Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-23T20:37:10.271Z Has data issue: false hasContentIssue false

80 MHz Observations of the Coronal Broadening of the Crab Nebula

Published online by Cambridge University Press:  25 April 2016

J. R. Harries
Affiliation:
Department of Physics, University of Adelaide
R. G. Blesing
Affiliation:
Department of Physics, University of Adelaide
P. A. Dennison
Affiliation:
Department of Physics, University of Adelaide

Extract

Regions of the interplanetary medium currently inaccessible to space vehicles may conveniently be studied using the radio scattering properties of the interplanetary plasma. These effects may give rise to angular broadening of radio sources sufficiently close to the Sun, or to amplitude scintillation of sources of small angular size.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1970

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. and Wyndham, J. D., MNRAS, 126, 469 (1963).Google Scholar
2 Slee, O. B., Aust. J. Phys., 12, 134 (1959).CrossRefGoogle Scholar
3 Erickson, W. C., Ap. J., 139, 1290 (1963).CrossRefGoogle Scholar
4 Dennison, P. A. and Hewish, A., Nature, 213, 343 (1967).CrossRefGoogle Scholar
5 Dennison, P. A., Planet Space Sci., 17, 189 (1969).CrossRefGoogle Scholar
6 Wild, J. P. et al., ProcIREE Aust., 28, No. 9 (1967).Google Scholar