Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-30T03:32:33.099Z Has data issue: false hasContentIssue false

Simple Formula for Radio Jet Surface Brightness

Published online by Cambridge University Press:  14 August 2015

R. N. Henriksen*
Affiliation:
Institute for Plasma Research Stanford University

Extract

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.

Henriksen, Bridle and Chan (1981; HBC) have proposed that the energy for the synchrotron emission of radio jets is derived ultimately from the turbulent hydrodynamic eddy cascade between the Taylor wave number, kT, and the Kolmogorov wave number. This cascade is established during the development of a turbulent jet by the shearing action of large-scale vortical entrainment of ambient material (Brown & Roshko, 1974).

Type
Research Article
Copyright
Copyright © Reidel 1982 

References

Bridle, A. H., Chan, K. L., Heinriksen, R. N. 1981, J.R.A.S.C., 75.Google Scholar
Brown, G. L., and Roshko, A. 1974, J. Fluid Mech., 64, 775.Google Scholar
Eilek, Jean A. 1979, Ap. J. 230, 373.Google Scholar
Eilek, Jean A., and Henriksen, R. N. 1982, this volume, p. 233.Google Scholar
Henriksen, R. N., Bridle, A. H., Chan, K. L. 1981, Ap. J. submitted and SUIPR report #844, Inst. for Plasma Research, Stanford University.Google Scholar
Lacombe, Catherine, 1979, Astronomy and Astrophysics 71. 169.Google Scholar
Willis, A. G., et al. 1981, Astronomy and Astrophysics, submitted.Google Scholar