How Does Synchrotron Radiation Influence Observations in Radio Astronomy?

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Synchrotron radiation in radio astronomy is emitted by high-energy electrons spiraling in magnetic fields, with radiation concentrated in the direction of their motion. Observers can detect this radiation continuously because, despite the electrons' varied positions in their orbits, many are oriented towards Earth at any given time. The instantaneous motion of these electrons allows for consistent observation of their emissions. The vast number of electrons involved ensures that at least some are always aligned to emit radiation towards us. This phenomenon is crucial for understanding the dynamics of cosmic sources in radio astronomy.
shirin
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I read in radio astronomy book that radiation from high-energy electrons radiating synchrotron emision, is concentrated in the direction of its instantaneous motion. So if we see them, their orbital motion plane contains us(as observer). I am wondering if they have spiral motion in the related magnetic field, their orbital motion plane is moving instantaneously. So how are we observing their radiation continiously?
 
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There are a huge (real huge!) number of electrons all spiraling around the magnetic field and all in different points of their orbits. So there are always some pointing at us.
 
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