首页> 外文会议>2011 30th URSI General Assembly and Scientific Symposium >Comparative study of riometer absorption and GPS TEC during absorption events in the high latitude ionosphere
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Comparative study of riometer absorption and GPS TEC during absorption events in the high latitude ionosphere

机译:高纬度电离层吸收过程中测距仪吸收和GPS TEC的比较研究

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Regions of enhanced ionization are a frequent occurrence in the high latitude ionosphere, and can significantly affect the absorption of propagating radio waves in this region. Using Global Positioning System (GPS) receivers of the Canadian High Arctic Ionospheric Network (CHAIN) and co-located riometers at several high latitude stations, we have concurrently examined variations in ionospheric total electron content (TEC) and absorption of 30 MHz cosmic radio noise (CRN) for different types of ionospheric absorption events. A survey of 128 events including substorm injections, auroral precipitation and polar patches revealed four clear relationships between TEC and absorption. At stations close to auroral latitudes we found separate relationships for events associated with precipitation of low (< 20 keV) and high (< 200 keV) energy particles in addition to substorm injections. For stations located well inside the polar cap we found separate relationships associated with low energy precipitation and polar patches, while substorm injections and high energy precipitation were less frequent at these latitudes. The distinct relationships can be attributed to the nature of the absorption and TEC measurements as well as the height-dependent electron production rate for precipitating particles at a range of energies. The TEC-absorption relationships show good agreement with theoretical relationships for non-deviative absorption in the lower ionosphere and deviative absorption in the upper ionosphere.
机译:电离增强区域在高纬度电离层中经常发生,并且会严重影响该区域中传播无线电波的吸收。使用加拿大高北极电离层网络(CHAIN)的全球定位系统(GPS)接收器和几个高纬度站的并置测距仪,我们同时研究了电离层总电子含量(TEC)的变化和30 MHz宇宙无线电噪声的吸收(CRN)用于不同类型的电离层吸收事件。对包括亚暴雨注入,极光降水和极地斑块在内的128个事件的调查显示,TEC与吸收之间存在四个明确的关系。在接近极光纬度的站台上,除了亚暴雨注入外,我们还发现了与低(<20 keV)和高(<200 keV)能量粒子的降水相关的事件的独立关系。对于位于极地帽内部的台站,我们发现与低能量降水和极地斑块相关的独立关系,而在这些纬度,次风暴注入和高能量降水的频率较低。不同的关系可以归因于吸收和TEC测量的性质,以及在一定范围的能量下沉淀颗粒的高度相关的电子生产率。 TEC的吸收关系与下部电离层的非偏离吸收和上部电离层的偏离吸收的理论关系很好地吻合。

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