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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.
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Light Acquisition

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Radiation Pressure: Problem Solving

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The Wave Nature of Light02:12

The Wave Nature of Light

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Atomic Absorption Spectroscopy: Radiation and Light Sources01:13

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Updated: Jun 16, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

Rayleigh, the unit for light radiance.

D J Baker

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

    A new formula accurately converts power spectral radiance to rayleigh spectral radiance, simplifying atmospheric and optical measurements. This conversion aids in calculating photon emission rates from various altitudes.

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    Area of Science:

    • Atmospheric Optics
    • Radiometry
    • Spectroscopy

    Background:

    • Power spectral radiance (L(lambda)) is a standard unit for measuring light intensity.
    • Rayleigh spectral radiance is a more intuitive unit for certain atmospheric and astrophysical phenomena.
    • A direct and accurate conversion between these units is needed for consistent data analysis.

    Purpose of the Study:

    • To derive an accurate formula for converting power spectral radiance to rayleigh spectral radiance.
    • To elucidate the physical basis for the rayleigh unit in terms of photon and solid angle factors.
    • To extend the application of this conversion for calculating photon volume emission rates.

    Main Methods:

    • Derivation of a conversion formula: R(lambda) = 2πλL(lambda) x 10^13.
    • Analysis of the photon rate factor and solid angle factor.
    • Application of an equivalence theorem for optical receivers and extended sources.

    Main Results:

    • A formula with 0.7% accuracy for converting L(lambda) (W cm⁻² sr⁻¹ μm⁻¹) to R(lambda) (Rayleigh/μm).
    • The formula is R(lambda) = 2πλL(lambda) x 10^13, with λ in μm.
    • Demonstrated extension to compute photon volume emission rates from zenith radiance profiles.

    Conclusions:

    • The derived formula provides an easy and accurate method for interconverting radiance units.
    • Understanding the factors behind the rayleigh unit enhances data interpretation in atmospheric studies.
    • This conversion facilitates the calculation of photon emission rates, crucial for atmospheric modeling.