Physics – Plasma Physics
Scientific paper
Jun 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ang....34..105k&link_type=abstract
Annales de Geophysique, vol. 34, Apr.-June 1978, p. 105-112. Research supported by the Ministerio da Aeronautica, Centro Tecnic
Physics
Plasma Physics
Ionospheric Propagation, Lower Ionosphere, Solar Flares, Solar Terrestrial Interactions, Solar X-Rays, Statistical Analysis, Phase Shift, Plasma Physics, Radiant Flux Density, Satellite Observation, Very Low Frequencies
Scientific paper
Magnitudes corresponding to solar flare soft X-ray mean fluxes and energies can be derived from phase anomalies produced in lower ionosphere VLF propagation, producing a homogeneous set of data (500 events). The statistical analysis of a large collection of events indicates that they might behave as the integrated response to a quantisable phenomenon. A characteristic frequency can be tentatively assigned to every event, of which the corresponding total energy would be a multiple of an elementary magnitude that could be statistically estimated. This concept may be reconciled with recent hard X-ray on solar flares and with characteristic Alfven parameters associated with flaring centers.
Iacomo Jr. P.
Kaufmann Patrik
Rizzo Piazza Liliana
Schaal Ricardo E.
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