Cosmic ray fluctuations - Power spectrum of the north-south intensity difference

Details Cosmic ray fluctuations - Power spectrum of the north-south intensity difference Cosmic ray fluctuations - Power spectrum of the north-south intensity difference

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....4...14o&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 4. (A81-12386 02-93) T

Computer Science

Cosmic Rays, Neutron Counters, Particle Flux Density, Power Spectra, Interplanetary Magnetic Fields, Neutral Sheets, Scintillation

Scientific paper

The fluctuations in the counting rate of earth-based neutron monitors pointing toward the north and south geomagnetic poles are discussed. The power spectrum of the counting-rate difference (i.e., intensity facing north minus intensity facing south) has two important components: scintillations due to particle scattering, and intensity changes due to magnetic sector crossings. The discussion of Jokipii and Owens (1975, 1976) is applied to the north-south intensity difference, and good quantitative agreement with observations is shown.

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