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Related Concept Videos

Radiation: Applications01:17

Radiation: Applications

The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
P-N junction01:11

P-N junction

A p-n junction is formed when p-type and n-type semiconductor materials are joined together. At the interface of the p-n junction, holes from the p-side and electrons from the n-side begin to diffuse into the opposite sides due to the concentration gradient. This diffusion of carriers leads to a region around the junction where there are no free charge carriers, known as the depletion region. The charge density within the depletion region for the n-side and p-side can be described by the...
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Light as Energy01:35

Light as Energy

The energy required to carry out photosynthesis is light— typically electromagnetic radiation from the sun. The range of all possible wavelengths is known as the electromagnetic spectrum.
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Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
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UV–Vis Spectrometers01:14

UV–Vis Spectrometers

The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell. Samples for...

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Experimental System of Solar Adsorption Refrigeration with Concentrated Collector
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Absorber for solar power.

W R Powell

    Applied Optics
    |February 6, 2010
    PubMed
    Summary
    This summary is machine-generated.

    This study introduces a new, economical solar absorber with low reradiation losses. It achieves high thermal and conversion efficiencies, making it suitable for terrestrial and space applications.

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    Area of Science:

    • Thermodynamics
    • Solar Energy Conversion
    • Materials Science

    Background:

    • Traditional solar absorbers often suffer from significant reradiation losses, limiting their efficiency.
    • Developing cost-effective absorbers is crucial for widespread solar energy adoption.

    Purpose of the Study:

    • To describe a novel, economical solar absorber design.
    • To analyze the performance and efficiency of this new absorber technology.

    Main Methods:

    • The study details a new operating principle for a solar absorber.
    • Performance analysis was conducted for terrestrial and space-based applications.

    Main Results:

    • The absorber demonstrates very low reradiation losses.
    • Achieved approximately 90% thermal efficiency and 73% conversion efficiency for terrestrial use.
    • Higher conversion efficiencies are possible in space applications below 300 K.

    Conclusions:

    • The developed solar absorber is both simple and economical.
    • Its high efficiency and compatibility with low-cost concentrators make it viable for diverse applications.
    • Space-based applications offer potential for even greater conversion efficiency.