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Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

686
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...
686
Maxwell-Boltzmann Distribution: Problem Solving01:20

Maxwell-Boltzmann Distribution: Problem Solving

2.7K
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
2.7K
Calculation of Electric Flux01:25

Calculation of Electric Flux

2.7K
Consider the electric field of an oppositely charged, parallel-plate system and an imaginary box between those plates. Let the bottom face of the box be ABCD, and the top face be FGHK. The electric field between the plates is uniform and points from the positive plate toward the negative plate. The calculation of this field's flux through the box's various faces shows that the net flux through the box is zero. Why does the flux cancel out here?
2.7K
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

2.3K
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.
2.3K
Potential Due to a Magnetized Object01:24

Potential Due to a Magnetized Object

701
Magnetic dipoles in magnetic materials are aligned when placed under an external magnetic field. For paramagnets and ferromagnets, dipole alignment occurs in the direction of the magnetic field. However, the dipoles align opposite to the field in the case of diamagnets. This state of magnetic polarization due to the external field is called magnetization. Magnetization is defined as the dipole moment per unit volume. It plays a similar role to polarization in electrostatics.
The vector...
701
Potential Due to a Polarized Object01:29

Potential Due to a Polarized Object

648
A neutral atom consists of a positively charged nucleus surrounded by a negatively charged electron cloud. When placed in an external electric field, the external electric force pulls the electrons and nucleus apart, opposite to the intrinsic attraction between the nucleus and the electrons. The opposing forces balance each other with a slight shift between the center of masses of the nucleus and the electron cloud, resulting in a polarized atom. On the other hand, a few molecules, like water,...
648

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Related Experiment Video

Updated: Dec 13, 2025

Indoor Experimental Assessment of the Efficiency and Irradiance Spot of the Achromatic Doublet on Glass ADG Fresnel Lens for Concentrating Photovoltaics
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Indoor Experimental Assessment of the Efficiency and Irradiance Spot of the Achromatic Doublet on Glass ADG Fresnel Lens for Concentrating Photovoltaics

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A physics-based method that can predict imminent large solar flares.

Kanya Kusano1, Tomoya Iju2, Yumi Bamba3,4

  • 1Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8601, Japan. kusano@nagoya-u.jp.

Science (New York, N.Y.)
|August 1, 2020
PubMed
Summary
This summary is machine-generated.

A new physics-based model, the κ-scheme, accurately predicts large solar flares by identifying critical magnetohydrodynamic instability. This model uses magnetic twist flux density to determine flare occurrence, location, and size, improving space weather forecasting.

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Area of Science:

  • * Solar Physics
  • * Space Weather
  • * Plasma Physics

Background:

  • * Solar flares are energetic coronal events impacting Earth's space weather.
  • * Current solar flare prediction relies on empirical methods due to an unknown onset mechanism.
  • * Understanding flare triggers is crucial for improving forecasting capabilities.

Purpose of the Study:

  • * To introduce a physics-based model, the κ-scheme, for predicting large solar flares.
  • * To investigate the role of magnetohydrodynamic instability and magnetic reconnection in flare initiation.
  • * To identify key parameters determining flare occurrence, location, and magnitude.

Main Methods:

  • * Development of the κ-scheme, a physics-based predictive model.
  • * Analysis of X-class solar flares from 2008 to 2019 (Solar Cycle 24).
  • * Examination of magnetic twist flux density near polarity inversion lines.

Main Results:

  • * The κ-scheme successfully predicts most imminent large solar flares.
  • * A small number of confined flares were exceptions to the model's predictions.
  • * Magnetic twist flux density near polarity inversion lines is a key predictor.

Conclusions:

  • * The κ-scheme offers a physics-based approach to solar flare prediction.
  • * Magnetic twist flux density is a critical factor in determining solar flare characteristics.
  • * This research advances our understanding of solar flare mechanisms and forecasting.