The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance

Details The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance The cosmic ray differential diurnal variation dependences on the zenith angle and the geomagnetic disturbance

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..139k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 139-142 (SEE N85-34991 23-93)

Mathematics

Differential Geometry

Cosmic Rays, Diurnal Variations, Magnetic Disturbances, Muons, Particle Motion, Amplitudes, Azimuth, Differential Geometry, Geomagnetism, Interplanetary Medium, Zenith

Scientific paper

Simultaneous and continuous muon measurements in two opposite azimuthal directions under equal zenith angles demonstrated the importance of this method for cosmic ray diurnal variation investigations. Lately these measurements were extended by means of improved telescopes. The obtained cosmic ray diurnal variations were presented as intensity differential curves. Theoretical investigations connected the properties of these curves with some interplanetary space parameters. The harmonics of these curves were interpreted physically. Some order difference curves were introduced. In earlier works some dependences between the parameters characterizing the first and the second harmonics of the differential intensity curves and the geomagnetic activity were found. Then all measurements were carried out under only one zenith angle. The results of investigations of similar dependences using data of simultaneous measurements under three different zenith angles are presented.

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