首页> 外文会议>Propagation Engineering: Fourth in a Series >High-resolution astronomical observations using deconvolution from wavefront sensing
【24h】

High-resolution astronomical observations using deconvolution from wavefront sensing

机译:使用波前感测反卷积的高分辨率天文观测

获取原文
获取原文并翻译 | 示例

摘要

Abstract: Deconvolution from wavefront sensing is a new technique of high-resolution imaging through atmospheric turbulence developed at ONERA. The capabilities of the method have been demonstrated during first laboratory experiments. A deconvolution experimental set-up was installed on the 4.2 m William Herschel telescope on La Palma in November 1990. The results obtained during these observations are presented: the astronomical sources were observed at optical wavelengths; the resolution improvement reached a factor greater than 10.!
机译:摘要:波前传感的反卷积是一种由ONERA开发的通过大气湍流进行高分辨率成像的新技术。该方法的功能已在首次实验室实验中得到证明。 1990年11月在拉帕尔玛岛的4.2 m威廉·赫歇尔望远镜上安装了反卷积实验装置。这些观测结果表明:在光学波长下观测了天文观测源;分辨率提高到10倍以上!

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号