radiation$66417$ - traducción al español
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radiation$66417$ - traducción al español

USED TO SOLVE THE HELMHOLTZ EQUATION
Sommerfield radiation condition; Radiation condition; Radiation conditions

radiation      
n. radiación, irradiación
background radiation         
  • gamma radiation]] level is 9.8 [[μR/h]] (0.82 mSv/a) This is very close to the world average background radiation of 0.87 mSv/a from cosmic and terrestrial sources.
  • Displays showing ambient radiation fields of 0.120–0.130 μSv/h (1.05–1.14 mSv/a) in a nuclear power plant. This reading includes natural background from cosmic and terrestrial sources.
  •  access-date=2008-02-19}}</ref>
LEVEL OF IONIZING RADIATION PRESENT IN THE NATURAL ENVIRONMENT
Background Radiation; Natural radioactivity; Terrestrial radiation; Natural radiation; Background count; Natural background radiation; Environmental radiation; Radiation background; Ambient radiation
radiación de fondo (radiación débil sobre la tierra)
thermal radiation         
  • Thermal radiation in visible light can be seen on this hot metalwork. Its emission in the [[infrared]] is invisible to the human eye. [[Infrared cameras]] are capable of capturing this infrared emission (see [[Thermography]]).
  • National Research Council]], near [[Ottawa]], [[Ontario]], Canada
  • Spectral response of two paints and a mirrored surface, in the visible and the infrared. From NASA.
ELECTROMAGNETIC RADIATION GENERATED BY THE THERMAL MOTION OF CHARGED PARTICLES IN MATTER
Radiant heat; Heat radiator; Thermal radiator; Thermal Radiation; Thermal light; Heat radiation; Radiative heat transfer; Radiation of heat; Thermal emission; Radiation heat transfer; Radiation properties
Radiación térmica

Definición

synchrotron radiation
¦ noun Physics polarized radiation emitted by a charged particle spinning in a magnetic field.

Wikipedia

Sommerfeld radiation condition

In applied mathematics, the Sommerfeld radiation condition is a concept from theory of differential equations and scattering theory used for choosing a particular solution to the Helmholtz equation. It was introduced by Arnold Sommerfeld in 1912 and is closely related to the limiting absorption principle (1905) and the limiting amplitude principle (1948).