Physics
Scientific paper
Dec 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...81..367v&link_type=abstract
Solar Physics, vol. 81, Dec. 1982, p. 367-374.
Physics
25
Interplanetary Magnetic Fields, Magnetic Flux, Periodic Variations, Radial Distribution, Solar Wind Velocity, Wave Propagation, Astronomical Models, Data Processing, Helios A, Helios B, Propagation Modes, Solar System
Scientific paper
An analysis is conducted of the radial evolution of the wave phenomena observed in the inner solar system and associated with the high velocity solar wind stream pattern. The combined interplanetary magnetic field observations performed by Helios-1 and Helios-2 spacecraft allow to draw the following conclusions: (1) The compressive contribution to field fluctuations with periods less than 6 hr is observed to increase with the increasing heliocentric distance and the total variance of the field components decreases appreciably faster than r to the -3rd. (2) When compared with theoretical models, Helios observations confirm a better agreement with wave modes which saturate at a constant value of the ratio between the wave energy density and the ambient field energy density.
Vellante Massimo
Villante Umberto
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