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This is called the "albedo." It is the ratio of reflected light compared to incident light, and depends on the surface material and its condition (e.g. snow, grassland).
An absorption nebula is a dark nebula, which absorbs all incident radiation without reemission.
You could simply say 'the percentage of incident light which is not absorbed by the surface'. The technical term, used mainly in astronomy, is albedo.
The quantity of solar radiation incident normally per minute on 1 cm2 surface of a perfectly black body on the Earth.
i do know that its a diffuse mass of interstellar dust or gas or both, visible as luminous patches or areas of darkness depending on the way the mass absorbs or reflects incident radiation. Hope that helps. :)
An absorptance is a ratio measuring absorbed radiation and incident radiation - to show how well a particular surface absorbs radiation.
About 19% of incoming solar radiation is absorbed by clouds and the atmosphere.Incoming solar radiation: 100%Reflected by the atmosphere: 6% : Absorbed by the atmosphere: 16%Continuing incoming solar radiation: 78%Reflected by clouds: 20% : Absorbed by clouds: 3%Continuing incoming solar radiation: 55%Reflected by the earth's surface: 4% : Absorbed by the earth's surface (lands and oceans): 51%Source: (NASA)
A higher albedo means that more of the incident radiation is reflected, and less of it is absorbed.
There are many factors associated with the absorption of solar energy based primarily on the wavelength or nature of the solar energy under consideration. For example, neutrinos are mostly not absorbed at all. "Albedo" is used to express how much incident radiation from the Sun is reflected or absorbed, and the albedo changes for different wavelengths of light (electromagnetic radiation); it is a specific term of "reflectivity." In turn, albedo is determined by the cloud cover, terrestrial terrain, composition of the atmosphere etc. Longwave (red-shift) radiation absorption may be very different than UV (shortwave), and some wavelenghts may "bounce" completely, and very little of the incident radiation may be absorbed on the Earth's surface.
There are many factors associated with the absorption of solar energy based primarily on the wavelength or nature of the solar energy under consideration. For example, neutrinos are mostly not absorbed at all. "Albedo" is used to express how much incident radiation from the Sun is reflected or absorbed, and the albedo changes for different wavelengths of light (electromagnetic radiation); it is a specific term of "reflectivity." In turn, albedo is determined by the cloud cover, terrestrial terrain, composition of the atmosphere etc. Longwave (red-shift) radiation absorption may be very different than UV (shortwave), and some wavelenghts may "bounce" completely, and very little of the incident radiation may be absorbed on the Earth's surface.
radiation use efficiency is the percentage part of incident solar radiation spectrum being utilized by plants.
An absorption coefficient is a measure of the absorption of electromagnetic radiation as it passes through a specific substance - calculated as the fraction of incident radiation absorbed by unit mass or unit thickness.
This is called the "albedo." It is the ratio of reflected light compared to incident light, and depends on the surface material and its condition (e.g. snow, grassland).
The answer to this question involves the angle at which solar radiation is intercepted by the earth's atmosphere. The rule is that if solar radiation is incident perpendicular to the atmosphere the solar radiation that is incident on the earth's surface will be greatest. Incoming solar radiation at the poles comes in at a sharper angle and is spread over a greater surface area of atmosphere than at the equator. In this way, the poles have more of an atmospheric filter and experience less radiation per area time and hence have lower average temperatures.
It is likely that ozone only absorbs a tiny percentage of the UV-C incident on Earth's atmosphere. Likely the majority of UV-C is absorbed by nitrogen and oxygen in the atmosphere, and that in the lower stratosphere (where ozone is produced).
If you are referring to visible light, which lies in the wavelength range from 380 to 740 nm of the electromagnetic radiation spectrum, an opaque body won't allow light to travel trough it. When light hits the surface of the body the light can be, reflected, absorbed, or part of it reflected and the rest absorbed. In the case you are referring to thermal radiation which lies in the wavelength range from about 1 x 102 to 1 x 105 nm, an opaque body to thermal radiation will behave the same. In this later case the way the body's surface will behave is given by the surface properties reflectivity and absorptivity, which are the fraction of the incident radiation that is reflected and absorbed by the surface respectively.
Radiation is a general term for the energy transmitted through space.Incident radiation is a term used when referring to the radiation hitting a specific surface. For instance, the incident radiation for a solar panel is the total amount of radiation hitting the surface of the solar panel. This is in contrast to direct beam radiation which refers to only that radiation which arrives in a strait line from the sun. (It differs in that total incident radiation includes additionally the component of diffuse radiation.)