Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3665m&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
1
Scientific paper
The Force-Field equation is a classical, convenient means to describe modulation effects in the one-dimensional approximation. It serves mainly as a tool for experimentalists to give a concise description of modulation strength. By comparing the Force-Field solution to numerical solutions of the transport equation, however, we show that the Force-Field approximation gets progressively worse with increasing radial distance. The reason is that adiabatic losses in the outer heliosphere become unimportant, and the ForceField equation can not simulate that. It is shown that the convection-diffusion approximation is more appropriate in the outer heliosphere. This result has consequences for the interpretation of Pioneer/Voyager observations in the outer heliosphere.
Moraal Harm
Steenberg Conrad D.
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