Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-14T06:42:02.558Z Has data issue: false hasContentIssue false
  • English
  • Français

Impact of Pulsar Giant Pulses on Distant Clocks Comparison

Published online by Cambridge University Press:  21 October 2010

Yury P. Ilyasov ,
Vladimir E. Zharov  and
M. Sekido
Yury P. Ilyasov
Affiliation:
Pushchino Radio Astronomical Observatory of P.N. Lebedev Physical Institute of the Russian academy of science, Pushchino, Moscow region, Russia email: ilyasov@prao.ru
Vladimir E. Zharov
Affiliation:
Department of Physics, Moscow State University, Moscow, Russia email: zharov@sai.msu.ru
M. Sekido
Affiliation:
National Institute of Information and Communications Technology Kashima, Japan email: sekido@nict.go.jp
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

New method of precise clocks comparison based on observation and registration of giant pulses of the millisecond pulsars is discussed. It was shown that expected accuracy of comparison is about 0.2–2 ns and depends on uncertainty of delay in the Earth ionosphere and troposphere.

Keywords

Pulsarstime transfergiant pulses
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 232
Copyright
Copyright © International Astronomical Union 2010

References

Hankins, T. H. & Eilek, J. A. 2007, ApJ, 670, 693CrossRefGoogle Scholar
Popov, M., Soglasnov, A., et al. 2008, J.Astr, 85, 1Google Scholar
Ilyasov, Yu., Kuzmin, A., et al. 1991, Technique of clocks synchronization by pulsars signals, Patent (Soviet Union) No 1669301Google Scholar
Ilyasov, Yu, Oreshko, V., et al. 2007, Proc. of the IAA RAS (St. Petersburg), 17, 128Google Scholar