Estimating the change in asymptotic direction due to secular changes in the geomagnetic field

Details Estimating the change in asymptotic direction due to secular changes in the geomagnetic field Estimating the change in asymptotic direction due to secular changes in the geomagnetic field

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..336f&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 336-339 (SEE N85-34991 23-93)

Physics

Optics

Cosmic Rays, Estimates, Geomagnetism, Orbits, Particle Trajectories, Vertical Distribution, Asymptotic Methods, Flux (Rate), Magnetic Rigidity, Time Measurement

Scientific paper

The concept of geomagnetic optics, as described by the asymptotic directions of approach, is extremely useful in the analysis of cosmic radiation data. However, when changes in cutoff occur as a result of evolution in the geomagnetic field, there are corresponding changes in the asymptotic cones of acceptance. A method is introduced of estimating the change in the asymptotic direction of approach for vertically incident cosmic ray particles from a reference set of directions at a specific epoch by considering the change in the geomagnetic cutoff.

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