|V|: New insight into the circular polarization of radio pulsars

We present a study of single pulses from nine bright northern pulsars to investigate the behaviour of circular polarisation, V. The observations were conducted with the Effelsberg 100-m radio telescope at 1.41 GHz and 4.85 GHz and the Westerbork radio telescope at 352 MHz. For the first time, we pre...

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Main Authors: Karastergiou, A, Johnston, S, Mitra, D, Leeuwen, A, Edwards, RT
Format: Journal article
Published: 2003
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author Karastergiou, A
Johnston, S
Mitra, D
Leeuwen, A
Edwards, RT
author_facet Karastergiou, A
Johnston, S
Mitra, D
Leeuwen, A
Edwards, RT
author_sort Karastergiou, A
collection OXFORD
description We present a study of single pulses from nine bright northern pulsars to investigate the behaviour of circular polarisation, V. The observations were conducted with the Effelsberg 100-m radio telescope at 1.41 GHz and 4.85 GHz and the Westerbork radio telescope at 352 MHz. For the first time, we present the average profile of the absolute circular polarisation |V| in the single pulses. We demonstrate that the average profile of |V| is the distinguishing feature between pulse components that exhibit low V in the single pulses and components that exhibit high V of either handedness, despite both cases resulting in a low mean. We also show that the |V| average profile remains virtually constant with frequency, which is not generally the case for V, leading us to the conclusion that |V| is a key quantity in the pulsar emission problem.
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spelling oxford-uuid:233ee387-5aa1-4924-885a-06ce9549d4192022-03-26T11:43:19Z|V|: New insight into the circular polarization of radio pulsarsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:233ee387-5aa1-4924-885a-06ce9549d419Symplectic Elements at Oxford2003Karastergiou, AJohnston, SMitra, DLeeuwen, AEdwards, RTWe present a study of single pulses from nine bright northern pulsars to investigate the behaviour of circular polarisation, V. The observations were conducted with the Effelsberg 100-m radio telescope at 1.41 GHz and 4.85 GHz and the Westerbork radio telescope at 352 MHz. For the first time, we present the average profile of the absolute circular polarisation |V| in the single pulses. We demonstrate that the average profile of |V| is the distinguishing feature between pulse components that exhibit low V in the single pulses and components that exhibit high V of either handedness, despite both cases resulting in a low mean. We also show that the |V| average profile remains virtually constant with frequency, which is not generally the case for V, leading us to the conclusion that |V| is a key quantity in the pulsar emission problem.
spellingShingle Karastergiou, A
Johnston, S
Mitra, D
Leeuwen, A
Edwards, RT
|V|: New insight into the circular polarization of radio pulsars
title |V|: New insight into the circular polarization of radio pulsars
title_full |V|: New insight into the circular polarization of radio pulsars
title_fullStr |V|: New insight into the circular polarization of radio pulsars
title_full_unstemmed |V|: New insight into the circular polarization of radio pulsars
title_short |V|: New insight into the circular polarization of radio pulsars
title_sort v new insight into the circular polarization of radio pulsars
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AT johnstons vnewinsightintothecircularpolarizationofradiopulsars
AT mitrad vnewinsightintothecircularpolarizationofradiopulsars
AT leeuwena vnewinsightintothecircularpolarizationofradiopulsars
AT edwardsrt vnewinsightintothecircularpolarizationofradiopulsars