Abstract
Two remarkable intensity-time patterns in the 113 and 64 MHz single-frequency radio flux records during a type I noise storm and/or a type IV burst on 31 July, 1983 are studied. A comparison of the patterns at both frequencies reveals a high degree of resemblance and inherent common structure although the 64 MHz pattern was seen 40 min later than the 113 MHz pattern. An interpretation is given assuming a slowly uprising and thereby expanding clumpy plasma-magnetic field configuration which is (via accompanying coronal loops) two times illuminated by energetic electrons coming from the soft X-ray flare precursor source region of the H-alpha flares F1 and F2 (see Figure 1).
Similar content being viewed by others
References
Blanco, C.: 1986, private communication.
Box, G. E. P. and Jenkins, G. M.: 1970, Time Series Analysis, Forecasting and Control, Holden Day, San Francisco.
De Groot, T., Loonen, J., and Slottje, C.: 1976, Solar Phys. 48, 321.
Dulk, G. A., Smerd, S. F., Mac Queen, R. M., Gosling, J. T., Magun, A., Stewart, R. T., Sheridan, K. V., Robinson, R. D., and Jacques, S.: 1976, Solar Phys. 49, 369.
Elgarøy, Ø.: 1976, Solar Noise Storms, Pergamon Press, Oxford.
Elgarøy, Ø. and Ugland, O.: 1970, Astron. Astrophys. 5, 372.
Fárník, F.: 1985, private communication.
Gary, D. E., Dulk, G. A., House, L., Illing, R., Sawyer, C., Wagner, W. J., Mc Lean, D. J., and Hildner, E.: 1984, Astron. Astrophys. 134, 222.
Hanasz, J.: 1966, Australian J. Phys. 19, 635.
Harrison, R. A., Waggett, P. W., Bentley, R. D., Phillips, K. J. H., Bruner, M., Dryer, M., and Simnett, G. M..: 1985, Solar Phys. 97, 387.
Harrison, R. A.: 1985, ‘Solar Coronal Mass Ejections and Flares’, High Altitude Observatory, preprint.
Hofmann, A., Rendtel, J., Aurass, H., and Kalman, B.: 1986, Solar Phys., in press.
Jackson, B. V. and Hildner, E.: 1978, Solar Phys. 60, 155.
Kerdraon, A., Pick, M., Trottet, G., Sawyer, C., Illing, R., Wagner, W., and House, L.: 1983, Astrophys. J. 265, L19.
Krüger, A.: 1979, Introduction to Solar Radioastronomy and Radiophysics, D. Reidel Publ. Co., Dordrecht, Holland.
Kurths, J.: 1986, in preparation.
Lantos, P., Kerdraon, A., Rapley, G. G., and Bentley, R. D.: 1981, Astron. Astrophys. 101, 33.
Loçans, V.: 1985, private communication.
Newkirk, G. A.: 1961, Astrophys. J. 133, 983.
Sheeley, N. R., Howard, R. A., Koomen, M. J., and Michels, D. J.: 1983, Astrophys. J. 272, 349.
Spicer, D. S., Benz, A. O., and Huba, J. D.: 1981, Astron. Astrophys. 105, 221.
Solar Geophysical Data: 1983, No. 468, Part I, U.S. Dept. of Commerce, Boulder, Colorado, U.S.A., 80, p. 303.
Urbarz, H.: 1983, Solar Radio Emission, Spectral Observations at Weissenau Station.
Urbarz, H.: 1985, private communication.
Valniček, B., Fárník, F., Sudová, J., Komárek, B., Linkin, O., and Pisarenko, N.: 1985, PROGNOZ-9 Data, part IV, Publ. Astron. Inst. Czechoslovak Acad. Sci., No. 62.
Wentzel, D. G.: 1982, in Proc. 4th Workshop on Solar Noise Storms, Trieste, Italy, p. 145.
Wild, J. P. and Tlamicha, A.: 1965, Nature 203, 1128
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Aurass, H., Kurths, J., Mann, G. et al. On a strange recurring type I burst pattern. Sol Phys 107, 123–133 (1986). https://doi.org/10.1007/BF00155347
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00155347