radio wave

This well-known fringe pattern phenomenon is caused by consistent constructive interference but has different characteristics when radio waves propagate around a neutron star.

This will slowly come into view as the probe uses penetrating radio waves to peer beneath the icy crust — much like an X-ray machine.

Light that reaches our telescopes ranges in wavelength from long radio waves to energetic gamma rays.

The findings could make scientists reconsider their decades-old understanding of neutron stars or white dwarfs; how they emit radio waves and what their populations are like in our Milky Way galaxy.

The problem is that the standard codes used to simulate the plasma and radio wave interactions are very complicated and run too slowly to be used to make real-time decisions.