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Interstellar Scattering: Observations and Interpretations
Published online by Cambridge University Press: 12 April 2016
Abstract
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The successful theory for radio propagation through the interstellar plasma is reviewed, where the density spectrum follows the Kolmogorov model. However, there are also several observations indicating more refraction than expected. A particular model of enhanced refraction is proposed in which isolated regions of the warm ionized medium support filaments of enhanced density on a scale of 1 AU, which do not couple to a turbulent cascade.
- Type
- Part 6 Winds and the ISM
- Information
- International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 439 - 446
- Copyright
- Copyright © Astronomical Society of the Pacific 1996
References
Cordes, J.M., Wolszczan, A., Dewey, R.J., Blaskiewicz, M., Stinebring, D.R., 1990, ApJ, 349, 245
Google Scholar
Cordes, J.M., Weisberg, J.M., Frail, D.A., Spangler, S.R., Ryan, M., 1991, Nature, 354, 121
Google Scholar
Ewing, M.S., Batchelor, R.A., Friefeld, R.D., Price, R.M., Staelin, D.H., 1970, ApJ, 162, L169
Google Scholar
Gwinn, C., Ojeda, M., Brotton, M., Reynolds, J., Jauncey, D., King, E., Flanagan, C., Smits, D., Preston, R., Jones, D., 1996, this volumeGoogle Scholar
Lo, K.Y., Backer, D.C., Ekers, R.D., Kellerman, K.I., Reid, M., Moran, J.M., 1985, Nature, 249, 504
Google Scholar
Spangler, and Cordes, , 1988, Radiowave Scattering in the Interstellar Medium, AIP Conf. Proc, 174, p66
Google Scholar