Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-23T19:12:25.315Z Has data issue: false hasContentIssue false
  • English
  • Français

Solar Burst Observations at Metre and Decametre Wavelengths

Published online by Cambridge University Press:  14 August 2015

D.J. McLean
D.J. McLean*
Affiliation:
Division of Radiophysics, CSIRO, Sydney, Australia

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.

Our success or failure in understanding solar bursts is largely determined by the kinds of instrument with which we observe them. For example, although the basic feature of Type II bursts, a slow drift from high to low frequencies, was recognized and correctly interpreted from radiometer measurements at a few frequencies (Payne-Scott et al., 1947) other properties of Type II bursts such as fundamental-harmonic structure, split bands and herringbone structure can only be recognized on dynamic spectrograms. For this review I have chosen to group together the observations made with a particular type of instrument. I have also tended to emphasize what remains to be done rather than what has already been done. Unfortunately, with so many topics to choose from my treatment can only be cursory; and in attempting to select the interesting topics I have inevitably been biased toward the work I know best - that is, the work of the group to which I belong.

Type
Session IV - Solar Bursts - Meter Wavelengths
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 223 - 233
Copyright
Copyright © Reidel 1980 

References

Aubier, M.G., Leblanc, Y., and Møller-Pedersen, B.: 1978, Astron. Astrophys. 70, p. 685.Google Scholar
Boischot, A.: 1958, Ann. Astrophys. 21, p. 273.Google Scholar
Bougeret, J.L., and Steinberg, J.L.: 1977, Astron. Astrophys. 61, p. 777.Google Scholar
Dulk, G.A., and Sheridan, K.V.: 1974, Solar Phys. 36, p. 191.Google Scholar
Dulk, G.A., Sheridan, K.V., Smerd, S.F., and Withbroe, G.L.: 1977, Solar Phys. 52, p. 349.Google Scholar
Dulk, G.A., Smerd, S.F., MacQueen, R.M., Gosling, J.T., Magun, A., Stewart, R.T., Sheridan, K.V., Robinson, R.D., and Jacques, S.: 1976, Solar Phys. 49, p. 369.Google Scholar
Duncan, R.A.: 1979, “Wave ducting of solar metre-wave radio emission as an explanation of fundamental/harmonic source coincidence and other anomalies”. Solar Phys. 63, 389.Google Scholar
Elgaroy, E.O.: 1977, Solar Noise Storms, Pergamon Press, Oxford, 363 pp.Google Scholar
Gary, D.E., Suzuki, S., and Dulk, G.A.: 1980, Proc. IAU Symp. 86 (this volume), pp. 333.Google Scholar
Gergely, T.E., and Erickson, W.C.: 1975, Solar Phys. 42, p. 467.Google Scholar
Gergely, T.E., and Kundu, M.R.: 1975, Solar Phys. 41, p. 163.CrossRefGoogle Scholar
Gergely, T.E., and Kundu, M.R.: 1976, Solar Phys. 48, p. 357.CrossRefGoogle Scholar
Ginzburg, V.L., and Zheleznyakov, V.V.: 1958, Astron. Zh. 35, p. 364.Google Scholar
Gordon, I.M.: 1971, Astrophys. Lett. 5, p. 251.Google Scholar
Grognard, R.J.-M.: 1980, Proc. IAU Symp. 86 (this volume), pp. 303.CrossRefGoogle Scholar
Gurnett, D.A., and Anderson, R.R.: 1976, Science 194, p. 1159.CrossRefGoogle Scholar
Gurnett, D.A., and Anderson, R.R.: 1977, J. Geophys. Res. 82, p. 632.Google Scholar
Jackson, B.V., and Hildner, E.: 1978, Solar Phys. 60, p. 155.Google Scholar
Kai, K.: 1975, Solar Phys. 45, p. 217.Google Scholar
Kai, K., and Sheridan, K.V.: 1974, Solar Phys. 35, p. 181.Google Scholar
Lantos, P., and Avignon, Y.: 1975, Astron. Astrophys. 41, p. 137.Google Scholar
Lantos-Jarry, M.F.: 1970, Solar Phys. 15, p. 40.CrossRefGoogle Scholar
McLean, D.J.: 1959, Aust. J. Phys. 12, p. 404.Google Scholar
McLean, D.J.: 1970, Proc. Astron. Soc. Aust. 1, p. 315.Google Scholar
McLean, D.J.: 1973, Proc. Astron. Soc. Aust. 2, p. 222.CrossRefGoogle Scholar
McLean, D.J.: 1974, in Coronal Disturbances (IAU Symp. 57) (ed. Newkirk, G. Jr.), p. 301, Reidel, Dordrecht.Google Scholar
McLean, D.J.: 1979, “A proposed correlator back-end for the Culgoora radioheliograph”. Proc. IAU/URSI Colloquium, “Formation of images from spatial coherence functions in astronomy” (in press).Google Scholar
McLean, D.J., and Dulk, G.A.: 1978, Proc. Astron. Soc. Aust. 3, p. 249.Google Scholar
McLean, D.J., and Nelson, G.J.: 1977, Izv. Vyssh. Uchebn. Radiofiz. 20, p. 1359; Radiophys. Quantum Electron. 20, p. 938.Google Scholar
McLean, D.J., Beard, M., and Bos, A.: 1979, “A proposed correlator back-end for the Culgoora radioheliograph”. Proc. Astron. Soc. Aust. (in press).CrossRefGoogle Scholar
McLean, D.J., Sheridan, K.V., Stewart, R.T., and Wild, J.P.: 1971, Nature 234, p. 140.Google Scholar
Magelssen, G.R., and Smith, D.F.: 1977, Solar Phys. 55, p. 212.Google Scholar
Magun, A., Stewart, R.T., and Robinson, R.D.: 1975, Proc. Astron. Soc. Aust. 2, p. 367.Google Scholar
Malville, J.M.: 1962, Astrophys. J. 136, p. 266.Google Scholar
Meerson, B.I., Sasorov, P.V., and Stepanov, A.V.: 1978, Solar Phys. 58, p. 165.Google Scholar
Melrose, D.B., and Sy, W.: 1972, Aust. J. Phys. 25, p. 387.Google Scholar
Melrose, D.B., Dulk, G.A., and Smerd, S.F.: 1978, Astron. Astrophys. 66, p. 315.Google Scholar
Nelson, G.J., and McLean, D.J.: 1977, Contributed Papers to the Study of Interplanetary Phenomena 1977 (Proc. COSPAR Symp. B, Tel Aviv, June, 1977) (eds. Shea, M.A., Smart, D.F., and Wu, S.T.), U.S. Air Force Geophysics Laboratory Special Report No. 209.Google Scholar
Payne-Scott, R., Yabsley, D.E., and Bolton, J.G.: 1947, Nature 160, p. 256.Google Scholar
Riddle, A.C.: 1974, Solar Phys. 35, p. 153.Google Scholar
Roberts, J.A.: 1958, Aust. J. Phys. 11, p. 215.Google Scholar
Robinson, R.D.: 1978, Aust. J. Phys. 31, p. 533.Google Scholar
Robinson, R.D., and Smerd, S.F.: 1975, Proc. Astron. Soc. Aust. 2, p. 374.Google Scholar
Rosenberg, H.: 1970, Astron. Astrophys. 9, p. 159.Google Scholar
Sheridan, K.V., Jackson, B.V., McLean, D.J., and Dulk, G.A.: 1978, Proc. Astron. Soc. Aust. 3, p. 249.Google Scholar
Smerd, S.F.: 1970, Proc. Astron. Soc. Aust. 1, p. 305.Google Scholar
Steinberg, J.L., Caroubalos, C., and Bougeret, J.L.: 1974, Astron. Astrophys. 37, p. 109.Google Scholar
Stewart, R.T.: 1976, Solar Phys. 50, p. 437.CrossRefGoogle Scholar
Stewart, R.T., and Labrum, N.R.: 1972, Solar Phys. 27, p. 192.Google Scholar
Stewart, R.T., Duncan, R.A., Suzuki, S., and Nelson, G.J.: 1978, Proc. Astron. Soc. Aust. 3, p. 247.Google Scholar
Suzuki, S., Dulk, G.A., and Sheridan, K.V.: 1980, Proc. IAU Symp. 86 (this volume), pp. 315.Google Scholar
Uchida, Y.: 1974, Solar Phys. 39, p. 431.Google Scholar
Takakura, T.: 1977, Solar Phys. 52, p. 429.Google Scholar
Takakura, T.: 1979a, Solar Phys. 61, p. 143.Google Scholar
Takakura, T.: 1979b, Solar Phys. 61, p. 161.Google Scholar
Takakura, T., and Shibahashi, H.: 1976, Solar Phys. 46, p. 323.Google Scholar
Wild, J.P.: 1950a, Aust. J. Sci. Res. A3, p. 399.Google Scholar
Wild, J.P.: 1950b, Aust. J. Sci. Res. A3, p. 541.Google Scholar
Wild, J.P.: 1970, Proc. Astron. Soc. Aust. 1, p. 365.Google Scholar
Wild, J.P., and McCready, L.L.: 1950, Aust. J. Sci. Res. A3, p. 387.Google Scholar
Zaitsev, V.V., and Stepanov, A.V.: 1975, Issled. Geomagn. Aeron. Fiz. Solntsa 37, p. 3.Google Scholar