A compact, high resolution Michelson interferometer for atmospheric spectroscopy in the near ultraviolet

1993 ◽  
Author(s):  
Stanley P. Sander ◽  
Richard P. Cageao ◽  
Randy R. Friedl
Keyword(s):  
High Resolution ◽  
Michelson Interferometer ◽  
Near Ultraviolet ◽  
Atmospheric Spectroscopy

Atmospheric spectroscopy at very high resolution in the middle infrared with a rapid-scan Michelson interferometer

1976 ◽  
Vol 16 (1-2) ◽  
pp. 329 ◽  
Author(s):  
M. Anderegg ◽  
J.E. Beckman ◽  
A.F.M. Moorwood ◽  
J.P. Baluteau ◽  
E. Bussoletti ◽  
...  
Keyword(s):  
High Resolution ◽  
Michelson Interferometer ◽  
Rapid Scan ◽  
Atmospheric Spectroscopy ◽  
Middle Infrared ◽  
Very High

Coherent Control of Semiconductor Quantum Wire by High-Resolution and Stable Michelson Interferometer

2008 ◽  
Vol 128 (6) ◽  
pp. 285-291
Author(s):  
Takumi Okada ◽  
Kazuhiro Komori ◽  
Xue-Lun Wang ◽  
Mutsuo Ogura ◽  
Noriaki Tsurumachi
Keyword(s):  
High Resolution ◽  
Quantum Wire ◽  
Coherent Control ◽  
Michelson Interferometer

scholarly journals A non-iterative linear retrieval for infrared high-resolution limb sounders

2013 ◽  
Vol 6 (5) ◽  
pp. 1381-1396
Author(s):  
L. Millán ◽  
A. Dudhia
Keyword(s):  
High Resolution ◽  
Computing Time ◽  
Michelson Interferometer ◽  
High Spectral Resolution ◽  
Radiative Transfer Model ◽  
Spectral Signature ◽  
Transfer Model ◽  
Concentration Difference ◽  
Error Margin ◽  
Retrieval Scheme

Abstract. Currently, most of the high-spectral-resolution infrared limb sounders use subsets of the recorded spectra (microwindows) in their retrieval schemes to reduce the computing time of rerunning the radiative transfer model. A fast linear retrieval scheme is described which allows the whole spectral signature of the target molecule to be used. We determine that pressure and temperature retrievals can be treated linearly up to a 20% difference between the atmospheric state and the linearisation point for a 3% error margin and up to 10 K "difference" for a 3 K error margin near the stratopause and less than 0.5 K elsewhere. Assuming perfect pT knowledge, CH4 retrievals can be be treated linearly up to a 20% CH4 concentration "difference" for a 2% error margin. As an example, this technique is implemented for the Michelson Interferometer for Passive Atmospheric Sounding instrument, but it is applicable to any high-resolution limb sounder.

High resolution Michelson interferometer for airborne infrared astronomical observations 1: Concept and performance

1977 ◽  
Vol 16 (7) ◽  
pp. 1834 ◽  
Author(s):  
J. P. Baluteau ◽  
M. Anderegg ◽  
A. F. M. Moorwood ◽  
N. Coron ◽  
J. E. Beckman ◽  
...  
Keyword(s):  
High Resolution ◽  
Michelson Interferometer ◽  
Astronomical Observations ◽  
And Performance

scholarly journals Michelson Interferometer for Global High-Resolution Thermospheric Imaging (MIGHTI): Monolithic Interferometer Design and Test

2017 ◽  
Vol 212 (1-2) ◽  
pp. 601-613 ◽  
Author(s):  
John M. Harlander ◽  
Christoph R. Englert ◽  
Charles M. Brown ◽  
Kenneth D. Marr ◽  
Ian J. Miller ◽  
...  
Keyword(s):  
High Resolution ◽  
Michelson Interferometer

scholarly journals Analysis of new species retrieved from MIPAS

2014 ◽  
Vol 56 ◽  
Author(s):  
Shaomin Cai ◽  
Anu Dudhia
Keyword(s):  
Fourier Transform ◽  
New Species ◽  
High Resolution ◽  
Trace Gases ◽  
Michelson Interferometer ◽  
Emission Spectra ◽  
Fourier Transform Spectrometer ◽  
Mid Infrared ◽  
The Third ◽  
Atmospheric Sounding

The Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) instrument which operated on the Envisat satellite from 2002-2012 is a Fourier transform spectrometer for the measurement of high-resolution gaseous emission spectra at the Earth's limb. It operates in the near- to mid-infrared, where many of the main atmospheric trace gases have important emission features. The initial operational products were profiles of Temperature, H2O, O3, CH4, N2O, HNO3, and NO2, and this list was recently extended to include N2O5, ClONO2, CFC-11 and CFC-12. Here we present preliminary results of retrievals of the third set of species under consideration for inclusion in the operational processor: HCN, CF4, HCFC-22, COF2 and CCl4.

scholarly journals New Infrared Spectra of the Jovian Planets: Study of Jupiter and Saturn in the 3v3 Methane Band by Fourier Transform Spectroscopy

1974 ◽  
Vol 65 ◽  
pp. 357-358
Author(s):  
C. De Bergh ◽  
M. Combes ◽  
Th. Encrenaz ◽  
J. Lecacheux ◽  
M. Vion ◽  
...  
Keyword(s):  
Fourier Transform ◽  
High Resolution ◽  
Infrared Spectra ◽  
Rotational Temperature ◽  
Michelson Interferometer ◽  
Fourier Transform Spectroscopy ◽  
Half Width ◽  
Layer Model ◽  
Jovian Planets

High resolution spectra of Jupiter and Saturn were obtained with a Fourier Transform Michelson interferometer. A comparison of the observed spectra, after elimination of the solar and terrestrial contributions to absorption, with synthetic profiles for the reflecting layer model has permitted new determinations of the Lorentz half-width, the methane abundance, the rotational temperature and the pressure at the level of formation of the methane lines for both Jupiter and Saturn.

High resolution Michelson interferometer for airborne infrared astronomical observations 2: System design

1977 ◽  
Vol 16 (7) ◽  
pp. 1841 ◽  
Author(s):  
A. Langlet ◽  
C. Delage ◽  
D. Stefanovitch ◽  
B. Talureau ◽  
J. Tualy ◽  
...  
Keyword(s):  
High Resolution ◽  
System Design ◽  
Michelson Interferometer ◽  
Astronomical Observations

Sub‐Doppler high‐resolution spectroscopy and the Zeeman effect of CS2 in the near ultraviolet

1994 ◽  
Vol 100 (5) ◽  
pp. 3394-3406 ◽  
Author(s):  
Kiyoshi Nishizawa ◽  
Shunji Kubo ◽  
Atsushi Doi ◽  
Hajime Katô
Keyword(s):  
High Resolution ◽  
Zeeman Effect ◽  
High Resolution Spectroscopy ◽  
Near Ultraviolet
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