Find the following statement s that correctly describe the stefan boltzmann s law.
The solar constant is quizlet.
It is measured by satellite as being 1 361 kilo watts per square meter kw m at solar minimum the time in the 11 year solar cycle when the number of sunspots is minimal and approximately 0 1 greater roughly 1 362 kw m at solar maximum.
Refers to the intensity of solar radiation that actually reaches earth s surface.
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Must be measured at perihelion.
What is the unit of measurement for the sun s altitude.
How does a pv cell receive the highest average insolation.
The sun s altitude is measured in the number of degrees above the horizon.
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.
It is most accurately measured from satellites where atmospheric effects are absent.
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.
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.
Is about 0 5 calories per square centimeter per minute.
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 includes all types of solar radiation other than neutrinos not just the visible light.
The solar constant at the surface of the earth is 1 000 watts per square meter at sea level at solar noon.
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Earth s solar constant a.
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.
Must be measured at aphelion.