Synchrotron Emission

Synchrotron emission is a type of radiation produced when charged particles, such as electrons, move at speeds close to the speed of light within a magnetic field. As these particles accelerate along curved paths, they emit energy in the form of electromagnetic waves, often observed as bright beams or jets in space. This process is common in astrophysical environments like active galaxies and pulsars, and it helps scientists study high-energy phenomena in the universe. The emitted light spans a wide range of wavelengths, including radio, visible, and X-rays, depending on the particle energies and magnetic field strength.