The Experimental Results from SURA HF Facility and CSES Satellite

Xuemin Zhang, V. Frolov, Shufan Zhao, Chen Zhou, Yalu Wang
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Abstract

Since June 2018, SURA heating facility in Russia has carried out the experiments in emitting high frequency (HF) radio waves with O-mode and disturbing the ionosphere, together with the in-orbit satellite of China Seismo-Electromagnetic Satellite (CSES). By collecting the observing data onboard CSES including electric field, in-situ plasma parameters and energetic particle flux, the results show that in local daytime no pumping waves were detected by the electric field detector (EFD) on CSES even the emitted power reaching 90 MW, and no any obvious plasma disturbances were observed from CSES. While in local nighttime, the pumping waves were clearly distinguished in HF-band electric field at the emitted frequency with the emitted power only 30MW, in which the power spectrum density of electric field was larger than the normal background to an order of magnitude, with the propagating radius exceeding 200 km. This joint experiment of SURA-CSES illustrates that, CSES can cross SURA facility within a quite near distance with present designed orbit, which can insure the effective heating time from SURA and make CSES most possibly to observe the perturbations at the topside ionosphere excited by SURA.
SURA高频设备和CSES卫星的实验结果
自2018年6月以来,俄罗斯SURA加热设施与中国地震电磁卫星在轨卫星一起开展了发射o型高频无线电波干扰电离层的实验。通过收集CSES上的电场、原位等离子体参数和高能粒子通量等观测数据,结果表明:在局部白天,即使发射功率达到90 MW, CSES上的电场探测器(EFD)也未探测到抽运波,未观测到明显的等离子体扰动。而在局部夜间,发射频率仅为30MW的高频电场中抽运波明显,其中电场功率谱密度比正常背景大一个数量级,传播半径超过200 km。这次联合实验表明,CSES在现有设计轨道上可以在相当近的距离内穿越SURA设施,保证了SURA的有效加热时间,使CSES最有可能观测到SURA激发的上层电离层扰动。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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