Characteristics of the latitudinal effect in the charged component of cosmic rays in the atmosphere at a height of 3-5 km

Details Characteristics of the latitudinal effect in the charged component of cosmic rays in the atmosphere at a height of 3-5 km Characteristics of the latitudinal effect in the charged component of cosmic rays in the atmosphere at a height of 3-5 km

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..386a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, May-June 1984, p. 386-392. In Russian.

Computer Science

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Charged Particles, Cosmic Ray Showers, Galactic Cosmic Rays, Geomagnetic Latitude, Lower Atmosphere, Solar Magnetic Field, Spatial Distribution, U.S.S.R.

Scientific paper

Measurements of the charged component of cosmic rays taken from aircraft in the height range 2-10 km over various parts of the Soviet Union are discussed. Reverse latitudinal effects of 5-10 percent in cosmic ray distribution are identified which have been observed for periods of one year and longer. The observed anomalies cannot be explained by thermal or geomagnetic effects or in terms of the anisotropy of galactic cosmic rays and need to be further investigated.

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