Atmospheric correction

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Atmospheric correction is the process of removing the scattering and absorption effects of the atmosphere on the reflectance values of images taken by satellite or airborne sensors. [1] [2] Atmospheric effects in optical remote sensing are significant and complex, dramatically altering the spectral nature of the radiation reaching the remote sensor. [3] The atmosphere both absorbs and scatters various wavelengths of the visible spectrum which must pass through the atmosphere twice, once from the sun to the object and then again as it travels back up the image sensor. These distortions are corrected using various approaches and techniques, as described below. [4]

Contents

Examples of Atmospheric Correction Methods

Examples of atmospheric correction techniques for multispectral remote-sensing images, ordered chronologically to show the historical development of atmospheric correction methods in remote-sensing.
SensorApproach
MSSband-to-band regression [5]
MSSall-band spectral covariance [6]
airborne MSSband-to-band regression [7]
AVHRRiterative estimation [8]
MSS, TMDOS with exponential scattering model [9]
TMDOS with exponential scattering model, downwelling atmospheric radiance measurements [10]
TMpixel-by-pixel tasseled cap haze parameter [11]
AVHRRDOS, NDVI, AVHRR band 3 [12]
airborne TMS, Landsat TMground and airborne solar measurements, atmospheric modeling code [13]
TMcomparison of ten DOS and atmospheric modeling code variations with field data [14]
TMdark target, modeling code [15]
TM (all bands)atmospheric modeling code, region histogram matching [16]
TMDOS with estimated atmospheric transmittance [17]
TMdark target, atmospheric modeling code
TM, ETM+empirical line method, single target, ground measurements
TMwater reservoirs, comparison of 7 methods for 12 dates
AVHRR2-band PCT used to separate aerosol components

See also

Related Research Articles

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References

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