Context. LOFAR offers the unique capability of observing pulsars across the 10−240 MHz frequency range with a fractional bandwidth of roughly 50%. This spectral range is well suited for studying the frequency evolution of pulse profile morphology caused by both intrinsic and extrinsic effects such as changing emission altitude in the pulsar magnetosphere or scatter broadening by the interstellar medium, respectively.
No takes yet. Share an insight, caveat, or question.
A 2015 study studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: