On scattering of Giant Pulses from the Crab Pulsar: a Scattering Function
Alexander A. Ershov (Pushchino Radio Astronomy Observatory, ASC, LPI)

TL;DR
This study analyzes the scattering of giant pulses from the Crab pulsar using simultaneous dual-frequency observations, revealing that the scattering occurs at a thick screen rather than a thin one, which impacts understanding of pulsar signal propagation.
Contribution
It provides new evidence that scattering of Crab pulsar's giant pulses occurs at a thick screen, challenging previous thin-screen models.
Findings
Scattering occurs at a thick screen.
Simultaneous dual-frequency observations were conducted.
Implications for pulsar signal propagation models.
Abstract
Simultaneous dual-frequency observations of giant pulses from the Crab pulsar were performed at the frequencies of 61 and 111 MHz. It is shown that scattering of giant pulses from the Crab pulsar occurs at thick, and not at thin screen.
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Taxonomy
TopicsGeophysics and Sensor Technology · Pulsars and Gravitational Waves Research · Geophysics and Gravity Measurements
