The magnetic north (H), magnetic east (D) and vertically downward (Z) compo
nents of the geomagnetic field were monitored at Elazig, Turkey, with a thr
ee-component fluxgate magnetometer during the 1999 August 11 total eclipse
of the Sun. The results were compared with those obtained with an identical
instrument at Kandilli magnetic observatory, which is at a similar latitud
e to Elazig, but clear of the band of totality. An increase of D is found d
uring the eclipse, rising to a maximum close to the time of maximum eclipse
. The reality of this effect is confirmed by noting a similar feature, also
centred on the time of eclipse, at a number of European observatories.