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Jets and hotspots are the usual sources of high-frequency synchrotron emission.
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In the rapidly expanding blast wave of the supernova, energetic electrons produced synchrotron emission.
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How does Io help to modulate the synchrotron emission from the Jovian radiation belt in which it lives?
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The radio emission from radio-loud active galaxies is synchrotron emission, as inferred from its very smooth, broad-band nature and strong polarization.
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Fast particles spiralling in a magnetic field generate a kind of light, what astronomers call 'synchrotron emission', which displays a characteristic pattern of polarisation.
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Based on some first CMB maps showing the faint synchrotron emission, the project sought to also provide reliable ones for the coming two years.
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Extremely energetic electrons within the shock wave are accelerated by strong local magnetic fields and radiate as synchrotron emission across most of the electromagnetic spectrum.
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Astronomers working on the GIANT RADIO HALOS project calculated for the first time the re-acceleration of cosmic ray electrons and their synchrotron emission from first principles.
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The outflowing relativistic wind from the neutron star generates synchrotron emission, which produces the bulk of the emission from the nebula, seen from radio waves through to gamma rays.
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Radio waves coming from the planet Jupiter are electromagnetic phenomena generated by synchrotron emission mechanism, due to the interaction of Jovian magnetic field with charged particles produced by the satellite Io.
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Researchers performed a case-by-case analysis of several PWNe, showing that the emission from these sources can be very well modelled assuming that they are evolved PWNe in which the magnetic field has now decreased, thus suppressing the synchrotron emission.
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Moreover, there is no way to determine the energy densities in particles and magnetic fields from observation: the same synchrotron emissivity may be a result of a few electrons and a strong field, or a weak field and many electrons, or something in between.
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For example, in radio astronomy they are used to show the emission from synchrotron radiation, free-free emission and other emission mechanisms.
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Again, polarization and continuum spectrum are used to distinguish the synchrotron radiation from other emission processes.
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In general, the synchrotron theory of the decimeter emission from Jupiter is confirmed.
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The radio emission is due to the synchrotron process.
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The SHALOM team explored the scenario in which the observed emission is dominated by synchrotron radiation from electrons accelerated at the shock and radiating in the presence of amplified electric fields.
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He found that the light from the Crab Nebula was polarized, and produced by synchrotron emission. [edit] Honors
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If, on the other hand, the particles are relativistic, the emission is called synchrotron emission.
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It comes from the region surrounding the galactic centre and looks like a form of energy called synchrotron emission.
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Not all objects however are energetic enough to produce synchrotron emission and in these cases other mechanisms are utilised.
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Taking into consideration the reabsorption of synchrotron radiation by the electrons themselves, NEWEVLA astronomers modelled the radio emission to estimate the average expansion velocity.
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Among the many possibilities LOFAR observation, is being able to track the radio synchrotron emission of low energy cosmic rays in weak magnetic fields.
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Synchrotron emission associated with the Galactic Haze seen by Planck exhibits distinctly different characteristics from the synchrotron emission seen elsewhere in the Milky Way.
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The curiosity is that the synchrotron emission associated with the galactic haze exhibits different characteristics from the synchrotron emission seen elsewhere in the Milky Way.
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50 sinne gevind in 15 ms. Hulle kom uit baie bronne en word nie nagegaan nie.