Computer Science
Scientific paper
Mar 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984rspta.310..365j&link_type=abstract
Royal Society (London), Philosophical Transactions, Series A (ISSN 0080-4614), vol. 310, no. 1513, March 16, 1984, p. 365-406. R
Computer Science
2
Geomagnetism, Magnetic Storms, Magnetic Variations, Data Smoothing, Geoelectricity, Secular Variations
Scientific paper
It is noted that with modern computing facilities and techniques and the availability of digitized data from an improved distribution of magnetic observatories, it is now possible to analyze magnetic storms for a greatly extended period, up to 10 days or so, after the onset of the storm. An analysis is made here of six storms, two of which occurred during the quiet part of the solar cycle (June 1964 and April 1965), the remainder occurring during a more active part (February 1969, March 1970, and August 1970). For each storm, data at hourly intervals from at least 58 observatories within + or - 55 deg latitude of the geomagnetic equator are used. Values of the external and internal parts of the variation field are obtained and are presented along with their associated errors for the dominant P sub 1 harmonic. Also given is an assessment of the results on the basis of statistical arguments.
Jady R. J.
Marshall T. R.
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