This paper describes the electric and electronic apparatus of balloon borne telescope for far infrared observation of the sun.
本文介绍了一个用于观测太阳远红外辐射的球载望远镜电气设备。
The bright spot at the top right of the image is an active star-forming region called W3, which Wright studied with a 4-pixel balloon-borne telescope for his Ph.D. thesis in the 1970s.
在图像的右上角的亮点是一个名为w3的活跃的恒星形成区域，是由Wright在20世纪70年代在写研究4像素气球传播望远镜的博士论文期间发现并命名的。
It's a space-borne telescope that will be able to measure the tiniest dimming (caused by a planet crossing in front of the host star), to one part in 100,000, allowing us to detect Earth-like planets.
这是一个太空望远镜，能够观察由行星在主星(恒星)前横移造成的最微弱的亮度变化。如果允许我们探测类似地球的行星，那么需要达到该亮度变化的十万分之一。
This paper introduces the state-space model of the detecting platform of the balloon-borne hard X-ray astronomical telescope HAPI-4 system. and its LQR designing method.
本文介绍了球载硬x射线空间高能天文望远镜HAPI - 4系统探测器平台即吊舱系统的状态空间模型。
This paper introduces the state-space model of the detecting platform of the balloon-borne hard X-ray astronomical telescope HAPI-4 system. and its LQR designing method.
本文介绍了球载硬x射线空间高能天文望远镜HAPI - 4系统探测器平台即吊舱系统的状态空间模型。
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