The role of turbulence of the relativistic electron-positron plasma in generating in the prepulses of the Crab radio pulsar Academic Article uri icon

abstract

  • to be regarded as filled with electrons and positrons moving along open magnetic field lines at relativistic velocities. I~ n the case of the Crab Nebula pulsar, NP 0531+ 21,

publication date

  • April 1, 1982