来自威尔逊山100英寸望远镜的卡塞格林自适应光学系统的结果

Adaptive Optics Pub Date : 1900-01-01 DOI:10.1364/adop.1996.amb.13

J. Shelton, T. G. Schneider, D. McKenna, S. Baliunas

{"title":"来自威尔逊山100英寸望远镜的卡塞格林自适应光学系统的结果","authors":"J. Shelton, T. G. Schneider, D. McKenna, S. Baliunas","doi":"10.1364/adop.1996.amb.13","DOIUrl":null,"url":null,"abstract":"Since June of 1994 we have been operating and improving a natural-guide-star adaptive optics system on the Mount Wilson 100-inch telescope.1,3 The system is routinely operated by one person plus a telescope operator. First astronomical observations have achieved image profiles with a full-width-at-half-max (FWHM) of 0.068 arcsec, using a silicon CCD with no wavelength discrimination (Fig. 1).","PeriodicalId":256393,"journal":{"name":"Adaptive Optics","volume":"30 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"Results from the Cassegrain adaptive optics system of the Mount Wilson 100-inch telescope\",\"authors\":\"J. Shelton, T. G. Schneider, D. McKenna, S. Baliunas\",\"doi\":\"10.1364/adop.1996.amb.13\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Since June of 1994 we have been operating and improving a natural-guide-star adaptive optics system on the Mount Wilson 100-inch telescope.1,3 The system is routinely operated by one person plus a telescope operator. First astronomical observations have achieved image profiles with a full-width-at-half-max (FWHM) of 0.068 arcsec, using a silicon CCD with no wavelength discrimination (Fig. 1).\",\"PeriodicalId\":256393,\"journal\":{\"name\":\"Adaptive Optics\",\"volume\":\"30 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Adaptive Optics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1364/adop.1996.amb.13\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Adaptive Optics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/adop.1996.amb.13","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}

引用次数: 3

摘要

自1994年6月以来，我们一直在操作和改进威尔逊山100英寸望远镜上的自然导星自适应光学系统。这个系统通常由一个人加上一个望远镜操作员来操作。首次天文观测使用无波长分辨的硅CCD获得了0.068弧秒的全宽半最大(FWHM)的图像轮廓(图1)。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

查看原文本刊更多论文

Results from the Cassegrain adaptive optics system of the Mount Wilson 100-inch telescope

Since June of 1994 we have been operating and improving a natural-guide-star adaptive optics system on the Mount Wilson 100-inch telescope.1,3 The system is routinely operated by one person plus a telescope operator. First astronomical observations have achieved image profiles with a full-width-at-half-max (FWHM) of 0.068 arcsec, using a silicon CCD with no wavelength discrimination (Fig. 1).

求助全文

通过发布文献求助，成功后即可免费获取论文全文。去求助

来源期刊

Adaptive Optics

自引率

0.00%

发文量