Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-28T00:21:05.050Z Has data issue: false hasContentIssue false

Cosmic Ray Astronomy at Hobart

Published online by Cambridge University Press:  25 April 2016

R. M. Jacklyn*
Affiliation:
Antarctic Division, Melbourne and University of Tasmania, Hobart

Extract

In the field of cosmic ray galactic studies, two kinds of phenomenon are currently being investigated by members of the Hobart cosmic ray group, led by Dr. A. G. Fenton. In a combined project with the University of South Australia, the University of Tasmania is participating in an experiment whose aim is to locate sources of galactic X-rays in a part of the southern sky inaccessible from the northern hemisphere. The object of the other investigation, which forms part of a joint ANARE-University programme of cosmic ray research, is to elucidate the evidence for intensity maxima from fixed galactic directions in the otherwise isotropic charged primary radiation.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1967

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 Jacklyn, R. M., Symposium: Radio and Optical Studies of the Galaxy, Stromlo, Mt. (1966).Google Scholar
2 Jacklyn, R. M., Nature 111, 690 (1966).Google Scholar