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Parkes observations for project P1031 semester 2019OCTS_01

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Parkes observations for project P1031 semester 2019OCTS_01


We propose to study the pulsar emission mechanism using novel statistical methods that enable us to study the dynamics of the radio pulsar signal on short time scales (e.g. quasi-periodic sub-pulse structure, transitions between orthogonally polarized modes of emission, nulling, etc.) without needing to detect individual pulses. This pilot study w... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5db02c185f645


01 Oct 2019


31 Mar 2020


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CSIROEnquiries@csiro.au
1300 363 400

pulsars neutron stars P1031_2019OCTS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Primak, Natalia; van Straten, Willem; Tiburzi, Caterina; Parthasarathy, Aditya (2019): Parkes observations for project P1031 semester 2019OCTS_01. v1. CSIRO. Data Collection. https://doi.org/10.25919/5db02c185f645


All Rights (including copyright) CSIRO 2019.


Access to this collection's metadata and/or files (if any) are restricted until 30 Sep 2021.

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More about this Collection

ivo://au.csiro.atnf/P1031-2019OCTS_01


About this Project

Australia Telescope National Facility


P1031 - A pilot study to demonstrate novel radio pulsar emission analysis techniques


Pulsars emit light-house like beams of radio waves that sweep across the Galaxy with each rotation of the star. Unlike a steady search beam, the pulsar beam crackles and pops with lightning-like discharges of energy. By studying these discharges, we learn more about what generates the pulsar signal and the physics of the turbulent plasma in the p... more


Observation


Parkes


Natalia Primak


Willem van Straten


Caterina Tiburzi


Aditya Parthasarathy


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