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ORBITING NANO-SATELLITES FOR EARTHQUAKE PREDICTION (ONSEP), A FEASIBILITY STUDY.

机译:轨道纳米卫星用于地震预报(ONSEP),一项可行性研究。

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The ONSEP mission is a proposed nano-satcllitc constellation mission which is intended to perform measurements in the VLF (Very Low Frequency) and HF (High Frequency) bands in Low Earth Orbit (LEO) to understand the pre-scismic anomalies (in particular scismic-clcctromagnetic mechanisms) occurring in the ionosphere, which will help predict earthquakes. Over the last 25 years, ground based and satellite based observations have been carried out to understand the precursory signatures that could help reliably predict earthquakes. The ionosphere is a portion of the atmosphere that is densely populated with ionized particles and contains plasma, helping in long distance radio communications. But, the characteristics of the ionosphere have been highly un-prcdictablc due to its dependence on various phenomena such as solar activity, thunder-storms, earth-quakes, volcanic eruptions and man-made noise. The seismo-clectromagnctic process prior to an earth-quake have proven to be a reliable pre-scismic phenomenon for short-term prediction of earth-quakes. The plate tectonics close to the epicenter of an earthquake cause the rocks to compress and expand, causing a piezoelectric effect. As a result of this tribo-electric effect and rising warm gases, Earth's surface potential around the epicenter changes and this creates anomalies in the earth's electric field and subsequently the ion density in the ionosphere. The associated anomalies have been observed over a wide frequency range from DC to VHF. The observations made by the DEMETER mission launched in 2004 have ronfirmed these anomalies. The results and observations made by the ICE (Instrument Champ Elcctrique) instrument on-board DEMETER mission is used as a case study to derive the mission requirements for the ONSEP mission. The primary mission objective of ONSEP is to perform measurements in the VLF and HF bands to record the anomalies during pcr-scismic activities, at the time of an earthquake and post-seismic activities and compare it with the measurements carried out during thunder-storms, volcanic-eruptions and other man-made noise. A feasibility study is performed to see if the OLFAR (Orbiting Low Frequency Antennas for Radio astronomy) payload (which forms a Low frequency radio-telescope), can also be used as the primary payload for the ONSEP mission. The main advantage of using a constellation concept for earthquake prediction is, apart from providing wider-coverage and better temporal resolution, that simultaneous measurements carricd-out by the constellation of satellites will provide more consistent data and will help in predicting the location of seismic activity more accurately.
机译:ONSEP任务是一项拟议的纳米卫星星座任务,旨在在低地球轨道(LEO)的VLF(甚低频)和HF(高频)波段进行测量,以了解前断层异常(特别是地震)电离层中发生的-clcctromagnetic机制),这将有助于预测地震。在过去的25年中,已经进行了基于地面和基于卫星的观测,以了解可以帮助可靠地预测地震的先兆特征。电离层是大气中充满电离粒子并包含等离子体的一部分,有助于进行长距离无线电通信。但是,电离层的特性由于其对各种现象的依赖而高度不实用,例如太阳活动,雷暴,地震,火山喷发和人为噪声。地震之前的地震-静磁过程已被证明是对地震的短期预测的可靠的断前现象。靠近地震震中的板块构造使岩石压缩并膨胀,从而产生压电效应。由于这种摩擦电效应和上升的温暖气体的影响,震中周围的地球表面电势发生了变化,这在地球电场中产生了异常,随后在电离层中产生了离子密度。在从直流到甚高频的较宽频率范围内都观察到了相关的异常现象。 2004年启动的DEMETER任务组的观测结果证实了这些异常现象。 ICE(仪器冠军Elcctrique)机载DEMETER任务的结果和观察结果被用作案例研究,以得出ONSEP任务的任务要求。 ONSEP的主要任务目标是在VLF和HF波段进行测量,以记录地震和地震后活动期间pcr断层活动期间的异常,并将其与雷暴期间进行的测量相比较,火山喷发和其他人为噪音。进行了可行性研究,以查看OLFAR(射电天文学用低频天线)有效载荷(形成低频无线电望远镜)是否也可以用作ONSEP任务的主要有效载荷。使用星座概念进行地震预测的主要优势在于,除了提供更广泛的覆盖范围和更好的时间分辨率外,卫星星座同时进行的测量还将提供更一致的数据,并有助于预测地震活动的位置更精确地。

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