188 research outputs found
On the influence of the heliomagnetospheric periphery on the galactic cosmic rays
The suggestion is substantiated that the periphery of the heliomagnetosphere, the region in which properties depend on both solar wind and interstellar space parameters, plays a much more important role in the solar modulation of galactic cosmic rays than previously believed
Influence of the surface layer characteristics on the regularities of the cutting process
The article considers the influence of the surface layer characteristics on the regularities of the cutting process and the formation of the quality of the surface machined. This effect has been confirmed by the study results of the combined cutting method with advanced plastic deformation (APD). The work estimates the impact of the change in the surface layer properties on the forces and temperature of cutting, stability of the chip formation and quality parameters of the surface machined
The development of the maximum phase of solar cycle 23 in the galactic cosmic ray intensity
[1] The overall features of the solar cycle maximum phase in the galactic cosmic ray intensity near the Earth and the solar and heliospheric factors responsible for them are discussed. The development of the solar cycle in the galactic cosmic ray intensity near the Earth and in the outer heliosphere is compared, both for the absolute intensity and for that normalized allowing for the changing radial position of the spacecraft and the 22-year wave
The Gnevyshev Gap Effect in Galactic Cosmic Rays
Abstract During the last three solar cycles and in a wide energy range of galactic cosmic rays both the modulation and the variability of the intensity demonstrate effects related to the Gnevyshev Gap (GG) -a substantial decrease once or twice during the maximum phase of each solar cycle of a parameter that generally varies in phase with the cycle. The GG-effect also manifests itself in the behaviour of both the strength of the average interplanetary magnetic field and the power of its fluctuating component. The energy dependence of the GGeffect in the modulation and in the variability of the cosmic ray intensity was found to be different. The start of the GG-effect in the cosmic ray modulation practically coincides with a change in the energy dependence of the cosmic ray modulation
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