Interplanetary cosmic ray radial gradients with steady state modulation models

Details Interplanetary cosmic ray radial gradients with steady state modulation models Interplanetary cosmic ray radial gradients with steady state modulation models

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94.2323p&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 94, March 1, 1989, p. 2323-2332.

Physics

48

Cosmic Rays, Interplanetary Medium, Radial Distribution, Radiation Distribution, Atmospheric Models, Drift, Heliosphere, Steady State

Scientific paper

The degree of success of steady-state modulation models of increasing complexity in accounting for the observed internal radial gradient from 1977 to 1986 is presently illustrated. In general, it is found that pure drift models based on what may be considered standard modulation parameters may not quantitatively yield the radial gradients observed before and after the recent polarity reversal. Less conventional parameters and/or methods will have to be considered; for instance, models in which most of the modulation takes place in the outer heliosphere.

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