Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-27T11:57:27.718Z Has data issue: false hasContentIssue false

Pulsar Amplitude Variations

Published online by Cambridge University Press:  25 April 2016

R. Wielebinski*
Affiliation:
School of Electrical Engineering, University of Sydney

Extract

Pulsars display a complicated pattern of amplitude variations. The scale of variations range from months through hours to sub-milliseconds. The purpose of this note is to present polarization data for CP 1919 and intensity distribution data for PSR 0833—45 which are relevant to pulse-to-pulse variations and the variation over periods of hours respectively.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1969

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F. and Collins, R. A. Nature, 217, 709, (1968).Google Scholar
2 Wielebinski, R., Nature, 219, 1135 (1968).CrossRefGoogle Scholar
3 Craft, H. D. Jr., Comella, J. M. and Drake, F. D., Nature, 218, 1122 (1968).Google Scholar
4 Robinson, B. J., Cooper, B. F. C., Gardner, F. F., Wielebinski, R. and Landecker, T. L., Nature, 218, 1143 (1968).Google Scholar
5 Sheuer, P. A. G., Nature, 218, 920 (1968).CrossRefGoogle Scholar
6 Lovelace, R. V. E. and Craft, H. D. Jr., Nature, 220, 875 (1968).CrossRefGoogle Scholar
7 Large, M. I., Vaughan, A. E. and Wielebinski, R., Nature, 220, 753 (1968).Google Scholar
8 Ekers, R. D. and Moffet, A. T., Nature, 220, 756, (1968).CrossRefGoogle Scholar