Radio Observations of the Pulse Profiles and Dispersion Measures of Twelve Pulsars |
Common terms and phrases
analog-digital converter antenna appears Arecibo Observatory assumed average pulse profile average pulse shapes bandwidth behavior class 2 period Comella components constant correlation corresponding Crab Nebula decreasing radio frequency detected Dirac comb discussed drift Eastlund effect electron content emission profile emission regions estimates filter frequency dependence group delay Hewish histogram individual pulses interpulse interstellar interstellar medium interval ionosphere limits linear magnetic field main pulse MHz pulse microseconds milliseconds Milliseconds Figure Nature neutron star number of pulses observed operational amplifiers parsecs polarization pulsar period pulsar pulse pulse arrival pulse delays pulse energy pulse intensity pulse structure pulse to pulse pulse width pulsed emission pulses from CP pulses shown quency radiation receiver bandwidth relatively resolution rotation sampling sars scan seen separation shown in Figure single pulse smearing stability subpulse suggested sweep rate Table techniques thesis white dwarf Zeissig