๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

A study of the modulating effect of solar flares on the cosmic ray intensity using time series analysis

โœ Scribed by G. A. Bowe; C. J. Hatton

Publisher
Springer
Year
1982
Tongue
English
Weight
417 KB
Volume
80
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

The cosmic ray 11-year variation for solar cycle 20 is attributed to the modulating effect of solar flare-induced shocks propagating through the interplanetary medium to the boundary of the heliosphere. The relative influence of these disturbances upon the cosmic ray intensity as a function of their travel time from the Sun is determined by a deconvolution of a linear system with the number of solar flares (importance > 1) and the observed cosmic ray intensity as the input and output respectively of this system. The 'impulse response function' so determined indicates that the solar flare -induced disturbances significantly modulate cosmic rays out to a distance of 70-90 AU where the modulating effect of the disturbances abruptly ends. This is interpreted as the boundary of the heliosphere.

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