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Related Concept Videos

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 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...
Nuclear Power02:36

Nuclear Power

Controlled nuclear fission reactions are used to generate electricity. Any nuclear reactor that produces power via the fission of uranium or plutonium by bombardment with neutrons has six components: nuclear fuel consisting of fissionable material, a nuclear moderator, a neutron source, control rods, reactor coolant, and a shield and containment system.
Nuclear Fuels
Nuclear fuel consists of a fissile isotope, such as uranium-235, which must be present in sufficient quantity to provide a...
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...
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

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. Nichols...

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Updated: May 18, 2026

Effective Analysis of Human Exposure Conditions with Body-worn Dosimeters in the 2.4 GHz Band
06:43

Effective Analysis of Human Exposure Conditions with Body-worn Dosimeters in the 2.4 GHz Band

Published on: May 2, 2018

Space radiation protection issues.

Amy Kronenberg1, Francis A Cucinotta

  • 1Life Sciences Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA. a_kronenberg@lbl.gov

Health Physics
|October 4, 2012
PubMed
Summary
This summary is machine-generated.

Space radiation, including solar particle events and galactic cosmic radiation, presents significant health risks for astronauts. Further research is crucial to reduce uncertainties in cancer and non-cancer late effects for improved space mission safety.

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Area of Science:

  • Space science
  • Astrobiology
  • Radiation biology

Background:

  • Space radiation environments, composed of charged particles, pose significant health risks impacting space mission design and crew selection.
  • Uncertainties regarding the biological effects of various ions, both individually and in combination, are a major concern for astronaut health, particularly for late effects like cancer and non-cancer diseases.

Purpose of the Study:

  • To introduce the principal issues concerning space radiation protection.
  • To highlight the need for reducing uncertainties in understanding the biological impacts of space radiation.

Main Methods:

  • This paper reviews the primary components of space radiation: Solar Particle Events (SPE) and Galactic Cosmic Radiation (GCR).
  • It addresses the composition of SPE (primarily low- to moderate-energy protons) and GCR (broader proton energy range, plus light and heavy ions).

Main Results:

  • Space radiation comprises two main components: Solar Particle Events (SPE) and Galactic Cosmic Radiation (GCR).
  • SPE are sporadic and proton-dominated, while GCR is isotropic, less variable, and includes a wider range of ions.
  • Both SPE and GCR contribute to health risks, with GCR posing additional concerns due to its diverse ion composition.

Conclusions:

  • Understanding the complex charged particle environments in space is essential for astronaut health and mission planning.
  • Reducing the high uncertainties in the biological effects of space radiation is a high priority for ensuring crew safety.