Abstract
Routine SIDs of the types described in Sections 2.1–2.7 are now available over many years, and statistical relationship between them, and between any of the SID event and the solar ionizing radiations have been examined by many authors. Much of the early works relating to the statistical characteristics of the SIDs concerned the use of Hα emissions in the absence of information of X-ray fluxes. Amongst the major works in this line are the work of Bracewell and Straker (1949) giving the statistical properties of SCNAs observed at Hornsby on 18.3 MHz and that of Ellison (1953) giving the statistical properties of SEAs recorded on 27 kHz.
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© 1974 D. Reidel Publishing Company, Dordrecht, Holland
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Mitra, A.P. (1974). SID Phenomenology. In: Ionospheric Effects of Solar Flares. Astrophysics and Space Science Library, vol 46. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2231-6_4
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DOI: https://doi.org/10.1007/978-94-010-2231-6_4
Publisher Name: Springer, Dordrecht
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