Rovibrational analysis of the ν71 intermolecular hydrogen bond bending vibration in HCN---HF using far infrared fourier transform spectroscopy

1988 ◽  
Vol 152 (4-5) ◽  
pp. 299-304 ◽  
Author(s):  
B.A. Wofford ◽  
R.S. Ram ◽  
A. Quinonez ◽  
J.W. Bevan ◽  
W.B. Olson ◽  
...  
Keyword(s):  
Hydrogen Bond ◽  
Fourier Transform ◽  
Intermolecular Hydrogen Bond ◽  
Far Infrared ◽  
Fourier Transform Spectroscopy ◽  
Bending Vibration ◽  
Bond Bending

Polarization-Sensitive Fourier-Transform Spectroscopy of HgTe/CdHgTe Quantum Wells in the Far Infrared Range in a Magnetic Field

JETP Letters ◽  
2018 ◽  
Vol 108 (5) ◽  
pp. 329-334 ◽  
Author(s):  
L. S. Bovkun ◽  
A. V. Ikonnikov ◽  
V. Ya. Aleshkin ◽  
S. S. Krishtopenko ◽  
N. N. Mikhailov ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Fourier Transform ◽  
Quantum Wells ◽  
Far Infrared ◽  
Fourier Transform Spectroscopy ◽  
Infrared Range

Fourier transform far-infrared spectroscopy of the hydrogen bond in 4-n-alkoxybenzoic acids

1995 ◽  
Vol 8 (2) ◽  
pp. 193-198 ◽  
Author(s):  
K. Antonova ◽  
M. Petrov ◽  
N. Kirov ◽  
T. Tenev ◽  
H. Ratajczak
Keyword(s):  
Hydrogen Bond ◽  
Fourier Transform ◽  
Infrared Spectroscopy ◽  
Far Infrared ◽  
Far Infrared Spectroscopy

scholarly journals Astronomical imaging Fourier spectroscopy at far-infrared wavelengths

2013 ◽  
Vol 91 (11) ◽  
pp. 870-878 ◽  
Author(s):  
David A. Naylor ◽  
Brad G. Gom ◽  
Matthijs H.D. van der Wiel ◽  
Gibion Makiwa
Keyword(s):  
Fourier Transform ◽  
Imaging Spectroscopy ◽  
Far Infrared ◽  
Fourier Transform Spectroscopy ◽  
Calibration Data ◽  
Fourier Spectroscopy ◽  
Astronomical Imaging ◽  
Infrared Wavelengths

The principles and practice of astronomical imaging Fourier transform spectroscopy (FTS) at far-infrared wavelengths are described. The Mach–Zehnder (MZ) interferometer design has been widely adopted for current and future imaging FTS instruments; we compare this design with two other common interferometer formats. Examples of three instruments based on the MZ design are presented. The techniques for retrieving astrophysical parameters from the measured spectra are discussed using calibration data obtained with the Herschel–SPIRE instrument. The paper concludes with an example of imaging spectroscopy obtained with the SPIRE FTS instrument.

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