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GOME-1 surface LER database |
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Tropospheric
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NO2
- global CH2O - global CO - global |
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UV
- UV index - UV dose |
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Ozone
- total column - global field - ozone bulletin - ozone profiles - tropospheric |
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Aerosol
- ADRE - aerosol index Methane - global CO2 - global Clouds - cloud info Surface - solar irradiance |
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Volcanic plume
- SO2 & AAI |
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Albedo
- climatologies Fluorescence - sun-induced |
Robert Koelemeijer has created a surface albedo database that contains the minimum Lambertian-equivalent reflectivity (LER) values at 11 one-nm wide wavelength bins. The surface LER values were derived from GOME-1 data using the Doubling-Adding KNMI (DAK) polarised radiative transfer code. The model consists of an atmosphere for which Rayleigh scattering and ozone absorption is taken into account, and which is bounded below by a Lambertian surface. You can read Robert Koelemeijer's README file for more details.
An alternative for the GOME-1 surface LER database is the SCIAMACHY surface LER database. This database is based on SCIAMACHY mission data and as a result offers a higher quality in terms of stability, residual cloud contamination, and spatial resolution near coastlines.
Validation of the GOME-1 surface LER climatology based on direct
intercomparison with the SCIAMACHY, OMI, and GOME-2 surface LER
climatologies is described here.
If you're planning to use this database, please refer to the scientific
paper describing the database, which is available as a PDF file (2.7 MB).
Some examples
of the database:
Examples of the GOME-1 surface LER: for 4 different wavelength bands (left) and for 4 different months (right). |
Surface albedo
improvements at 758 and 772 nm:
This improved surface albedo database is based on the original surface
albedo database created by Koelemeijer et al. (2003) which has a
1°×1° spatial resolution. The surface albedo grids at 758
and 772 nm were refined to a spatial resolution of
0.25°×0.25° at coastlines. Because of absorbing aerosol
over desert areas, the retrieved surface albedo over these areas is
lower than its real value. This problem was corrected by increasing the
surface albedo over desert areas by 20% (Fournier et al., 2006). These
improvements were only applied to the surface albedos at 758 and 772 nm,
not to the other wavelength bands.
Archive:
The database, consisting of a large number of files (196 kB each), was
originally put together in one large file, together with a PostScript
image of the data. The large file containing the entire database can be
downloaded below. For more convenient downloading, the database has also
been split up into 11 zip-files, one per wavelength. Each of these files
contains the following files:
sacspecTOTL[mm]_[wvl].dat
[mm]
and
wavelength [wvl]
nm sacspecALLM[wvl].dat
[wvl]
nm sacspecFLAG[wvl].dat
sacspecFLAG[mm].dat
for the TOTL files, one for each month and valid for all wavelength bands.
These are zipped together in a 12-th file. The reason for splitting up the
database is to minimise the download effort in case you do not need the
data of all wavelength bands.
Wavelength band | Monthly data files (zipped) * | Monthly PostScript images (zipped) * |
335 nm | ler335nm.zip | ler335nm_ps.zip |
380 nm ** | ler380nm.zip | ler380nm_ps.zip |
416 nm | ler416nm.zip | ler416nm_ps.zip |
440 nm | ler440nm.zip | ler440nm_ps.zip |
463 nm | ler463nm.zip | ler463nm_ps.zip |
494 nm | ler494nm.zip | ler494nm_ps.zip |
555 nm | ler555nm.zip | ler555nm_ps.zip |
610 nm | ler610nm.zip | ler610nm_ps.zip |
670 nm | ler670nm.zip | ler670nm_ps.zip |
758 nm | ler758nm.zip ler758nm_corr.zip *** |
ler758nm_ps.zip ler758nm_corr_ps.zip *** |
772 nm | ler772nm.zip ler772nm_corr.zip *** |
ler772nm_ps.zip ler772nm_corr_ps.zip *** |
for all wavelengths |
lerFLAG.zip (145 kB; unzipped 2.4 MB) |
lerFLAG_ps.zip (765 kB; unzipped 3.7 MB) |
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Documentation: