Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..469n&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 469-472 (SEE N85-34729 23-92)
Physics
Current Sheets, Galactic Cosmic Rays, Gradients, Heliosphere, Interplanetary Medium, Latitude, Magnetic Fields, Polarity, Reversing, Solar Magnetic Field, Solar Wind Velocity, Ecliptic, Evaluation, Models, Modulation, Rigidity, Solar Corona
Scientific paper
Within the statistical limits imposed by the currently available data and the noise inherent in the determination of the latitudinal gradient, no evidence for the expected change in the latitudinal gradient from pre-1980 to post-1980 epochs can be found. In addition, the rigidity dependence of the gradient appears to be the same in the two epochs. Thus, no evidence is found for a sensitivity of the latitudinal gradient to the polarity of the largescale heliospheric magnetic field such as has been predicted by models incorporating particle drifts.
Garcia-Munoz Manuel
Lockwood John A.
Newkirk Gordon Jr.
Simpson André J.
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