IEEE International Geoscience and Remote Sensing Symposium
DOI: 10.1109/igarss.2002.1026134
|View full text |Cite
|
Sign up to set email alerts
|

FLAASH, a MODTRAN4-based atmospheric correction algorithm, its application and validation

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
180
0
6

Publication Types

Select...
5
4
1

Relationship

0
10

Authors

Journals

citations
Cited by 285 publications
(186 citation statements)
references
References 15 publications
0
180
0
6
Order By: Relevance
“…These outputs extend from the UV into the far-infrared (0.2-10,000 µm) spectral range and are provided at a resolution as fine as 0.1 cm −1 (0.01-0.1 nm in the VIS-SWIR spectral range). However, in most MODTRAN remote sensing application (e.g., [9,[64][65][66]), these outputs are decomposed in a set of key atmospheric transfer functions [63,67] that allows to invert the atmospheric TOA radiance equation. The standard formulation under the Lambertian assumption is given by:…”
Section: Modtran5mentioning
confidence: 99%
“…These outputs extend from the UV into the far-infrared (0.2-10,000 µm) spectral range and are provided at a resolution as fine as 0.1 cm −1 (0.01-0.1 nm in the VIS-SWIR spectral range). However, in most MODTRAN remote sensing application (e.g., [9,[64][65][66]), these outputs are decomposed in a set of key atmospheric transfer functions [63,67] that allows to invert the atmospheric TOA radiance equation. The standard formulation under the Lambertian assumption is given by:…”
Section: Modtran5mentioning
confidence: 99%
“…The pan sharpened Worldview-2 image, acquired on 9 th December 2009, was comprised of eight wavebands each with a spatial resolution of 0.5 m. Pre-processing procedures including atmospheric correction using the FLAASH (Fast Line-of-sight Atmospheric Analysis of Spectral Hypercubes) algorithm provided in the Environment for Visualising Images (TM) software (Cooley et al 2002), image masking and water column correction were applied to the satellite image to yield radiance data that could be used as input to a classification algorithm. Bathymetric information to support these corrections was provided by the Australian Hydrographic office in the form of an airborne survey flown by LADS (Laser Airborne Depths Sounder), corrected to a horizontal datum of WGS1984 and a vertical datum of Lowest Astronomical tide (Fugro, 2011).…”
Section: Image Processingmentioning
confidence: 99%
“…Some pre-processing steps are necessary before using image. Firstly, some bad pixel value in original image were replaced by the means of two pixels value beside its two sides; then the image was radiometrically corrected using calibration coefficient; at last, the image was atmospheric corrected using FLAASH model [10]. Figure 3 and figure 4 shows different ground objects spectra before and after atmospheric correction.…”
Section: Remote Sensing Datamentioning
confidence: 99%