[5] The magnetograms with the sweeping velocity of 90 mm h -1 of the following observatories: Molodezhnaya for 1976-1992, Novolazarevskaya for 1981-1988, and Borok for 1965-1998 and also analog recordings of the magnetic field to magnetic carriers in the observatories Borok, Molodezhnaya, Vostok, and College (the data archived at Geophysical Observatory Borok) were used. Table 1 shows the codes, corrected geomagnetic coordinates, and L shells of the used observatories. The hourly mean data on the parameters of the solar wind and interplanetary magnetic field (IMF) from the digital King catalog (the data from the World Data Center WDC B) were additionally used.
Citation: (2004), On the relation of giant pulsations (Pg) to pulsations in the PC1 band (the “pearl” series), Int. J. Geomagn. Aeron., 5, GI2001, doi:10.1029/2003GI000062.
Copyright 2004 by the American Geophysical Union