Frequency spectra of short-period variations of cosmic ray

Details Frequency spectra of short-period variations of cosmic ray Frequency spectra of short-period variations of cosmic ray

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..278a&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 278-280 (SEE N85-34991 23-93)

Computer Science

Geomagnetism, Neutron Counters, Periodic Variations, Solar Cosmic Rays, Interplanetary Space, Solar Activity Effects, Solar Cycles

Scientific paper

Frequency spectra for different periods of solar activity were calculated by 5-minutes data of a neutron super-monitor, (altitude 3340 m, cutoff rigidity is 6, 7 GV, counting rate is about 4.5.10 per hour). It was shown that shifting of the spectrum power from low-frequency range to high-frequency range takes place from minimum to maximum of the solar activity. It was reliably distinguished the peak with 160-minutes period coincided with the period of the Sun's atmosphere oscillation and some types of geomagnetic pulsation by the method of accumulation of the frequency spectra. It was conducted the comparison of cosmic ray spectra with spectra of geomagnetic field for the same point of the registration and at the same period.

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