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Biological Effects of Radiation02:59

Biological Effects of Radiation

All radioactive nuclides emit high-energy particles or electromagnetic waves. When this radiation encounters living cells, it can cause heating, break chemical bonds, or ionize molecules. The most serious biological damage results when these radioactive emissions fragment or ionize molecules. For example, α and β particles emitted from nuclear decay reactions possess much higher energies than ordinary chemical bond energies. When these particles strike and penetrate matter, they produce ions...
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...
Electric Flux01:15

Electric Flux

The concept of flux describes how much of something goes through a given area. More formally, it is the dot product of a vector field within an area. For a better understanding, consider an open rectangular surface with a small area that is placed in a uniform electric field. The larger the area, the more field lines go through it and, hence, the greater the flux; similarly, the stronger the electric field (represented by a greater density of lines), the greater the flux. On the other hand, if...
Calculation of Electric Flux01:25

Calculation of Electric Flux

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?
Magnetic Flux01:18

Magnetic Flux

The magnetic flux measures the number of magnetic field lines passing through a given surface area. The SI unit for magnetic flux is the weber (Wb). Magnetic flux is a scalar quantity. It depends on three factors: the strength of the magnetic field B, the area through which the field lines pass, and the relative orientation of the field with the surface area.
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
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.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...

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Related Experiment Video

Updated: May 9, 2026

Dosimetry for Cell Irradiation using Orthovoltage (40-300 kV) X-Ray Facilities
06:51

Dosimetry for Cell Irradiation using Orthovoltage (40-300 kV) X-Ray Facilities

Published on: February 20, 2021

A note on vector flux models for radiation dose calculations.

J W Kern1

  • 1Rockwell International Space Systems Division, Houston, TX 77058, USA.

Radiation Measurements
|January 1, 1994
PubMed
Summary

This study introduces new equations for modeling anisotropic proton fluxes in Earth's radiation belts. These models improve understanding of proton flux anisotropy and trapped proton lifetimes, crucial for space radiation studies.

Area of Science:

  • Space Physics
  • Plasma Physics
  • Atmospheric Science

Background:

  • Radiation belt protons exhibit anisotropic fluxes, particularly at higher energies.
  • Modeling these fluxes is complex due to atmospheric density variations with altitude.
  • Existing models often rely on data-based vector flux models.

Purpose of the Study:

  • To develop closed-form equations for vector proton fluxes and anisotropy.
  • To provide a flexible alternative to current data-based models.
  • To investigate the influence of atmospheric density on proton flux anisotropy.

Main Methods:

  • Review and extension of anisotropic flux modeling for radiation belt protons.
  • Derivation of equations relating vector flux to omnidirectional flux.

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A Computational Modeling Approach to Investigate the Influence of Hyperthermia on the Tumor Microenvironment
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A Computational Modeling Approach to Investigate the Influence of Hyperthermia on the Tumor Microenvironment

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Last Updated: May 9, 2026

Dosimetry for Cell Irradiation using Orthovoltage (40-300 kV) X-Ray Facilities
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Published on: February 20, 2021

Irradiator Commissioning and Dosimetry for Assessment of LQ α and β Parameters, Radiation Dosing Schema, and in vivo Dose Deposition
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Irradiator Commissioning and Dosimetry for Assessment of LQ α and β Parameters, Radiation Dosing Schema, and in vivo Dose Deposition

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  • Calculation of trajectory-averaged atmospheric densities and scale heights.
  • Main Results:

    • Closed-form equations for vector proton fluxes and anisotropy were developed.
    • Trajectory-averaged scale heights were found to be 10-20% higher than standard models for low-altitude mirroring protons.
    • Calculated trapped proton lifetimes provide time-averaging intervals for equilibrium models.

    Conclusions:

    • The new equations offer a flexible modeling approach for radiation belt proton fluxes.
    • Atmospheric density variations significantly impact proton flux anisotropy, especially in the South Atlantic Anomaly.
    • The study provides a pathway to improved equilibrium models for trapped proton fluxes and their lifetimes.