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Related Concept Videos

Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

729
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.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
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Maxwell-Boltzmann Distribution: Problem Solving01:20

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Individual molecules in a gas move in random directions, but a gas containing numerous molecules has a predictable distribution of molecular speeds, which is known as the Maxwell-Boltzmann distribution, f(v).
This distribution function f(v) is defined by saying that the expected number N (v1,v2) of particles with speeds between v1 and v2 is given by
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Absorption of Radiation01:05

Absorption of Radiation

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The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
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Design Example: Calculating Safe Diameter for Wind-Exposed Disc01:17

Design Example: Calculating Safe Diameter for Wind-Exposed Disc

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Assessing safety in wind-exposed installations is crucial to preventing potential failures. This example explores the calculation and design adjustments needed to mount a circular disc on a building facade, where wind forces are a primary concern. A 4-meter diameter disc was initially designed as an aesthetic feature facing winds at a velocity of 25 meters per second, with an air density of 1.25 kilograms per cubic meter. Given these conditions, the drag force on the disc was determined using...
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Radiation: Applications01:17

Radiation: Applications

1.6K
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...
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Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

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An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container.
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Related Experiment Video

Updated: Dec 27, 2025

Scattering And Absorption of Light in Planetary Regoliths
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A Physics-Based DNI Model Assessing All-Sky Circumsolar Radiation.

Yu Xie1, Manajit Sengupta1, Yangang Liu2

  • 1Power Systems Engineering Center, National Renewable Energy Laboratory, Golden, CO 80401, USA.

Iscience
|February 24, 2020
PubMed
Summary

Accurate solar energy calculations require precise direct normal irradiance (DNI) measurements. This study introduces a new physical model to significantly reduce bias in cloudy-sky DNI, improving solar power generation estimates.

Keywords:
Energy ResourcesEnvironmental ScienceRadiation Measurement

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Area of Science:

  • Atmospheric science
  • Renewable energy systems

Background:

  • Current methods for calculating direct normal irradiance (DNI) using the Beer-Bouguer-Lambert law and empirical models exhibit significant bias under cloudy-sky conditions.
  • This bias introduces substantial uncertainty in estimating solar energy conversion system electricity generation.

Purpose of the Study:

  • To address the bias in cloudy-sky DNI calculations.
  • To propose a physically-based, all-sky DNI model that enhances accuracy for solar energy applications.

Main Methods:

  • Utilized long-term observations from the Atmospheric Radiation Measurement (ARM) Southern Great Plains (SGP) site.
  • Developed a novel model computing solar radiation along the sun's direction and scattered circumsolar radiation using finite-surface integration in differential solid angles.

Main Results:

  • The proposed physical model significantly reduces uncertainty in DNI calculations by a factor of 2-7 compared to existing methods.
  • Demonstrated a substantial improvement in computing cloudy-sky DNI.

Conclusions:

  • The new all-sky DNI model offers a more accurate and reliable method for solar radiation assessment.
  • Reduced uncertainty in DNI estimation will lead to more precise solar electricity generation forecasts.