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Planning and Scheduling of Payloads of AstroSat During Initial and Normal Phase Observations

机译:初始和正常相位观察期间雾度的有效载荷规划和调度

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On 28th September 2015, India launched its first astronomical space observatory AstroSat, successfully. AstroSat carried five astronomy payloads, namely, (i) Cadmium Zinc Telluride Imager (CZTI), (ii) Large Area X-ray Proportional Counter (LAXPC), (iii) Soft X-ray Telescope (SXT), (iv) Ultra Violet Imaging Telescope (UVIT) and (v) Scanning Sky Monitor (SSM) and therefore, has the capability to observe celestial objects in multi-wavelength. Four of the payloads are co-aligned along the positive roll axis of the spacecraft and the remaining one is placed along the positive yaw axis direction. All the payloads are sensitive to bright objects and specifically, require avoiding bright Sun within a safe zone of their bore axes in orbit. Further, there are other operational constraints both from spacecraft side and payloads side which are to be strictly enforced during operations. Even on-orbit spacecraft manoeuvres are constrained to about two of the axes in order to avoid bright Sun within this safe zone and a special constrained manoeuvre is exercised during manoeuvres. The planning and scheduling of the payloads during the Performance Verification (PV) phase was carried out in semi-autonomous/manual mode and a complete automation is exercised for normal phase/Guaranteed Time Observation (GuTO) operations. The process is found to be labour intensive and several operational software tools, encompassing spacecraft sub-systems, on-orbit, domain and environmental constraints, were built-in and interacted with the scheduling tool for appropriate decision-making and science scheduling. The procedural details of the complex scheduling of a multi-wavelength astronomy space observatory and their working in PV phase and in normal/GuTO phases are presented in this paper.
机译:2015年9月28日,印度成功地推出了第一个天文空间天文台雾度。 astosat载有五个天文有效载荷,即(i)镉碲化物成像仪(Czti),(ii)大面积X射线比例计数器(LAXPC),(III)软X射线望远镜(SXT),(IV)超紫成像望远镜(UVIT)和(V)扫描天空监视器(SSM),因此具有遵守多波长的天体的能力。四个有效载荷沿着航天器的正辊轴共对,并且其余的沿着正横摆轴方向放置。所有有效载荷对明亮物体敏感,具体地,要求避免在轨道上的孔轴的安全区域内避免明亮的太阳。此外,来自航天器侧和有效载荷侧的其他操作约束,在操作期间将被严格强制执行。即使是轨道的航天器机动也受到约束的约两个轴,以避免在这种安全区域内的明亮太阳,并且在演习期间锻炼特殊的约束机动。在性能验证(PV)阶段的有效载荷的规划和调度是在半自动/手动模式下进行的,并且对正常相/保证时间观察(Guto)操作进行完整的自动化。该过程被发现是劳动密集型和若干操作软件工具,包括航天器子系统,轨道,域和环境约束,内置并与适当的决策和科学调度的调度工具进行互动。本文介绍了多波长天文空间观测站的复杂调度的程序细节及其在PV相和正常/古托阶段。

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