Abstract
The more impulsive 7 GHz bursts seem to prefer the solar limb regions, while the degree of polarization decreases with increasing impulsivity.
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References
Basu, D. and Covington, A. E.: 1968, Solar Phys. 5, 102.
Ginzburg, V. L. and Syrovatskii, S. I.: 1965, Ann. Rev. Astron. Astrophys. 3, 297.
Kaufmann, P., Matsuura, O. T., dos Santos, P. M., and Mascaro, A. C. M.: 1968, Astrophys. Letters 2, 149.
Kaufmann, P.: 1969, Solar Phys. 9, 166.
Kaufmann, P.: Matsuura, O. T., and dos Santos, P. M.: 1970, Solar Phys., 14, 190.
Pneuman, G. W.: 1967, Solar Phys. 2, 462.
Swarup, G.: 1964, AAS-NASA Symposium on the Physics of Solar Flares (ed. by W. N. Hess), NASA SP-50, p. 179.
Takakura, T.: 1967, Solar Phys. 1, 304.
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Matsuura, O.T., Nave, M.F.F. Some center-limb statistical trends of impulsive solar bursts at 7 GHz. Sol Phys 14, 384–388 (1970). https://doi.org/10.1007/BF00221323
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DOI: https://doi.org/10.1007/BF00221323