Abstract
THE effects of solar eclipses on the geomagnetic field have been summarized by Matsushita1. On quiet days clear changes in the geomagnetic field were seen superimposed on the Sq variation by Egedal and Ambolt2 and by Kato3. The effect to be described here is somewhat different in that the eclipse occurred during a magnetically disturbed time, and the effect could only be isolated by comparing magnetic records at an eclipsed station with simultaneous records at other stations situated outside the region of total eclipse. In the present study four stations situated on a line approximately at right angles to the path of totality were specially equipped with geomagnetic variographs (Table 1).
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References
Matsushita, S., Physics of Geomagnetic Phenomena, 1 (edit. by Matsushita, S., and Campbell, W. H.), 348 (1967).
Egedal, J., and Ambolt, N., J. Atmos. Terr. Phys., 7, 40 (1966).
Kato, Y., Sci. Rept. Tohoku Univ., Fifth Ser., 12 (1960).
Serson, P. H., Canad. J. Phys., 35, 1387 (1957).
Roy, J. L., Canad. J. Phys., 42, 831 (1964).
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STENING, R., GUPTA, J. & VAN BEEK, G. Magnetic Observations in Canada during the Solar Eclipse of March 7, 1970. Nature Physical Science 230, 22–23 (1971). https://doi.org/10.1038/physci230022a0
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DOI: https://doi.org/10.1038/physci230022a0