If we place the pole of an electro-magnet over the jets of electric light that are made to converge in extremely rarefied air, we shall see that the electric light, instead of coming out indifferently from all points of the upper surface, as had taken place before the magnetization, comes out from the points of the circumference only of this surface, so as to form around it a continuous luminous ring. This ring possesses a movement of rotation around the magnetized cylinder, sometimes in one direction, sometimes in another, according to the direction of the discharge and of the magnetization. Finally, some more brilliant jets seem to come out from this luminous circumference without being confounded with the rest of the group. Now the magnetic pole exercises over the luminous haze which we have mentioned as always present during an aurora precisely the same action which the pole of the electro-magnet exercises in the experiment just described; and what takes place on the small scale of the experiment is precisely what takes place on the large scale of the phenomenon of the aurora borealis. The arc of the aurora borealis is a portion of a luminous ring, the different points of which are sensibly at equal distances from the earth, and which centres upon the boreal magnetic pole, so as to cut at right angles all the magnetic meridians that converge towards this pole. Such a ring, seen by an observer placed at the surface of the earth, evidently presents to him the known arc of the aurora; and its _apparent_ summit is always necessarily situated in the magnetic meridian of the place. The diameter of the luminous ring is greater in proportion as the magnetic pole is more distant from the surface of the earth, since this pole must be situated upon the intersection of the plane of the ring with the axis of the terrestrial globe; if we could determine rigorously the position of the aurora borealis, we should then have the means of knowing exactly that of the pole itself. Each observer sees the summit of the auroral arc at his magnetic meridian; it is, therefore, only those who are on the same magnetic meridian who see the same summit, and who are able by simultaneous observations to take its height.