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首页> 外文期刊>Natural Hazards and Earth System Sciences Discussions >Ionosperic anomaly due to seismic activities – Part 1: Calibration of the VLF signal of VTX 18.2 KHz station from Kolkata and deviation during seismic events
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Ionosperic anomaly due to seismic activities – Part 1: Calibration of the VLF signal of VTX 18.2 KHz station from Kolkata and deviation during seismic events

机译:由于地震活动引起的IONOSPERIC异常 - 第1部分:VTX 18.2 kHz站VLF信号的校准从加尔各答和地震事件中的偏差

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VLF signals are long thought to give away important information about the lithosphere-ionosphere coupling. In order to establish co-relations, if any, between the ionospheric activities and the earthquakes, we need to understand what the reference signals are, throughout the year. The best opportunity to do this is during the period of solar minimum where the number of flares and sunspots are negligible and the data would be primarily affected by the sun and variation would be due to normal sunset and sunrise effects. In this paper, we present the result of the sunrise and sunset terminators as a function of the day of the year for a period of four years, viz, 2005–2008 when the solar activity was very low. The terminators are for the 18.2 KHz VTX signal of the Indian Navy as observed from Indian Centre for Space Physics receiving station located in Kolkata. A total of 624 days of data have been used to obtain the mean plot. Any deviation of observations from this so-called the standardized calibration curve would point to influences by terrestrial (such as earthquakes) and extra-terrestrial events (such as solar activities). We present examples of deviations which occur in a period of 16 months and show that the correlation with seismic events is significant and typically the highest deviation takes place up to a couple of days prior to the seismic event. Simultaneous observations of such deviations from more than one station could improve the predictability of earthquakes.
机译:VLF信号很长,旨在释放有关岩石圈电离层耦合的重要信息。为了建立共同关系,如果在电离层活动和地震之间,我们需要了解一年中的参考信号。这样做的最佳机会是在太阳能最小期间,耀斑和太阳黑子的数量可以忽略不计,数据主要受太阳的影响,变化是由于正常的日落和日出效果。在本文中,我们展示了日出和日落终止者作为一年中的一年中的一天,2005 - 2008年太阳能活动非常低的一年。终结者是印度海军的18.2kHz VTX信号,从位于加尔各答的印度空间物理接收站观察到。已经使用总共624天的数据来获得平均图。这种所谓的标准化校准曲线的观察结果的任何偏差都将指向陆地(如地震)和超级事件(如太阳能活动)的影响。我们提出了在16个月的时间内发生的偏差的例子,并表明与地震事件的相关性显着,通常最高偏差在地震事件前发生了几天。同时观察来自多个站的这种偏差可以提高地震的可预测性。

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