When solar irradiance is measured on the outer surface of earth s atmosphere 2 the measurements can be adjusted using the inverse square law to infer the magnitude of solar irradiance at one au and deduce the solar constant 3.
The solar constant is quizlet.
The sun s altitude is measured in the number of degrees above the horizon.
The solar constant is the amount of energy received at the top of the earth s atmosphere on a surface oriented perpendicular to the sun s rays at the mean distance of the earth from the sun.
What is the unit of measurement for the sun s altitude.
Solar constant the total radiation energy received from the sun per unit of time per unit of area on a theoretical surface perpendicular to the sun s rays and at earth s mean distance from the sun.
Find the following statement s that correctly describe the stefan boltzmann s law.
It is most accurately measured from satellites where atmospheric effects are absent.
What is the meaning of the solar constant the amount of energy the earth receives per unit area and unit time hydrogen burning by fusion reactions occurs only in the deep interior of the sun and other stars because this is the only place in the sun where.
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The solar constant at the surface of the earth is 1 000 watts per square meter at sea level at solar noon.
Refers to the intensity of solar radiation that actually reaches earth s surface.
The value of the constant is approximately 1 366 kilowatts per square metre.
The portion of solar radiation that is partially blocked by ozone in the stratosphere is the sun according to wien s displacement law which one of the following objects emits the most intense electromagnetic energy at the shortest wavelength.
The solar constant includes all types of solar radiation other than neutrinos not just the visible light.
Must be measured at aphelion.
The term radiative forcing describes a measure of the effect of a climatic factor has on the balance between incoming solar radiation and outgoing infrared radiation.
The solar constant a measure of flux is the amount of incoming solar electromagnetic radiation per unit area that would be incident on a plane perpendicular to the rays at a distance of one astronomical unit au roughly the mean distance from the sun to the earth.
Is about 0 5 calories per square centimeter per minute.
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Earth s solar constant a.