Observed geomagnetic field intensity in London since 1820 |
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Authors: | D. R. Barraclough,J. G. Carrigan,& S. R. C. Malin |
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Affiliation: | British Geological Survey, Murchison House, West Mains Road, Edinburgh EH9 3LA, UK. E-mail:;, Bogˇaziçi University, K.O.E.R.I., Çengelköy 81220, İstanbul, Turkey |
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Abstract: | ![]() Our main purpose is to collect all magnetic intensity data observed in the vicinity of London and to adjust these to a common site (Greenwich) to complement the 400-year series of declination ( D ) and inclination ( I ) data of Malin & Bullard (1981 ). The present series is necessarily shorter, since a method for the measurement of intensity in absolute units was not devised until 1832. We have also supplemented the D and I series of Malin & Bullard with recently acquired data. We have also made observations of D , I and total intensity ( F ) at a number of the sites, partly to bring the series up to date and partly to check on the site differences. With the increasing urbanization of London it is necessary to seek data from remoter sites. It is shown that the site differences change significantly with time, but that allowance can be made for this. We present curves of our best estimates of the variation of D , I , F and the horizontal intensity ( H ) that define the complete geomagnetic vector at Greenwich for the interval 1820–1998. Frequency analysis shows little support for a 60-year line in the power spectrum. Within the uncertainty of their determinations, there is good continuity between archaeomagnetic intensity measures and the present results. The moving eddy hypothesis of Malin & Bullard is found to be untenable. |
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Keywords: | geomagnetism secular variation. |
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