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Remote operation of the CHARA array via the Internet.

机译:通过Internet进行CHARA阵列的远程操作。

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摘要

Georgia State University's Center for High Angular Resolution Astronomy (CHARA) Array is located atop California's Mount Wilson in the San Gabriel Mountains northeast of Los Angeles. Approximately 2000 miles due west of the university's central campus, located in Atlanta Georgia, travel time to/from the array is generally several hours by air and ground for those individuals visiting the array who do not live in southern California. In Internet time, however, the array is a mere 60 milliseconds (ms) distance from Atlanta!; A remote operations system allowing multiple individuals to participate in remote observation sessions was designed and implemented. Several technological considerations were incorporated into the overall design including a secure network infrastructure with acceptable end-to-end latency, a control room replete with appropriate computing and projection systems, an efficient client-server model, and a data archival system.; The remote operations system was initially used to begin a prototypical survey of extra-solar planetary systems, establish operational procedures, and define performance expectations. The observations, comprised of the target/calibrator star pairs 51 Peg/HD 218792 and &egr; Eri/HD 21530, involved the sampling of several baseline-visibility data points collected over the course of several hours per evening per star. The downloaded scientific data were reduced and analyzed thus yielding the results contained herein.; Although independent of the local weather, remote operations have practical considerations such as routine preparations requiring on-site personnel and observation of astronomical targets with celestial coordinates appropriate to the Local Sidereal Time (LST) and U-V plane coverage of the array. Such considerations are necessary in order to obtain desired scientific data. This present work details all of the aforementioned topics that were required to produce the first-generation of the remote operations system.
机译:佐治亚州立大学的高角分辨率天文中心(CHARA)阵列位于洛杉矶东北部圣加布里埃尔山的加利福尼亚州威尔逊山顶上。该大学位于位于佐治亚州亚特兰大市中央校园以西约2000英里处,往返阵列的旅行时间通常为空运和地面飞行几个小时,对于那些不住在加利福尼亚南部的人来说,乘飞机到阵列的时间为数小时。但是,在互联网时代,该阵列与亚特兰大的距离只有60毫秒(ms)!设计并实现了一个远程操作系统,允许多个人参加远程观察会议。总体设计中考虑了多种技术因素,包括具有可接受的端到端等待时间的安全网络基础架构,配备适当的计算和投影系统的控制室,高效的客户端-服务器模型以及数据归档系统。远程操作系统最初用于对太阳系外行星系统进行原型调查,建立操作程序并定义性能期望。由目标/定标星对51 Peg / HD 218792和&egr;组成的观测值。 Eri / HD 21530,涉及从每颗恒星每晚几个小时的过程中收集的几个基线可见性数据点的采样。减少并分析了下载的科学数据,从而得出此处包含的结果。尽管不受当地天气影响,但远程操作具有实际考虑因素,例如需要现场工作人员进行例行准备工作以及观察天体目标并使其天体坐标适合于阵列的本地实时(LST)和U-V平面。为了获得所需的科学数据,必须考虑这些因素。本工作详细介绍了产生第一代远程操作系统所需的所有上述主题。

著录项

  • 作者

    Fallon, Thomas John.;

  • 作者单位

    Georgia State University.;

  • 授予单位 Georgia State University.;
  • 学科 Physics Astronomy and Astrophysics.; Computer Science.
  • 学位 Ph.D.
  • 年度 2003
  • 页码 248 p.
  • 总页数 248
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;自动化技术、计算机技术;
  • 关键词

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