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Paper detail

Preliminary results of giant pulse investigations from Crab pulsar with Radioastron

Giant pulses from Crab pulsar were observed together with Radioastron space radiotelescope, Global EVN radio telescopes and Kvazar-KVO VLBI stations to study the scattering effects in the ISM. Five observing sessions were conducted at 18 cm (EVN codes: EG060A, EG060B, EG067B, EG075) and one at 92 cm (EVN code: GS033A). We have estimated distance to the scattering screen, angular size of scattering disk, scattering time. All estimations were done in an assumption of single thin scattering screen. Also, a significant change in the shape of cross-correlation functions for space-ground baselines was found (starting from 4 up to 12 Earth diameters).

preprint2015arXivOpen access
Alexey RudnitskiyMikhail PopovVladimir Soglasnov
astro-ph.IMastro-ph.SR
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Alexey RudnitskiyMikhail PopovVladimir Soglasnov

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