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Maser Pulse Emission Mechanisms

Published online by Cambridge University Press:  14 August 2015

D. B. Melrose
D. B. Melrose*
Affiliation:
School of Physics, University of Sydney, NSW, 2006, Australia

Abstract

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The difficulties with “coherent” curvature emission by bunches of electrons formed through a streaming instability suggest that it cannot account for the observed radio emission for existing polar-cap models of pulsars. Amongst alternative maser mechanisms, that involving acceleration emission due to the electric fields in the waves generated by the bunching instability can account for the gross properties of the observed emission, provided that the relativistic electrons have γ ≤ 10 in the wave frame.

Type
II. Radio Emission Mechanism
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 133 - 140
Copyright
Copyright © Reidel 1981 

References

Benford, G. and Buschauer, R.: 1977, Mon. Not. Roy. Astron. Soc. 179, 189.Google Scholar
Blandford, R. D.: 1975, Mon. Not. Roy. Astron. Soc. 170, 551.Google Scholar
Cheng, A. F. and Ruderman, M. A.: 1977, Astrophys. J. 212, 800.Google Scholar
Cheng, A. F. and Ruderman, M. A.: 1980, Astrophys. J. 235, 576.Google Scholar
Chiu, H. Y. and Canuto, V.: 1971, Astrophys. J. 163, 577.Google Scholar
Cocke, W. J.: 1973, Astrophys. J. 184, 291.Google Scholar
Cordes, J.: 1978, Astrophys. J. 222, 1006.Google Scholar
Cox, J.: 1979, Astrophys. J. 229, 734.Google Scholar
Goldreich, P. and Keeley, D. A.: 1971, Astrophys. J. 170, 463.Google Scholar
Hardee, P. E. and Morrison, P.: 1979, Astrophys. J. 227, 252.Google Scholar
Hardee, P. E. and Rose, W. K.: 1976, Astrophys. J. 210, 533.Google Scholar
Hinata, S.: 1976a, Astrophys. J. 203, 223.CrossRefGoogle Scholar
Hinata, S.: 1976b, Astrophys. Space Sci. 44, 389.Google Scholar
Jackson, E. A.: 1976, Astrophys. J. 206, 831.Google Scholar
Kaplan, S. A. and Tsytovich, V. N.: 1973, Plasma Astrophysics, Pergamon Oxford Google Scholar
Kawamura, K. and Suzuki, I.: 1977, Astrophys. J. 217, 832.Google Scholar
Komesaroff, M. M.: 1970, Nature 225, 612.Google Scholar
Kroll, N. M. and McMullin, W. A.: 1979, Astrophys. J. 231, 425.Google Scholar
Matese, J. J. and Whitmere, D. P.: 1980, Astrophys. J. 235, 587.Google Scholar
Melrose, D. B.: 1978, Astrophys. J. 225, 557.Google Scholar
Radhakrishnan, V.: 1969, Proc. Astron. Soc. Australia 1, 254.Google Scholar
Ruderman, M. A. and Sutherland, P. A.: 1975, Astrophys. J. 196, 51.Google Scholar
Rylov, Yu. A.: 1976, Soviet Astron. AJ 20, 23.Google Scholar
Rylov, Yu. A.: 1977, Astrophys. Space Sci. 51, 59.Google Scholar
Rylov, Yu. A.: 1978, Astrophys. Space Sci. 53, 377.Google Scholar
Sturrock, P. A.: 1971, Astrophys. J. 164, 529.Google Scholar
Sturrock, P. A., Petrosian, V. and Turk, J. V.: 1975, Astrophys. J. 196, 73.Google Scholar
Virtamo, J. and Jauho, P.: 1973, Astrophys. J. 182, 935.Google Scholar