Abstract
Dynamic spectra of incremental solar radio emission reveal that (mostly faint) pulsating and morphologically similar structures, including patterns of ‘bright spots’, dominate between ca. 250 and 320 MHz. As ‘individual bursts’ these bright spots are similar to Type I bursts but they appear in an entirely different environment. This kind of activity is indicative of Type IV emission and seems to favour the generation of Type III bursts. Often its boundary with storm activity at the lower side of the band is rather sharp.
Similar content being viewed by others
References
De Groot, T.: 1960, Bull. Astron. Inst. Neth. 15, 229.
De Groot, T.: 1966, Rech. Utrecht XVIII-1.
De Groot, T. and Van Nieuwkoop, J.: 1968, Solar Phys. 4, 332.
Dröge, F. 1967, Z. Astrophys. 66, 200.
Elgarøy, Ø.: 1959, Paris Symposium on Radio Astronomy (ed. by R. N. Bracewell), Stanford University Press, Stanford, p. 248.
Elgarøy, Ø.: 1961, Astrophys. Norv. 7, 123.
Elgarøy, Ø.: 1965, Solar System Radio Astronomy (ed. by J. Aarons), p. 201.
Ellis, G. R. A. and McCulloch, P. M.: 1967, Australian J. Phys. 22, 177.
Ellis, G. R. A.: 1969, Australian J. Phys. 20, 583.
Fung, P. C. M. and Yip, W. K.: 1966, Australian J. Phys. 19, 759.
Hanasz, J.: 1966, Australian J. Phys. 19, 635.
Malville, J. M.: 1962, Astrophys. J. 136, 266.
Maxwell, A.: 1965, The Solar Spectrum (ed. by C. de Jager), p. 342.
Roberts, J. A.: 1959, Australian J. Phys. 12, 327.
Rosenberg, J.: 1970, Astron. Astrophys., in press.
Smerd, S.: 1964, Res. Geophys. 1, 65.
Van Nieuwkoop, J.: 1971, to be published.
Wild, J. P.: 1957, IAU Symp. 4, 321.
Wild, J. P.: 1963, The Solar Corona (ed. by J. W. Evans), p. 121.
Wild, J. P. and Tlamicha, A.: 1965, Nature 207, 1128.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
De Groot, T. Solar radio spectra between 160 and 320 MHz. Sol Phys 14, 176–189 (1970). https://doi.org/10.1007/BF00240176
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00240176