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D-region ionosphere response to the total solar eclipse of 22 July 2009 deduced from ELF-VLF tweek observations in the Indian sector

机译:根据印度部分地区的ELF-VLF tweek观测得出的D区电离层对2009年7月22日日全食的响应

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摘要

Observations of tweeks with higher harmonics (n > 1) at low latitude stations Allahabad and Nainital, in the Indian sector, during the total solar eclipse on 22 July 2009, are presented. Allahabad and Nainital stations were in 100% and 85% of the totality paths. Observations suggest that about 30-40% obscuration of solar disc can lead to the tweeks occurrence which otherwise occur only in nighttime. A total of 148 tweeks at Allahabad and 20 tweeks at Nainital were recorded with some of them up to 3rd harmonics. The World Wide Lightning Location Network data indicated that tweeks observed were generated by lightning's located in the partial eclipse area of Asia-Oceania region. The changes in D-region ionospheric VLF reflection height and electron density (similar to 22-23 cm(-3)) during eclipse have been estimated from the first cut-off frequency of the tweeks. The reflection height increased from similar to 89 km from the first occurrence of tweek to about 91-92 km at the totality and then decreased to similar to 87 km at the end of the eclipse, suggesting a change of about 5 km in the reflection height during eclipse. The reflection heights are lower by 2-3 km as compared to normal nighttime tweek reflection heights. The above increase in the reflection height indicate that the partial nighttime condition is created during eclipse, as the main D-region ionizing radiation Lyman alpha is blocked but solar soft X-ray and EUV radiations originating from the limb solar corona are not totally blocked which produce some of ionization in the D-region.
机译:提出了在2009年7月22日的日全食期间,在印度地区的低纬度站阿拉哈巴德和奈尼塔尔观测到的具有高次谐波的周(n> 1)。阿拉哈巴德站和奈尼塔尔站分别占总数的100%和85%。观察结果表明,大约30-40%的太阳圆盘遮盖可能导致tweek发生,否则仅在夜间发生。在安拉阿巴德(Allahabad)总共记录了148个星期,在奈尼塔尔(Nainital)记录了20个星期,其中一些记录达到了三次谐波。全球闪电定位网的数据表明,观测到的t周是由位于亚洲大洋洲部分月食区的闪电产生的。根据t周的第一个截止频率,估计了日食期间D区电离层VLF反射高度和电子密度(类似于22-23 cm(-3))的变化。反射高度从第一次出现以来的大约89 km增加到第t周的大约91-92 k​​m,然后在日食结束时减小到大约87 km,这表明反射高度大约变化了5 km在日食期间。与正常夜间tweek反射高度相比,反射高度降低了2-3 km。以上反射高度的增加表明,在日食时会产生部分夜间条件,因为主要的D区电离辐射莱曼α被阻挡,但源自肢体日冕的太阳软X射线和EUV辐射并未被完全阻挡,在D区域产生一些电离。

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