校准
迈克尔逊干涉仪
天文干涉仪
光学
遥感
干涉测量
卫星
物理
地质学
天文
量子力学
作者
Kenneth D. Marr,William H. Morrow,C. M. Brown,Christoph Englert,John M. Harlander,Angel Cerrato,Kelvin Lamport,S. Harris
出处
期刊:Optical Engineering
[SPIE - International Society for Optical Engineering]
日期:2019-05-31
卷期号:58 (05): 1-1
被引量:5
标识
DOI:10.1117/1.oe.58.5.054104
摘要
We describe the design and ground-based performance of the two-color calibration lamp for the Michelson Interferometer for Global High-Resolution Thermospheric Imaging (MIGHTI) instrument on the NASA Ionospheric Connection (ICON) satellite. The calibration lamp assembly contains radio frequency excited krypton and neon lamps, which generate emission lines at 557 and 630 nm, respectively, and which are used to monitor thermal drifts in the two MIGHTI Doppler asymmetric spatial heterodyne interferometers. The lamps are coupled to two mixed optical fiber bundles that deliver the calibration signals to the two MIGHTI optical units. The assembly starts reliably, consumes <8 W, and has passed environmental testing for the ICON satellite. The total mass of the lamp assembly is 1.8 kg. Special features of the assembly and its implementation are described along with results of life tests.
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