|
|
 |
|
 |
Surface AlbedoProducts - Radiation
The albedo is the fraction of the incoming solar radiation reflected by
the land surface, integrated over the whole viewing directions. The
albedo can be directional (calculated for a given sun zenith angle) or
hemispheric (integrated over the whole illumination directions),
spectral (for each narrow band of the sensor) or broadband (integrated
over the whole solar spectrum).
MEDIAS-France
and EARS
assess the various albedo products using different approaches applied to
VEGETATION and METEOSAT measurements.
Broadband hemispheric surface albedo derived
from VEGETATION data over South-West of France, August 2000
MEDIAS-France generates many albedo products
from VEGETATION / SPOT data using the
FP5 / CYCLOPES
processing line. Observations acquired during a compositing
period are first cloud-screened and corrected for atmospheric effects.
Then, they are directionnally normalized by inversion of a 3-parameter
linear bidirectional reflectance model (Roujean et al., 1992) following the
approach presented in Hagolle et al. (2005). The inversion yields three
coefficients, a nadir-zenith reflectance, a geometric and
a volumetric coefficients, used to estimate directional, hemispheric, spectral
and broadband albedos.
MEDIAS-France defines the customization specifications to fit
the ONC
requirements which needs 0.5°x0.5° tiled averages (mean and standard
deviation values) maps of broadband visible and near-infrared hemispheric
albedos for 8 vegetation classes ("conifer evergreen forest",
"deciduous forest", "broadleaf evergreen forest","grassland C3","grassland C4",
"crops C3", "crops C4"). The number of valid pixels available to compute the
average is also provided, because it is useful to assess the product quality.
Broadband visible surface albedo derived from METEOSAT images over
Euro-Mediterranean region, central 10-day period of July 1998.
The surface albedo is also a product of
the EWBMS (Energy Water Balance Monitoring System)
database provided by EARS. It is derived from METEOSAT
visible (0.3-1.5 µm) images, so its spatial resolution is 5 km
sub-satellite. The first step of the methodology consists in
calibrating the noon visible METEOSAT image to obtain the daily
planetary albedo. The planetary albedo is related to the surface albedo by
means of a two-flux radiation transmission model, modified after Kondratyev
(1969). In this model the turbidity of the atmosphere is parameterized by the
atmospheric optical depth. One pair of corresponding planetary and surface
albedo values is required to determine the atmospheric optical depth. A darkest
pixel approach is used, which relates the minimum planetary albedo of land
pixels occurring in the image, to the lowest land surface albedo, usually
present over forest. The value of atmospheric optical depth thus obtained is
assumed to apply as a first order atmospheric correction to the whole image.
Knowing this value, the actual atmospheric correction consists in converting
all planetary albedo to surface albedo. In this way, a daily surface albedo
map is obtained. Finally, as the daily surface albedo is not expected to
change fast, but may be sub-pixel cloud contaminated, a 10-day lowest value
surface albedo composite is generated, which is supposed to represent the
cloud free situation.
References
Hagolle, O., A. Lobo, P. Maisongrande, F. Cabot, B. Duchemin, A. De Peyreira,
Quality assessment and improvement of temporally composited products of
remotely sensed imagery by combination of VEGETATION 1&2 images, Remote
Sensing of Environment, vol.94, 2, 172-186, 2005.
Kondratyev, K.Y., Radiation in the atmosphere, New York, London: Academic
Press, 1969.
Roujean J.L., M. Leroy, and P.Y. Deschamps, A bidirectional
reflectance model of the Earth’s surface for the correction of remote
sensing data, Journal of Geophysical Research, 97, D18, 20,455-20,468,
1992.
Download
|
|
|
|