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gerb_content [2010/03/08 15:33] ebaudrez images were scaled down a bit (req NC) |
gerb_content [2022/06/14 09:34] (current) moreelsj [GERB Data Content] |
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====== GERB Data Content ====== | ====== GERB Data Content ====== | ||
- | These pages aim to give you a visual description of the main fields contained in the GERB data files. For each field, a short description is given and a false color image is presented. The full list and description of the GERB data content is available in the [[ftp://gerb.oma.be/Documents/userguide.pdf|GERB level 2 User Guide]]. | + | These pages aim to give you a visual description of the main fields contained in the GERB data files. For each field, a short description is given and a false color image is presented. The full list and description of the GERB data content is available in the [[this>/Documents/userguide.pdf|GERB level 2 User Guide]]. |
===== /Radiometry ===== | ===== /Radiometry ===== | ||
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==== /Radiometry/Solar Flux ==== | ==== /Radiometry/Solar Flux ==== | ||
- | This field gives the quantity of the incoming solar radiation which is reflected by the Earth-atmosphere system. The higher values for the solar reflected flux are observed over optically thick cloud cover located close to the Sun-subpoint where the illumination is maximum. The physical unit for this quantity is the Watt per square meter (W/m2). In the GERB data file, the solar flux is quantify using a quantification factor 0.25 W/m2. An animation showing the variation of the solar reflected flux for a 48-hour period is available [[http://gerb.oma.be/gerb/LastImages/anim_sol_flux.gif|here]]. | + | This field gives the quantity of the incoming solar radiation which is reflected by the Earth-atmosphere system. The higher values for the solar reflected flux are observed over optically thick cloud cover located close to the Sun-subpoint where the illumination is maximum. The physical unit for this quantity is the Watt per square meter (W/m2). In the GERB data file, the solar flux is quantify using a quantification factor 0.25 W/m2. |
{{sol_flux.jpg?400}} | {{sol_flux.jpg?400}} | ||
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==== /Radiometry/Thermal Flux ==== | ==== /Radiometry/Thermal Flux ==== | ||
- | This field gives the quantity of energy thermally emitted by the Earth-atmosphere system. The higher values for the thermal flux are observed over hot desert areas under clear sky conditions. Clouds usually cause a decrease of the thermal emission from the Earth to the space (greenhouse effect of clouds). The physical unit for this quantity is the Watt per square meter (W/m2). In the GERB data file, the thermal flux is quantify using a quantification factor 0.25 W/m2. An animation showing the variation of the thermally emitted flux for a 48-hour period is available [[http://gerb.oma.be/gerb/LastImages/anim_th_flux.gif|here]]. | + | This field gives the quantity of energy thermally emitted by the Earth-atmosphere system. The higher values for the thermal flux are observed over hot desert areas under clear sky conditions. Clouds usually cause a decrease of the thermal emission from the Earth to the space (greenhouse effect of clouds). The physical unit for this quantity is the Watt per square meter (W/m2). In the GERB data file, the thermal flux is quantify using a quantification factor 0.25 W/m2. |
{{th_flux.jpg?400}} | {{th_flux.jpg?400}} | ||
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The code is available on the web site of the CERES inversion group (led by Norman Loeb). | The code is available on the web site of the CERES inversion group (led by Norman Loeb). | ||
- | * [[http://asd-www.larc.nasa.gov/Inversion/adm/trmm-adm-sw-type.tab|CERES-TRMM code]] | + | * [[https://ceres.larc.nasa.gov/data/angular-distribution-models/|CERES-TRMM code]] |
^ value ^ scene ^ | ^ value ^ scene ^ |