Imaging Spectrometer Concepts For Next-Generation Planetary Missions

1984 ◽  
Author(s):  
M. Herring ◽  
D. W. Juergens ◽  
P. N. Kupferman ◽  
G. Vane
2019 ◽  
Vol 11 (18) ◽  
pp. 2129 ◽  
Author(s):  
John W. Chapman ◽  
David R. Thompson ◽  
Mark C. Helmlinger ◽  
Brian D. Bue ◽  
Robert O. Green ◽  
...  

We describe advanced spectral and radiometric calibration techniques developed for NASA’s Next Generation Airborne Visible Infrared Imaging Spectrometer (AVIRIS-NG). By employing both statistically rigorous analysis and utilizing in situ data to inform calibration procedures and parameter estimation, we can dramatically reduce undesirable artifacts and minimize uncertainties of calibration parameters notoriously difficult to characterize in the laboratory. We describe a novel approach for destriping imaging spectrometer data through minimizing a Markov Random Field model. We then detail statistical methodology for bad pixel correction of the instrument, followed by the laboratory and field protocols involved in the corrections and evaluate their effectiveness on historical data. Finally, we review the geometric processing procedure used in production of the radiometrically calibrated image data.


2019 ◽  
Vol 11 (24) ◽  
pp. 3054 ◽  
Author(s):  
Alana K. Ayasse ◽  
Philip E. Dennison ◽  
Markus Foote ◽  
Andrew K. Thorpe ◽  
Sarang Joshi ◽  
...  

This study evaluates a new generation of satellite imaging spectrometers to measure point source methane emissions from anthropogenic sources. We used the Airborne Visible and Infrared Imaging Spectrometer Next Generation(AVIRIS-NG) images with known methane plumes to create two simulated satellite products. One simulation had a 30 m spatial resolution with ~200 Signal-to-Noise Ratio (SNR) in the Shortwave Infrared (SWIR) and the other had a 60 m spatial resolution with ~400 SNR in the SWIR; both products had a 7.5 nm spectral spacing. We applied a linear matched filter with a sparsity prior and an albedo correction to detect and quantify the methane emission in the original AVIRIS-NG images and in both satellite simulations. We also calculated an emission flux for all images. We found that all methane plumes were detectable in all satellite simulations. The flux calculations for the simulated satellite images correlated well with the calculated flux for the original AVIRIS-NG images. We also found that coarsening spatial resolution had the largest impact on the sensitivity of the results. These results suggest that methane detection and quantification of point sources will be possible with the next generation of satellite imaging spectrometers.


2009 ◽  
Vol 78 (Suppl.A) ◽  
pp. 157-160 ◽  
Author(s):  
Mitsuteru Mimura ◽  
Hiroki Kusano ◽  
Shingo Kobayashi ◽  
Mitsuhiro Miyajima ◽  
Nobuyuki Hasebe

Author(s):  
Pantazis Mouroulis ◽  
Robert O. Green ◽  
Daniel W. Wilson ◽  
Christopher D. Smith ◽  
Myrtle F. Lin

2018 ◽  
Vol 215 ◽  
pp. 386-397 ◽  
Author(s):  
Alana K. Ayasse ◽  
Andrew K. Thorpe ◽  
Dar A. Roberts ◽  
Christopher C. Funk ◽  
Philip E. Dennison ◽  
...  

1996 ◽  
Vol 119 (3) ◽  
pp. 531-546 ◽  
Author(s):  
L. Weitzel ◽  
A. Krabbe ◽  
H. Kroker ◽  
N. Thatte ◽  
L. E. Tacconi-Garman ◽  
...  

2004 ◽  
Vol 34 (12) ◽  
pp. 2688-2690 ◽  
Author(s):  
T.G. Tsuru ◽  
T. Tanimori ◽  
A. Bamba ◽  
K. Imanishi ◽  
K. Koyama ◽  
...  

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