Hanel R, Schlachman B, Breihan E, Bywaters R, Chapman F, Rhodes M, Rodgers D, Vanous D
Appl Opt. 1972 Nov 1;11(11):2625-34. doi: 10.1364/AO.11.002625.
The Michelson interferometer on Mariner 9 measures the thermal emission spectrum of Mars between 200 cm(-1) and 2000 cm(-1) (between 5 microm and 50 microm) with a spectral resolution of 2.4 cm(-1) in the apodized mode. A noise equivalent radiance of 0.5 x 10(-7) W cm(-2) sr(-1)/cm(-1) is deduced from data recorded in orbit around Mars. The Mariner interferometer deviates in design from the Nimbus 3 and 4 interferometers in several areas, notably, by a cesium iodide beam splitter and certain aspects of the digital information processing. Special attention has been given to the problem of external vibration. The instrument performance is demonstrated by calibration data and samples of Mars spectra.
“水手9号”上的迈克尔逊干涉仪在变迹模式下测量火星在200厘米⁻¹至2000厘米⁻¹(5微米至50微米)之间的热发射光谱,光谱分辨率为2.4厘米⁻¹。从环绕火星轨道记录的数据中推断出噪声等效辐射率为0.5×10⁻⁷瓦·厘米⁻²·球面度⁻¹/厘米⁻¹。“水手号”干涉仪在设计上与“雨云3号”和“雨云4号”干涉仪在几个方面有所不同,特别是采用了碘化铯分束器以及数字信息处理的某些方面。对外部振动问题给予了特别关注。仪器性能通过校准数据和火星光谱样本得以证明。