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Titlebook: Solar-Terrestrial Physics/1970; Proceedings of the I E. R. Dyer Conference proceedings 1972 Springer Nature B.V. 1972 cosmic ray.ionosphere

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Conference proceedings 1972Space Research (COSPAR). These bodies are all concerned with one or another aspect of solar-terrestrial physics, and all joined in believing that the time was ripe for another comprehensive symposium on all aspects of this very active field of research.
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Local Magnetic Fields on the Sunly inhomogeneous, and has fine structure shown by a local maximum of the field strength at a certain depth (Guseeynov, 1969), the strong rotation of the transverse component of the magnetic field with depth (Severny, 1964), the fine structure in the pattern of vertical electric currents (Severny, 1964; Kotov, 1970).
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Particle Diffusion in the Solar Coronas and that, on occasion, the fields are of such a form as to permit rapid spreading in latitude and longitude and that this, coupled with the stochastic wandering of field lines, can readily account for the observed spread in solar longitude of particles at IAU.
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