Some relationships between solar X-ray bursts and SPA's produced on VLF propagation in the lower ionosphere

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Data de publicação
1969
Periódico
Solar Physics
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17
Autores
Kaufmann P.
Paes de Barros M.H.
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This paper discusses SPA's measured at long VLF propagation paths in the lower ionosphere and their association with solar X-ray bursts observed by USNRL satellites in the 0-3 Å, 0-8 Å and 8-20 Å bands. Excellent correlations were found between the SPA importances (in degrees per Mm) and the logarithm of the X-ray burst peak intensities. A hardening of the X-ray burst spectra is evident for increasing importance of SPA's; the threshold energy required for the occurrence of such anomalies was estimated, it is 4.3×10-5 ergs cm-2 sec-1 in the main ionizing band of 0-3 Å. It was also possible to derive the effective recombination coefficient at the normal D-region height of 70 km, this being αr≈6×10-6 cm3 sec-1; furthermore ion production rates were estimated during SPA's at heights below the reference level. © 1969 D. Reidel Publishing Company.
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