Linked from

The 58 pages that link to Synchrotron radiation, each with the reason it gives.

• Radio astronomyRelated: It produces radio emission from sources such as supernova remnants and active galaxies.

• Supernova remnantRelated: Relativistic electrons in remnant magnetic fields produce much of its radio emission.

• Particle acceleratorRelated: Unintended radiation losses became a powerful tool for imaging and materials research.

• PulsarRelated: Relativistic particles in pulsar magnetospheres produce nonthermal radiation through magnetic-field-driven motion.

• Relativistic jetRelated: It produces much of the radio through X-ray emission observed from jets.

• PhotoionizationRelated: Its intense, adjustable photon energies enable detailed photoionization experiments.

• Gamma-ray burstRelated: It explains much of the broadband afterglow emission from burst shocks.

• Brookhaven National LaboratoryRelated: Brookhaven’s National Synchrotron Light Source II produces this radiation for experiments.

• Radio galaxyRelated: Relativistic electrons in radio-galaxy jets and lobes produce much of their radio emission this way.

• Crab NebulaRelated: It produces much of the Crab’s emission, from radio waves to high-energy light.

• Charged particleRelated: It carries energy away from particles forced onto curved trajectories.

• Doppler beamingRelated: It is a common jet emission mechanism whose observed strength is altered by beaming.

• Diamond anvil cellRelated: Its intense, focused X-rays enable diffraction from the cell’s minute sample.

• BlazarRelated: It produces much of a blazar’s radio-to-optical and X-ray emission.

• Stanford Linear Accelerator CenterRelated: SLAC converts accelerated electrons into intense light for research.

• SynchrotronRelated: The radiation is an energy loss in colliders and a powerful experimental resource in light sources.

• Centaurus ARelated: It produces much of the radio emission from Centaurus A’s jets and lobes.

• Small-angle X-ray scatteringRelated: Synchrotron beams enabled faster, more precise SAXS measurements on weakly scattering samples.

• PETRARelated: Bending the stored beams caused energy loss through synchrotron radiation, a key design constraint.

• Cassiopeia ARelated: Relativistic electrons in Cassiopeia A’s shocks produce its bright radio emission this way.

• Faraday rotationRelated: Its intrinsic polarization can be modified by Faraday rotation while crossing the emitting plasma.

• Interstellar magnetic fieldRelated: Its intensity and polarization reveal magnetized regions of the interstellar medium.

• Pulsar wind nebulaRelated: Relativistic electrons spiraling through nebular magnetic fields produce much of its observed light.

• X-ray absorption spectroscopyRelated: Its tunable, bright X-rays make energy-scanned measurements practical.

• Jupiter's magnetosphereRelated: Energetic electrons in Jupiter's radiation belts produce detectable radio emission.

• Crab PulsarRelated: Relativistic particles from the Crab Pulsar produce much of the nebula’s broadband glow this way.

• Messier 87Related: Synchrotron emission makes M87’s jet visible across radio and other wavelengths.

• Cygnus ARelated: This process produces most of the extended radio emission mapped around Cygnus A.

• 3C 273Related: Relativistic electrons in 3C 273's jet produce its strong radio and optical emission.

• Relativistic mechanicsRelated: Relativistic particle speeds concentrate this radiation into a narrow forward beam.

• Neutron imagingRelated: Synchrotron X-rays offer complementary contrast and resolution for materials also studied with neutrons.

• SN 1054Related: It explains much of the Crab Nebula's continuous radiation.

• Astrophysical jetRelated: It produces much of the radio and higher-frequency emission observed from jets.

• High-energy astrophysicsRelated: Its characteristic spectrum identifies relativistic electrons and magnetic fields in cosmic sources.

• Markarian 421Related: It produces the lower-energy component of Markarian 421’s broad emission spectrum.

• Markarian 501Related: Relativistic electrons in the jet produce much of the source’s radio-to-X-ray emission this way.

• Robert BrownRelated: It is a major mechanism behind radio emission in energetic Galactic-center sources.

• Accelerator applicationsRelated: Storage rings produce intense beams of X-rays for imaging and materials research.

• Accelerators & storage ringsRelated: Bending stored electrons produces bright radiation used for research.

• Astronomical radio sourceRelated: It produces radio emission in many supernova remnants, jets, and galaxies.

• Astrophysical X-ray sourceRelated: It explains nonthermal X-rays from jets and pulsar wind nebulae.

• Beam dynamics (accelerator physics)Related: Radiation drains energy and can damp or excite oscillations in electron beams.

• BL LacertaeRelated: It produces much of the source's broad-band emission from its relativistic jet.

• Cygnus LoopRelated: Radio emission from remnants can trace energetic electrons and magnetic fields.

• Gamma-ray burst emission mechanismsRelated: Relativistic electrons in burst outflows can produce broad prompt spectra this way.

• Polarization in astronomyRelated: Its polarized emission traces magnetic-field structure in many astronomical sources.