Crockett W R, Patterson N P, Purcell J D, Schumacher R J, Tousey R
Appl Opt. 1977 Apr 1;16(4):893-7. doi: 10.1364/AO.16.000893.
An instrument for recording extreme ultraviolet television images of the sun was flown in the Apollo Telescope Mount on Skylab. Solar radiation in the 171-630 A wavelength range, defined by the transmission band of three thin-film aluminum filters, was focused onto a p-quaterphenyl photon conversion layer by a platinum-coated mirror at normal incidence. The conversion layer was attached to the faceplate of a low light level SEC vidicon. An onboard video monitor enabled the Skylab crews to observe the images in realtime and to identify and follow the development of solar features. Images were also transmitted to the mission control center, where they were used in planning the ATM observing schedule.
一台用于记录太阳极紫外电视图像的仪器搭载在天空实验室的阿波罗望远镜支架上。由三个薄膜铝滤光片的透射带所定义的171 - 630埃波长范围内的太阳辐射，通过一个镀铂镜面以垂直入射的方式聚焦到一个对四联苯光子转换层上。该转换层附着在一个低光照水平的SEC视像管的面板上。一个机载视频监视器使天空实验室的宇航员能够实时观测图像，并识别和跟踪太阳特征的发展。图像也被传输到任务控制中心，在那里它们被用于规划阿波罗望远镜支架的观测计划。
