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CONTROL METHOD removing space vehicles into orbit a planet artificial satellite

机译:控制方法将航天器移入人造卫星轨道

摘要

Method for controlling breeding of spacecraft into orbit planet artificial satellite, comprising a spacecraft approaching a predetermined entrance passage into the atmosphere, particularly in the i-th, where i = 1, 2, ..., N, times the motion parameters of the spacecraft, namely : its speed - V, the tilt angle of the speed vector of the spacecraft to the local horizon for the trajectory of its motion - θ, the radius - vector - r, atmospheric density - ρ, wherein the determination of spacecraft motion parameters is carried out on site in motion weatherp e planet providing entry of the spacecraft into the atmosphere with the value γ roll angle about 0 rad, and the value of the angle of incidence of the spacecraft about α, corresponding to the maximum value of aerodynamic control of the spacecraft, the control amount of the spacecraft γ roll angle to departure from the atmosphere, in determining the velocity spacecraft apocenter transition elliptical orbits - vulgaris implementation supply characteristic velocity accelerating pulse - ΔV in elliptical transition apocenter the orbit of the spacecraft to form the orbit with the given parameters, characterized in that the i-th, where i = K, K + 1, ..., R + M time points on a plot of the aerodynamic deceleration predicted at the time of the spacecraft from the atmosphere of the planet values ​​of the velocity of the spacecraft - vulgaris angle velocity vector to the local horizon for spacecraft trajectory - θpri motion of the spacecraft on the remaining parts of the flight in the atmosphere of the planet respectively with the magnitude of spacecraft roll angle γ equal
机译:用于控制航天器向轨道行星人造卫星的繁殖的方法,包括:航天器接近预定进入大气的通道,特别是在第i次,其中i = 1、2,...,N乘以其运动参数。航天器,即:其速度-V,航天器速度矢量相对于其运动轨迹的局部水平线的倾斜角-θ,半径-向量-r,大气密度-ρ,其中确定航天器运动参数是在运动天气行星的现场进行的,它使航天器以大约0 rad的γ侧倾角进入太空,并且航天器的入射角约为α,相当于空气动力学的最大值。航天器的控制,航天器的控制量γ侧倾角要偏离大气层,确定航天器的速度,重心过渡椭圆轨道-寻常型实现补充y椭圆过渡中的特征速度加速脉冲-ΔV偏离航天器的轨道以形成具有给定参数的轨道,其特征在于第i个,其中i = K,K + 1,...,R + M时间从行星大气的航天器速度值-寻常角速度矢量到航天器轨迹的局部视界-航天器上的θpri运动在航天器上预测的空气减速曲线上的点。行星大气中飞行的其余部分分别与航天器侧倾角γ相等

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