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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 ^
gerb_content.1268062432.txt.gz ยท Last modified: 2010/03/08 15:33 by ebaudrez