Computer Science
Scientific paper
Aug 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ge%26ae..18..680d&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 18, July-Aug. 1978, p. 680-683. In Russian.
Computer Science
Geomagnetism, Interplanetary Medium, Magnetic Disturbances, Solar Activity Effects, Identifying, Interplanetary Magnetic Fields, Magnetic Field Configurations, Satellite Observation, Solar Wind
Scientific paper
A method developed by Dolgoarshinnykh (1976) is used for the identification of 12-hour quiet and disturbed periods of geomagnetic activity. The data sample consisted of 50 quiet and 53 disturbed periods during 1967-1968. The quiet and disturbed periods were identified from the following parameters of the interplanetary medium: (1) the interplanetary magnetic field strength, B; (2) the B(x), B(y), and B(z) components of B in solar-ecliptic coordinates; (3) the velocity and density of the solar wind; (4) the mean-square deviations of the mean-hourly values of B(x), B(y), and B(z); (5) the absolute value of B(z); and (6) a parameter signifying the sum of negative values of B(z) for a specified period.
Dolgoarshinnykh B. G.
Dvinskikh N. I.
Rudneva N. M.
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