Observing the radiative properties of clear and cloudy skies in the far infrared, 14 -120µm, using the Tropospheric Airborne Fourier Transform Spectrometer (TAFTS)

2001 ◽  
Author(s):  
Jon. E. Murray ◽  
Antonio. A. Canas
Keyword(s):  
Fourier Transform ◽  
Far Infrared ◽  
Radiative Properties ◽  
Fourier Transform Spectrometer

Imaging Fourier transform spectrometer with photoconductive detector arrays: an application to the AKARI far-infrared instrument

2008 ◽  
Author(s):  
Mitsunobu Kawada ◽  
Hidenori Takahashi ◽  
Noriko Murakami ◽  
Yoko Okada ◽  
Akiko Yasuda ◽  
...  
Keyword(s):  
Fourier Transform ◽  
Far Infrared ◽  
Fourier Transform Spectrometer ◽  
Detector Arrays ◽  
Photoconductive Detector

Design of an efficient broadband far-infrared fourier-transform spectrometer

1999 ◽  
Vol 38 (18) ◽  
pp. 3945 ◽  
Author(s):  
Bruno Carli ◽  
Alessandra Barbis ◽  
John E. Harries ◽  
Luca Palchetti
Keyword(s):  
Fourier Transform ◽  
Far Infrared ◽  
Fourier Transform Spectrometer

Far-infrared high-resolution Fourier transform spectrometer

1987 ◽  
Vol 26 (18) ◽  
pp. 3818 ◽  
Author(s):  
Bruno Carli ◽  
Massimo Carlotti ◽  
Francesco Mencaraglia ◽  
Enzo Rossi
Keyword(s):  
Fourier Transform ◽  
High Resolution ◽  
Far Infrared ◽  
Fourier Transform Spectrometer

scholarly journals The Herschel SPIRE Fourier Transform Spectrometer Spectral Feature Finder − II. Estimating radial velocity of SPIRE spectral observation sources

2020 ◽  
Vol 496 (4) ◽  
pp. 4894-4905 ◽  
Author(s):  
Jeremy P Scott ◽  
Natalia Hładczuk ◽  
Locke D Spencer ◽  
Ivan Valtchanov ◽  
Chris Benson ◽  
...  
Keyword(s):  
Fourier Transform ◽  
Radial Velocity ◽  
Spectral Feature ◽  
Far Infrared ◽  
Spectral Observation ◽  
Spectral Features ◽  
Fourier Transform Spectrometer ◽  
Infrared Observations ◽  
Characteristic Lines

ABSTRACT The Herschel SPIRE FTS Spectral Feature Finder (FF) detects significant spectral features within SPIRE spectra and employs two routines, and external references, to estimate source radial velocity. The first routine is based on the identification of rotational 12CO emission, the second cross-correlates detected features with a line template containing most of the characteristic lines in typical far infrared observations. In this paper, we outline and validate these routines, summarize the results as they pertain to the FF, and comment on how external references were incorporated.

Far-infrared sensor for cirrus (FIRSC): an aircraft-based Fourier-transform spectrometer to measure cloud radiance: erratum

2001 ◽  
Vol 40 (22) ◽  
pp. 3710
Author(s):  
Michael D. Vanek ◽  
Ira G. Nolt ◽  
Nina D. Tappan ◽  
Peter A. R. Ade ◽  
Fred C. Gannaway ◽  
...  
Keyword(s):  
Fourier Transform ◽  
Far Infrared ◽  
Fourier Transform Spectrometer ◽  
Infrared Sensor

scholarly journals Technical note: First spectral measurement of the Earth's upwelling emission using an uncooled wideband Fourier transform spectrometer

2006 ◽  
Vol 6 (12) ◽  
pp. 5025-5030 ◽  
Author(s):  
L. Palchetti ◽  
C. Belotti ◽  
G. Bianchini ◽  
F. Castagnoli ◽  
B. Carli ◽  
...  
Keyword(s):  
Fourier Transform ◽  
Far Infrared ◽  
Space Mission ◽  
Technical Note ◽  
Spectral Measurement ◽  
Tropical Region ◽  
Fourier Transform Spectrometer ◽  
Field Campaign ◽  
Infrared Signature ◽  
Stratospheric Balloon

Abstract. The first spectral measurement of Earth's emitted radiation to space in the wideband range from 100 to 1400 cm−1 with 0.5 cm−1 spectral resolution is presented. The measurement was performed from a stratospheric balloon in tropical region using a Fourier transform spectrometer, during a field campaign held in Brazil in June 2005. The instrument, which has uncooled components including the detector module, is a prototype developed as part of the study for the REFIR (Radiation Explorer in the Far InfraRed) space mission. This paper shows the results of the field campaign with particular attention to the measurement capabilities of the prototype. The results are compared with measurements taken by IASI-balloon (Infrared Atmospheric Sounding Interferometer – Balloon version), aboard the same platform, and with forward model estimations. The infrared signature of clouds is observed in the measurements.

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