Alignment and cryogenic testing of the Cassini Composite InfraRed Spectrometer (CIRS) far-infrared (FIR) focal plane

Author(s):  
Julie A. Crooke ◽  
John G. Hagopian
2011 ◽  
Vol E94-B (11) ◽  
pp. 2952-2960 ◽  
Author(s):  
Hirohisa NAGATA ◽  
Takehiko WADA ◽  
Hirokazu IKEDA ◽  
Yasuo ARAI ◽  
Morifumi OHNO ◽  
...  

1992 ◽  
Vol 63 (6) ◽  
pp. 3293-3297 ◽  
Author(s):  
W. Knap ◽  
D. Dur ◽  
A. Raymond ◽  
C. Meny ◽  
J. Leotin ◽  
...  

1988 ◽  
Vol 42 (2) ◽  
pp. 289-292 ◽  
Author(s):  
J. C. Donini ◽  
K. H. Michaelian

Research-quality far-infrared photoacoustic (PA) spectra are obtainable with a Fourier transform infrared spectrometer, the only changes with respect to conventional mid-infrared PA spectroscopy being the use of (1) a caesium iodide or polyethylene window on the PA cell, and (2) a mylar beamsplitter. Far-infrared PA spectra of several solids (bentonite, Fe+3-bentonite, and asbestos), in addition to the PA reference carbon black, have been recorded in this way. In order to improve signal-to-noise ratios in one of the spectra, we recorded ten interferograms under identical conditions; it was found that the average of the ten individually calculated spectra displays less noise and fewer spurious features than the spectrum obtained by first averaging the interferograms and then calculating a single spectrum. The results of this investigation demonstrate the feasibility of far-infrared PA spectroscopy, and illustrate that both experimental and computational procedures should be optimized in order to obtain the most satisfactory spectra.


Author(s):  
David Arrazola ◽  
Marianela Fernández ◽  
Luis Miguel González Fernández ◽  
Tomás Belenguer ◽  
Josefina Torres ◽  
...  

1987 ◽  
Vol 115 ◽  
pp. 371-371
Author(s):  
Paul M. Harvey ◽  
Daniel F. Lester ◽  
Marshall Joy

New mapping and analysis techniques for NASA's Kuiper Airborne Observatory are described which permit us to obtain information of size scales of order 10″ in the far-infrared. Basically, the focal-plane image is highly oversampled while the telescope is scanned smoothly and repeatedly over the region of interest with a slit of size λ/D. Maximum-entropy deconvolution is then used to obtain spectral frequency information down to scales of ∼ λ/2D.


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