DocumentCode
1880880
Title
The signal to noise ratio assessment of CE-1 IIM data
Author
Shuai, Tong ; Zhang, Xia ; Zhao, Dong
Author_Institution
Inst. of Remote Sensing Applic., Beijing, China
fYear
2011
fDate
24-29 July 2011
Firstpage
1029
Lastpage
1032
Abstract
As one of the most important payloads on Chang´e-1 satellite, the Interference Imaging Spectrometer (IIM) got large amounts of hyperspectral data for retrieving elements and mineral information of the lunar surface. The signal to noise ratio (SNR) of the IIM hyperspectral data has been assessed for the further applications of the IIM data. As the assessment results show, the SNR of the IIM data shows good value on the whole and the middle bands are much higher than the bands at the both ends. As the reflectance peak of the plagioclase and the pyroxene spectrum, the bands centered around 750nm exhibit high SNR, which is of great importance for retrieving elements and minerals on the lunar surface. However, the bands centered around 930nm, as the absorption valley, exhibit poor SNR. As the SNRs are not high enough on the whole, the noises of the first nine bands should be reduced carefully before used, although they have an obvious trend of rising. Moreover, the first band and the last one have too low SNRs to use.
Keywords
astronomical instruments; astronomical spectra; lunar surface; CE-1 IIM DATA; Chang´e-1 satellite; Interference Imaging Spectrometer; absorption valley; element information retrieval; hyperspectral data; lunar surface; mineral information retrieval; plagioclase; pyroxene spectrum; reflectance peak; signal-to-noise ratio assessment; Hyperspectral imaging; Imaging; Moon; Reflectivity; Signal to noise ratio; CE-1; IIM; SNR; Signal to Noise Ratio; information quality;
fLanguage
English
Publisher
ieee
Conference_Titel
Geoscience and Remote Sensing Symposium (IGARSS), 2011 IEEE International
Conference_Location
Vancouver, BC
ISSN
2153-6996
Print_ISBN
978-1-4577-1003-2
Type
conf
DOI
10.1109/IGARSS.2011.6049309
Filename
6049309
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