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magnetobremsstrahlung
magnetobremsstrahlung n. 
/mæɡˌnɛdoʊˈbrɛmˌʃtrɑləŋ/ [ < magneto- comb. form + bremsstrahlung n.] synchrotron radiation, esp. the cosmic radiation emitted by electrons moving at relativistic speeds in galaxies.
Brit. /maɡˌniːtə(ʊ)ˈbrɛmzˌʃtrɑːlʊŋ/
, /maɡˌniːtə(ʊ)ˈbrɛmzˌʃtrɑːlʊŋ/U.S. /mæɡˌnidoʊˈbrɛmˌʃtrɑləŋ/
, /mæɡˌnidoʊˈbrɛmˌʃtrɑləŋ//mæɡˌnɛdoʊˈbrɛmˌʃtrɑləŋ/ΘΚΠ
the world > matter > physics > quantum theory > quantum mechanics > wave mechanics > [noun] > radiation produced by retardation
bremsstrahlung1944
magnetobremsstrahlung1968
1968 Ann. Rev. Astron. & Astrophysics 6 321 This article is concerned with the radio spectra of sources..whose radio emission is generally attributed to synchrotron radiation (magnetobremsstrahlung).
1980 Nature 20 Mar. 247/1 A substantial fraction of its rotational energy losses is thought to be converted into magnetobremsstrahlung of the Crab nebula.
1992 S. P. Maran Astron. & Astrophysics Encycl. 598/1 Magnetobremsstrahlung (magnetic braking radiation), the incoherent emission of electrons spiraling in a magnetic field, is the most prevalent emission mechanism in cosmic radio sources.
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