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Wave-Like Variations and Sudden Density Decreases in the Lower Thermosphere as Measured by the San Marco V Satellite

机译:如圣马可五世卫星所测量的那样,在较低的热圈中,类似波的变化和突然的密度降低

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Neutral density measurements were carried out by the microaccelerometer on board the Italian San Marco V satellite in 1988. During the final week of its existence the satellite's perigee decreased to as low as 130 km. Measured density values were compared to the corresponding CIRA '86 (MSIS '86) or to our dMSIS model values. The residuals reveal a wavy structure of different time scales. Characterising the wave amplitude by the average deviation of the residuals, its dependence on different parameters was studied. These investigations demonstrated that the wave-amplitude varies with height, local solar time and geomagnetic disturbance level. There is a particularly developed wave pattern in the average deviations below 200 km. Case studies indicates that there are sudden density decreases of 20-30 sec duration that might be in connection with plasma bubble crossings by the satellite. Altogether 261 such cases were identified and their distribution as a function of height, LST and longitude have been investigated.
机译:1988年,意大利圣马可V卫星上的微加速度计对中性密度进行了测量。在卫星的存在的最后一周,卫星的近地点降到了130公里。将测得的密度值与相应的CIRA '86(MSIS '86)或与我们的dMSIS模型值进行比较。残差显示出不同时间尺度的波浪结构。通过残差的平均偏差表征波幅,研究了波幅对不同参数的依赖性。这些研究表明,波幅随高度,当地太阳时间和地磁干扰水平而变化。在200 km以下的平均偏差中,有一个特别发达的波形。案例研究表明,密度突然降低了20-30秒,这可能与卫星穿越等离子体气泡有关。总共确定了261个此类案例,并研究了它们作为高度,LST和经度的函数的分布。

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