Evidence of X-mode heating suppressing O-mode heating

In this study, we present three experiments carried out at the EISCAT (European Incoherent Scatter Scientific Association) heating facility on October 29 and 30, 2015. The results from the first experiment showed overshoot during the O-mode heating period. The second experiment, which used cold-star...

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Bibliographic Details
Published in:Earth and Planetary Physics
Main Authors: Ting Feng, Chen Zhou, Xiang Wang, MoRan Liu, ZhengYu Zhao
Format: Article in Journal/Newspaper
Language:English
Published: Science Press 2020
Subjects:
ionospheric heating
parametric decay instability
thermal parametric instability
overshoot
suppression
envir
archi
EISCAT
Online Access:https://doi.org/10.26464/epp2020068
https://doaj.org/article/6ab2f7641fb64684b94a98086999516a
Description
Summary:In this study, we present three experiments carried out at the EISCAT (European Incoherent Scatter Scientific Association) heating facility on October 29 and 30, 2015. The results from the first experiment showed overshoot during the O-mode heating period. The second experiment, which used cold-start X-mode heating, showed the generation of parametric decay instability, whereas overshoot was not observed. The third experiment used power-stepped X-mode heating with noticeable O-mode wave leakage. Parametric decay instability and oscillating two-stream instability were generated at the O-mode reflection height without the overshoot effect, which implies suppression of the thermal parametric instability with X-mode heating. We propose that the electron temperature increased because X-mode heating below the upper hybrid height decreased the growth rate of the thermal parametric instability.

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