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A new altimeter for Mars land shape observations utilizing the ionospheric sounder system onboard the Planet-B spacecraft

机译:使用Planet-B航天器上的电离层测深仪系统的新型火星高度观测仪

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A new altimeter has been developed for the observation of the land shape of a planet from an orbiting spacecraft by transmitting RF pulses. The present system utilizes an RF sounder for observing the electron density profile of the topside ionosphere by selecting a transmission frequency f higher than the local cutoff frequency of the ionosphere by adding upper and lower side band modulations with a frequency p ; i.e. at frequencies f + p and f - p . The phase difference of the propagating signals at the upper and lower side band frequencies gives a fine delay time with a range resolution of 100m for p = 50 kHz and 20m for p = 250 kHz with f = 9 MHz corresponding to a resolution of 6° of the phase detector of the system onboard the spacecraft. Using 600 Watts transmitting power applied to a 52m tip-to-tip dipole antenna, the altitude of the spacecraft and the land shape can be measured while the spacecraft is in the range below 300km altitude at the planet.
机译:已经开发了一种新的高度计,用于通过发射RF脉冲从在轨的航天器观测行星的陆地形状。本系统利用射频测深仪,通过增加频率为p的上,下边带调制来选择比电离层的局部截止频率高的传输频率f,从而观察顶侧电离层的电子密度分布;即在频率f + p和f-p处。上,下边带频率上传播信号的相位差给出了一个精细的延迟时间,对于p = 50 kHz,其范围分辨率为100m;对于p = 250 kHz,其范围分辨率为20m,其中f = 9 MHz,其分辨率为6°航天器系统的相位检测器的示意图。使用施加在52m尖端对偶极天线上的600瓦发射功率,可以测量航天器的高度和陆地形状,而航天器的高度在300 km以下。

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