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Geophysical Effects of the March 29,2006, Solar Eclipse

机译:2006年3月29日日食的地球物理效应

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This paper presents results of comprehensive infra-sonic, radiophysical, and electromagnetic measurements during the March 29, 2006, solar eclipse. Investigations were carried out in the territory of the Mikh-nevo geophysical observatory (Institute of Geosphere Dynamics, Russian Academy of Sciences) located 80 km away from Moscow in the Serpukhov area of the Moscow region. We obtained the following results: (ⅰ) excitation of acoustic-gravitational waves at a frequency close to the Brent-Vasala frequency (1.7 · 10~(-3) Hz) was recorded in the atmosphere during the maximum phase of the solar eclipse; (ⅱ) variations were recorded in the total ionospheric electron content (TEC); (ⅲ) variations in the geomagnetic field, magnetic declination, and inclination were recorded during the maximum phase of the eclipse.
机译:本文介绍了在2006年3月29日日食期间进行的全面的超声波,放射性物理和电磁测量的结果。在距离莫斯科地区Serpukhov地区距离莫斯科80公里的Mikh-nevo地球物理观测站(俄罗斯科学院地球动力学研究所)的领土内进行了调查。我们获得了以下结果:(ⅰ)在日食最大相位期间,在大气中记录了接近Brent-Vasala频率(1.7·10〜(-3)Hz)的声引力波的激发; (ⅱ)记录了总电离层电子含量(TEC)的变化; (ⅲ)在月食最大期间记录了地磁场,磁偏角和倾角的变化。

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