注册 登录
EN | CN
  • 首页
  • 论文提交
  • 论文浏览
  • 论文检索
  • 个人中心
  • 帮助
按提交时间
  • 2
按主题分类
  • 2
按作者
  • 2
  • 2
  • 2
  • 2
  • 2
  • 2
  • 2
按机构
当前资源共 2条
隐藏摘要 点击量 时间 下载量
  • 1. ChinaXiv:202303.07976
    下载全文

    Astrometric Reduction of Saturnian Satellites with Cassini-ISS Images Degraded by Trailed Stars

    分类: 天文学 >> 天文学 提交时间: 2023-02-19

    Qing-Feng Zhang Meng-Qi Liu Yan Li Lin-Peng Wu Zhi-Qiang Wang Li-Sha Zhu Zhan Li

    摘要: Imaging Science Subsystem (ISS) mounted on the Cassini spacecraft has taken a lot of images, which provides an important source of high-precision astrometry of some planets and satellites. However, some of these images are degraded by trailed stars. Previously, these degraded images cannot be used for astrometry. In this paper, a new method is proposed to detect and compute the centers of these trailed stars automatically. The method is then performed on the astrometry of ISS images with trailed stars. Finally, we provided 658 astrometric positions between 2004 and 2017 of several satellites that include Enceladus, Dione, Tethys, Mimas and Rhea. Compared with the JPL ephemeris SAT427, the mean residuals of these measurements are 0.11 km and 0.26 km in right ascension and declination, respectively. Their standard deviations are 1.08 km and 1.37 km, respectively. The results show that the proposed method performs astrometric measurements of Cassini ISS images with trailed stars effectively.

    同行评议状态:待评议

     点击量 34  下载量 16  评论 0
  • 2. ChinaXiv:202303.04656
    下载全文

    Astrometric Reduction of Saturnian Satellites with Cassini-ISS Images Degraded by Trailed Stars

    分类: 天文学 >> 天文学 提交时间: 2023-02-19

    Qing-Feng Zhang Meng-Qi Liu Yan Li Lin-Peng Wu Zhi-Qiang Wang Li-Sha Zhu Zhan Li

    摘要: Imaging Science Subsystem (ISS) mounted on the Cassini spacecraft has taken a lot of images, which provides an important source of high-precision astrometry of some planets and satellites. However, some of these images are degraded by trailed stars. Previously, these degraded images cannot be used for astrometry. In this paper, a new method is proposed to detect and compute the centers of these trailed stars automatically. The method is then performed on the astrometry of ISS images with trailed stars. Finally, we provided 658 astrometric positions between 2004 and 2017 of several satellites that include Enceladus, Dione, Tethys, Mimas and Rhea. Compared with the JPL ephemeris SAT427, the mean residuals of these measurements are 0.11 km and 0.26 km in right ascension and declination, respectively. Their standard deviations are 1.08 km and 1.37 km, respectively. The results show that the proposed method performs astrometric measurements of Cassini ISS images with trailed stars effectively.

    同行评议状态:待评议

     点击量 28  下载量 13  评论 0
友情链接 : PubScholar 哲学社会科学预印本
  • 运营单位: 中国科学院文献情报中心
  • 制作维护:中国科学院文献情报中心知识系统部
  • 邮箱: eprint@mail.las.ac.cn
  • 地址:北京中关村北四环西路33号
招募预印本评审专家 许可声明 法律声明

京ICP备05002861号-25 | 京公网安备110402500046号
版权所有© 2016 中国科学院文献情报中心