Skip to main content
Log in

Type I Radio Bursts Deflected by Lower Hybrid Waves

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

What are the observational effects if type I bursts are deflected by lower-hybrid waves? The deflection creates an elliptical radio mirage, with the direct source at one end of the minor axis. Unlike a ‘scattering disk’, the mirage has considerable polarization structure which should be observable at high angular resolution. The lower-hybrid waves have four attractive features to explain existing observations of type I bursts: they naturally yield zero polarization for limb bursts; they preserve a high directivity even for limb bursts; they can explain the observed constancy of polarization during partially polarized bursts; and they depolarize at a sufficient height so that the resulting two circular polarizations arrive nearly simultaneously, as observed. The small time interval between the arrival of the two polarizations requires that we normally observe only the mirage and that the source be asymmetric with respect to azimuth around the magnetic field. The waves appear to be restricted to the vicinity of type I sources.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Bastian, T. S.: 1994, Astrophys. J. 426, 774.

    Article  Google Scholar 

  • Bastian, T. S.: 1995, Astrophys. J. 439, 494.

    Google Scholar 

  • Benz, A. O.: 1996, private communication.

  • Benz, A. O. and Pianezzi, P.: 1997, Astron. Astrophys., in press.

  • Benz, A. O. and Wentzel, D. G.: 1980, Astron. Astrophys. 94, 100.

    Google Scholar 

  • Caroubalos, C. and Steinberg, J. L.: 1974, Astron. Astrophys. 32, 245.

    Google Scholar 

  • Huba, J. D., Gladd, N. T., and Papadopoulos, K: 1978, J. Geophys. Res. 83, 5217.

    Google Scholar 

  • James, J. C.: 1970, Solar Phys. 12, 143.

    Google Scholar 

  • Krucker, S., Benz, A. O., Aschwanden, M. J., and Bastian, T. S.: 1995, Solar Phys. 160, 151.

    Google Scholar 

  • Melrose, D. B.: 1980, Plasma Astrophysics, Gordon and Breach, New York.

    Google Scholar 

  • Melrose, D. B.: 1989, Solar Phys. 119, 143.

    Google Scholar 

  • Steinberg, J. L, Caroubalos, C., and Bougeret, J. L.: 1974, Astron. Astrophys. 37, 109.

    Google Scholar 

  • Tsytovich, V. N.: 1970, Nonlinear Effects in Plasma, transl. M. Hamberger, Plenum Press, New York.

    Google Scholar 

  • Vlahos, L., Gergely, T. E., and Papadopoulos, K.: 1982, Astrophys. J. 258, 812.

    Article  Google Scholar 

  • Wentzel, D. G.: 1981a, Astrophys. J. 248, 1132.

    Article  Google Scholar 

  • Wentzel, D. G.: 1981b, Astron. Astrophys. 100, 20.

    Google Scholar 

  • Wentzel, D. G.: 1983, Astrophys. J. 270, 250.

    Article  Google Scholar 

  • Wentzel, D. G.: 1997, Solar Phys. 175, 191 (this issue).

    Article  Google Scholar 

  • Wentzel, D. G., Zlobec, P., and Messerotti, M.: 1986, Astron. Astrophys. 159, 40.

    Google Scholar 

  • Zlobec, P., Koren, U., and Messerotti, M.: 1982, in A. O. Benz and P. Zlobec (eds.), Proc. Solar Noise Storms, Trieste Observatory, p. 89.

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Wentzel, D.G. Type I Radio Bursts Deflected by Lower Hybrid Waves. Solar Physics 175, 175–189 (1997). https://doi.org/10.1023/A:1004912522778

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1023/A:1004912522778

Keywords

Navigation