Evidence of X-mode heating suppressing O-mode heating

被引:3
|
作者
Feng, Ting [1 ]
Zhou, Chen [1 ]
Wang, Xiang [1 ]
Liu, MoRan [1 ]
Zhao, ZhengYu [1 ]
机构
[1] Wuhan Univ, Sch Elect Informat, Dept Space Phys, Wuhan 430072, Peoples R China
基金
中国博士后科学基金; 瑞典研究理事会; 中国国家自然科学基金; 英国自然环境研究理事会;
关键词
ionospheric heating; parametric decay instability; thermal parametric instability; overshoot; suppression; STIMULATED ELECTROMAGNETIC EMISSION; IONOSPHERIC MODIFICATION; INSTABILITY; EXCITATION; WAVES; TURBULENCE; FIELD;
D O I
10.26464/epp2020068
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
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.
引用
收藏
页码:588 / 597
页数:10
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