Author pages are created from data sourced from our academic publisher partnerships and public sources.
- Publications
- Influence
Toward an empirical theory of pulsar emission. I: Morphological taxonomy
- J. M. Rankin
- Physics
- 1 November 1983
Pulsar polarization fluctuations. I. 1404 MHz statistical summaries.
- D. R. Stinebring, J. Cordes, J. M. Rankin, J. M. Weisberg, V. Boriakoff
- Physics
- 1 June 1984
Observations de polarisation des pulsations individuelles des 11 pulsars PSR 0525+21, PSR 0823+26, PSR 0834+06 a , PSR 0919+06, PSR 0950+08 a , PSR 1133+16, PSR 1237+25, PSR 1929+10 a , PSR 1944+17,… Expand
Toward an empirical theory of pulsar emission. II: On the spectral behavior of component width
- J. M. Rankin
- Physics
- 1 November 1983
The Crab Nebula pulsar - Variability of dispersion and scattering
- R. Isaacman, J. M. Rankin
- Physics
- 15 May 1977
Previous investigations of the effects of interstellar dispersion and scattering on the waveform of the Crab Nebula pulsar (NP 0532) have indicated a two-screen scattering model with one variable… Expand
Pulsar Polarization Fluctuations - Part One - 1404-MHZ Statistical Summaries
- D. R. Stinebring, J. Cordes, J. M. Weisberg, J. M. Rankin, V. Boriakoff
- Physics
- 1 June 1984
On a effectue des observations de polarisation de pulsations individuelles a 800 MHz pour quatre pulsars et a faible dispersion: PSR 0834+06, PSR 0950+08, PSR 1929+10 et PSR 2020+28
Statistical summaries of polarized pulsar radiation.
- D. Backer, J. M. Rankin
- Physics
- 1980
This paper considers the polarization behavior of 18 pulsars as observed at 430 MHz in the Arecibo Polarization Survey. The results following from a statistical analysis are presented as probability… Expand
Pulsar polarization: weak sources and emission features at 430 MHz.
- J. M. Rankin, J. Benson
- Physics
- 1 March 1981
Further observations of the binary pulsar PSR 1913+16.
- J. Taylor, R. Hulse, L. A. Fowler, G. Gullahorn, J. M. Rankin
- Physics
- 15 May 1976
We report the results of more than a year's timing observations of the binary pulsar PSR 1913+16. Within the accuracy of our measurements, about +- 300 ..mu..s, the pulse arrival times are exactly… Expand
Four-Stokes-parameter radiofrequency polarimetry of a flare from AD Leonis
- S. Spangler, J. M. Rankin, S. Shawhan
- Physics
- 1 July 1974
Observations of the four Stokes parameters of a 430-MHz flare from the UV Ceti-type star AD Leo are presented. The maximum amplitude of the event was 0.52 flux units, and the durations at one-half… Expand
Orthogonal mode emission in geometric models of pulsar polarisation
- D. Backer, J. M. Rankin, D. Campbell
- Physics
- Nature
- 1 September 1976
The varying incidence of orthogonal ‘states’ of linear polarisation across the pulse of PSR 2016+28 is discussed in terms of a model with subpulse beams drifting round the pole of a rotating magnetic… Expand