green_component_of_toa_outgoing_shortwave_flux_expressed_as_rgb_color

under discussion
Created: 28 Mar 2025
Proposer: Luke Marsden
Proposed Date: 2024-11-19
add to cfeditor
Change Date: 28 Mar 2025, 11:40 a.m.
normalised_green_wavelength_intensity_of_point 1
Intensity of electromagnetic radiation in the green wavelength band reflected or emitted from a point. Values are scaled relative to a reference intensity or maximum possible value. Green corresponds to the green component of the RGB colour model.
Change Date: 28 Mar 2025, 11:40 a.m.
normalised_green_wavelength_intensity_of_point 1 [UUUU]
Intensity of electromagnetic radiation in the green wavelength band reflected or emitted from a point. Values are scaled relative to a reference intensity or maximum possible value. Green corresponds to the green component of the RGB colour model.
Change Date: 28 Mar 2025, 3:09 p.m.
green_component_of_toa_outgoing_shortwave_flux_expressed_as_rgb_color 1 [UUUU]
Green corresponds to the green component of the RGB model. The term "shortwave" means shortwave radiation. The TOA outgoing shortwave flux is the reflected and scattered solar radiative flux, i.e., the "upwelling" TOA shortwave flux, sometimes called the "outgoing shortwave radiation" or "OSR". In accordance with common usage in geophysical disciplines, "flux" implies per unit area, called "flux density" in physics. The intensity is scaled relative to a reference intensity or the maximum possible value. It is recommended that the variable attributes valid_min and valid_max or valid_range are used to denote the range of possible values (e.g., 0 to 1, 0 to 255, 0 to 65,535). The radiation wavelength or frequency range for green can be denoted as bounds of a scalar coordinate variable.

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