi.org/10.1063/5.0158960 https://pubs.aip.org/aip/pop/article-pdf/doi/10.1063/5.0158960/18191359/102902_1_5.0158960.pdf en eng AIP Publishing Physics of Plasmas volume 30, issue 10 ISSN 1070-664X 1089-7674 Condensed Matter Physics journal-article 2023 craippubl https://doi.org/10.1063/5.0158960 2024-01-26T09:41:03Z The paper starts from the polarization of the electromagnetic wave launched by the transmitter, develops an ionospheric heating model for a wide range of launching angles and polarizations of powerful heating radio waves. The electric field polarization is characterized by Q and ϕ, where Q characterizes the relative amplitude of the electric field components and ϕ characterizes the relative phase of the electric field components. We use similarity transformation and tensor calculation in our calculations and give the optimal polarization equation using the idea of finding the maximum value of a binary function. Combining the ionospheric background data of three widely separated locations—EISCAT (polar region), Beijing (mid-latitude), and Sanya (low latitude)—we have numerically calculated and discussed the three sites based on the heating model. The following conclusions are drawn from the calculations. The Q of the optimal polarization gradually decreases and tends to be stable when the collision frequency becomes negligible relative to the ionospheric cyclotron frequency. Q also depends on the angle between the radio wave launching angle and the magnetic inclination angle. The optimal polarization angle ϕ is generally π/2 in northern hemisphere heating experiments. With the angle between the radio wave launching angle and the magnetic inclination angle increasing from 0, the optimal polarization changes from left-handed circular polarization to left-handed elliptical polarization, and when it reaches π/2, the optimal polarization becomes east–west linear polarization. These results will provide some guidance in future experiments. Article in Journal/Newspaper EISCAT AIP Publishing Physics of Plasmas 30 10
institution Open Polar
collection AIP Publishing
op_collection_id craippubl
language English
topic Condensed Matter Physics
spellingShingle Condensed Matter Physics
Li, Yong
Li, Hui
Wu, Jian
Lyu, Xingbao
Yuan, Chengxun
Li, Ce
Zhou, Zhongxiang
Effect of wave polarization on ionospheric Ohmic heating and optimal polarization
topic_facet Condensed Matter Physics
description The paper starts from the polarization of the electromagnetic wave launched by the transmitter, develops an ionospheric heating model for a wide range of launching angles and polarizations of powerful heating radio waves. The electric field polarization is characterized by Q and ϕ, where Q characterizes the relative amplitude of the electric field components and ϕ characterizes the relative phase of the electric field components. We use similarity transformation and tensor calculation in our calculations and give the optimal polarization equation using the idea of finding the maximum value of a binary function. Combining the ionospheric background data of three widely separated locations—EISCAT (polar region), Beijing (mid-latitude), and Sanya (low latitude)—we have numerically calculated and discussed the three sites based on the heating model. The following conclusions are drawn from the calculations. The Q of the optimal polarization gradually decreases and tends to be stable when the collision frequency becomes negligible relative to the ionospheric cyclotron frequency. Q also depends on the angle between the radio wave launching angle and the magnetic inclination angle. The optimal polarization angle ϕ is generally π/2 in northern hemisphere heating experiments. With the angle between the radio wave launching angle and the magnetic inclination angle increasing from 0, the optimal polarization changes from left-handed circular polarization to left-handed elliptical polarization, and when it reaches π/2, the optimal polarization becomes east–west linear polarization. These results will provide some guidance in future experiments.
author2 Fundamental Research Funds for the Central Universities
format Article in Journal/Newspaper
author Li, Yong
Li, Hui
Wu, Jian
Lyu, Xingbao
Yuan, Chengxun
Li, Ce
Zhou, Zhongxiang
author_facet Li, Yong
Li, Hui
Wu, Jian
Lyu, Xingbao
Yuan, Chengxun
Li, Ce
Zhou, Zhongxiang
author_sort Li, Yong
title Effect of wave polarization on ionospheric Ohmic heating and optimal polarization
title_short Effect of wave polarization on ionospheric Ohmic heating and optimal polarization
title_full Effect of wave polarization on ionospheric Ohmic heating and optimal polarization
title_fullStr Effect of wave polarization on ionospheric Ohmic heating and optimal polarization
title_full_unstemmed Effect of wave polarization on ionospheric Ohmic heating and optimal polarization
title_sort effect of wave polarization on ionospheric ohmic heating and optimal polarization
publisher AIP Publishing
publishDate 2023
url http://dx.doi.org/10.1063/5.0158960
https://pubs.aip.org/aip/pop/article-pdf/doi/10.1063/5.0158960/18191359/102902_1_5.0158960.pdf
genre EISCAT
genre_facet EISCAT
op_source Physics of Plasmas
volume 30, issue 10
ISSN 1070-664X 1089-7674
op_doi https://doi.org/10.1063/5.0158960
container_title Physics of Plasmas
container_volume 30
container_issue 10
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