论文标题

低质量星际探测通信中的技术挑战

Technological Challenges in Low-mass Interstellar Probe Communication

论文作者

Messerschmitt, David, Lubin, Philip, Morrison, Ian

论文摘要

基于从一群低质量的星际探针中的下行链路的初步纸张设计,用于从Proxima Centauri附近返回科学数据,总结了最关键的技术问题,其意义在整体系统设计的背景下解释了。主要目标是确定主要的挑战或展示策划者,如果要使用当前可用的现成技术来构建此类下行链路,从而为未来对组成设计挑战和技术的研究提供了方向和动力。尽管没有任何基本的物理限制可以防止这种通信系统,但目前可用的技术在几个领域都显着矮小,并且有不确定的解决方案还有其他主要的设计挑战。最大的确定挑战是质量限制,从多个探针到相同的目标系外行星,态度控制和指向准确性以及多普勒的多样性交流以及由于探针速度的不确定性而导致多普勒的转移。最大的技术挑战是电力,高功率和波长 - 敏捷的光源,光学带通滤波器的非常有选择性和波长 - 敏捷库,以及具有极低深度计数率的单光子检测器。对于其中的关键子集,我们描述了我们遇到的困难的性质及其在整个系统环境中的起源。还考虑了将接收到单个探针限制的接收器与群体相比。

Building on a preliminary paper design of a downlink from a swarm of low-mass interstellar probes for returning scientific data from the vicinity of Proxima Centauri, the most critical technology issues are summarized, and their significance is explained in the context of the overall system design. The primary goal is to identify major challenges or showstoppers if such a downlink were to be constructed using currently available off-the-shelf technology, and thereby provide direction and motivation to future research on the constituent design challenges and technologies. While there are not any fundamental physical limits that prevent such communication systems, currently available technologies fall significantly short in several areas and there are other major design challenges with uncertain solutions. The greatest identified challenges are in mass constraints, multiplexing simultaneous communication from multiple probes to the same target exoplanet, attitude control and pointing accuracy, and Doppler shifts due to uncertainty in probe velocity. The greatest technology challenges are electrical power, high power and wavelength-agile optical sources, very selective and wavelength-agile banks of optical bandpass filters, and single-photon detectors with extremely low dark-count rates. For a critical subset of these, we describe the nature of the difficulties we encounter and their origins in the overall system context. A receiver that limits reception to a single probe is also considered and compared to the swarm case.

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