Late on the night of the 21st of December the phenomenon appeared partially, and with a variable light, in different parts of the southern sky for several hours. At seven on the following morning it became more brilliant and stationary, describing a well-defined arch, extending from the E.S.E. horizon to that at W.N.W., and passing through the zenith. A very faint arch was also visible on each side of this, appearing to diverge from the same points in the horizon, and separating to twenty degrees distance in the zenith. It remained thus for twenty minutes, when the coruscations from each arch met, and after a short but brilliant display of light, gradually died away. Early on the morning of the 15th of January, 1825, the Aurora broke out to the southward, and continued variable for three hours, between a N.W. and S.E. bearing. From three to four o’clock the whole horizon, from south to west, was brilliantly illuminated, the light being continuous almost throughout the whole extent, and reaching several degrees in height. Very bright vertical rays were constantly shooting upwards from the general mass. At half-past five it again became so brilliant as to attract particular notice, describing two arches passing in an east and west direction, very near the zenith, with bright coruscations issuing from it; but the whole gradually disappeared with the returning dawn. At dusk the same evening, the Aurora again appeared in the southern quarter, and continued visible nearly the whole night, but without any remarkable feature.