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- 33f0ec3e-cd6d-498c-9468-749741fc12e2 TargetsLocation 507794a1-9563-49a4-b2d3-8a28347c1fd7 @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 type Science_Keyword @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 type Variable @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 broader 1eb0ea0a-312c-4d74-8d42-6f1ad758f999 @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 broader 2e83362e-d8f8-4bca-83fd-bae360ebe94b @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 broader 57383ac5-614c-4b84-9202-e137b000422b @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 broader e9f67a66-e9fc-435c-b720-ae32a2c3d8f5 @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 definition "Solar irradiance at the top of the atmosphere on a plane normal to theincidentradiation and at the mean distance of the Earth from the Sun Solarirradianceis also referred to as the solar constant In satellite remotesensing thesolar irradiance is used as an onboard calibration of visible bandsensorsSome climate studies suggest that small variations in the solarirradianceassociated with solar activity over days to decades may have aneffect theEarths climateThe intensity of the suns radiation at different wavelengths The radiation isgenerally given in terms of solar constant S defined in terms of flux oftotal radiation received outside the earths atmosphere per unit area at meansun earth distance and has the value S 134 X 106 ergs cm2 sec1" @default.
- 33f0ec3e-cd6d-498c-9468-749741fc12e2 prefLabel "SOLAR_IRRADIANCE" @default.