Experimental evidences of pre-seismic effects in the Earth's ionosphere as a reason for neutral density and temperature measurements onboard microsatellites

L. Bankov, A. Vassileva
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Abstract

Complexity of the seismic activity requires a wide number of control parameters to be used from ground-based and orbital observations to examine ionosphere-thermosphere-lithosphere coupling processes. At present, it is commonly accepted that some of the processes addressed to the ionospheric plasma response of the seismic activity include electromagnetic ULF/VLF emissions, ion density irregularities, ion drift velocity and ion composition changes, night time airglow emissions, stimulated high energy particle precipitation etc. In the present paper, experimental data from the Neutral Atmospheric Composition Spectrometer (NACS) onboard Dynamics Explorer-B (DE-B) satellite are used. In a selected case, we have observed increased neutral He concentration at 830 km altitude, preceding Guam earthquake at 0605UT on 4 January 1982 with M=6.1 magnitude of the main shock. At the maximum of the He enhancement, He density is of about 55% higher than the observed mean value over the same latitudes from the few lateral orbits before and after the earthquake. A possible explanation of such an enhancement of He is addressed to some increase of the exospheric temperature over the earthquake zone. The existence of strong geomagnetic field control to the ionospheric seismic effects could be a serious problem when we are interested of local effects over the earthquake epicentre. As an example, electromagnetic emissions associated with seismic activity often registered in a broad area around the epicentre could be observed at distant conjugate regions along the geomagnetic field line. Under the same reason, ionospheric plasma density or temperature perturbations due to Earth's seismic activity could be observed far from the earthquake epicentre. In this sense, we suggest in situ satellite measurements of the neutral composition and temperature near/and above the F-peak to be used as a new opportunity in search of additional sensitive key parameters to examine the seismic effects in the preparatory phase of a certain earthquake. It is obvious that combined ionospheric plasma and neutral gas measurements carried out onboard the satellite enlarge significantly investigation opportunities of the microsatellite platform.
地球电离层地震前效应的实验证据是微卫星上进行中性密度和温度测量的原因
地震活动的复杂性要求从地基和轨道观测中使用大量的控制参数来检查电离层-热层-岩石圈耦合过程。目前,人们普遍认为,地震活动电离层等离子体响应的过程包括电磁超低频/超低频发射、离子密度不规则、离子漂移速度和离子成分变化、夜间气辉发射、受激高能粒子沉淀等。本文采用了动力学探测- b (DE-B)卫星上的中性大气成分光谱仪(NACS)的实验数据。在一个选定的案例中,我们观察到在1982年1月4日0605UT主震M=6.1级的关岛地震之前,830公里高度的中性He浓度增加。在He增强的最大值时,He密度比地震前后几个侧向轨道在相同纬度上观测到的平均值高出约55%。对He的这种增强的一个可能的解释是,地震带上的外大气层温度有所升高。当我们对地震震中的局部效应感兴趣时,存在强地磁场对电离层地震效应的控制可能是一个严重的问题。例如,与地震活动有关的电磁辐射通常在震中周围的广阔地区记录下来,但在沿地磁力线的遥远共轭区域却可以观察到。基于同样的原因,地球地震活动引起的电离层等离子体密度或温度扰动可以在远离地震震中的地方观测到。从这个意义上说,我们建议将f峰附近和以上的中性成分和温度的原位卫星测量作为寻找其他敏感关键参数的新机会,以检查某一地震准备阶段的地震效应。卫星上进行的电离层等离子体和中性气体联合测量明显增加了微卫星平台的研究机会。
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