Zobrazeno 1 - 10
of 24
pro vyhledávání: '"McKinnon, Mark M."'
Autor:
Bera, Apurba, James, Clancy W., McKinnon, Mark M., Ekers, Ronald D., Dial, Tyson, Deller, Adam T., Bannister, Keith W., Glowacki, Marcin, Shannon, Ryan M.
Fast radio bursts (FRBs) are highly energetic events of short-duration intense radio emission, the origin of which remains elusive till date. Polarization of the FRB signals carry information about the emission source as well as the magneto-ionic med
Externí odkaz:
http://arxiv.org/abs/2411.14784
Autor:
McKinnon, Mark M.
Publikováno v:
Astrophys.J.692:459-469,2009
A variety of intriguing polarization patterns are created when polarization observations of the single pulses from radio pulsars are displayed in a two-dimensional projection of the Poincare sphere. In many pulsars, the projections produce two cluste
Externí odkaz:
http://arxiv.org/abs/0810.4135
Autor:
McKinnon, Mark M.
Publikováno v:
Astrophys.J. 645 (2006) 551-555
A statistical model of the polarization of pulsar radio emission is used to derive the general statistics of a polarization vector's orientation angles. The theoretical distributions are compared with orientation angle histograms computed from single
Externí odkaz:
http://arxiv.org/abs/astro-ph/0603446
Autor:
McKinnon, Mark M.
Publikováno v:
Astrophys.J. 606 (2004) 1154-1166
The polarization position angles (PA) of pulsar radio emission occupy a distribution that can be much wider than what is expected from the average linear polarization and the off-pulse instrumental noise. Contrary to our limited understanding of the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0401598
Autor:
McKinnon, Mark M.
The measurement of radio polarization may be regarded as a three-dimensional statistical problem because the large photon densities at radio wavelengths allow the simultaneous detection of the three Stokes parameters which completely describe the rad
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306063
Autor:
McKinnon, Mark M.
Publikováno v:
Astrophys.J. 590 (2003) 1026-1034
Polarization observations of the radio emission from PSR B2016+28 at 1404 MHz reveal properties that are consistent with two, very different, interpretations of the pulsar's viewing geometry. The pulsar's average polarization properties show a rapid
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306071
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Astrophysical Journal; 8/ 1/1998, Vol. 502 Issue 2, p883-897, 15p
Autor:
McKinnon, Mark M.
Publikováno v:
The Astrophysical Journal; March 2002, Vol. 568 Issue: 1 p302-311, 10p
Publikováno v:
The Astrophysical Journal; January 2000, Vol. 529 Issue: 1 p435-446, 12p