TheE following appearances are as noted in my journal at the time. They so entirely resembled auroral beams, that I had no hesitation in pronouncing them at the time to be such. This opinion has, however, been dissented from by some meteorologists, who consider that certain facts connected with the geographical distribution of auroras (if I may use the term), are opposed to it. I am well aware of the force of these arguments, which I shall not attempt to controvert; but for the information of those who may be interested in the matter, I may remark, that I am very familiar with the Aurora borealis in the northern temperate zone, and during the Antarctic expedition was in the habit of recording in the log-book the appearance presented by the Aurora australis. The late Mr. Williams, Mr. Haddon, and Mr. Theobald, who were also witnesses of the appearances on this occasion, considered it a brilliant display of the aurora. _Feb. 14th,_ 9 p.m.--Bax. Corr. 29.751; temp. 62 degrees; D.P. 41.0 degrees; calm, sky clear; moon three-quarters full, and bright. Observed about thirty lancet beams rising in the north-west from a low luminous arch, whose extremes bore W. 20 degrees S., and N. 50 degrees E.; altitude of upper limb of arch 20 degrees, of the lower 8 degrees. The beams crossed the zenith, and converged towards S. 15 degrees E. The extremity of the largest was forked, and extended to 25 degrees above the horizon in the S.E. by S. quarter. The extremity of the centre one bore S. 50 degrees E., and was 45 degrees above the horizon. The western beams approached nearest the southern horizon. All the beams moved and flashed slowly, occasionally splitting and forking, fading and brightening; they were brightly defined, though the milky way and zodiacal light could not be discerned, and the stars and planets, though clearly discernible, were very pale. At 10 p.m., the luminous appearance was more diffused; upper limb of the arch less defined; no beams crossed the zenith; but occasionally beams appeared there and faded away. Between 10 and 11, the beams continued to move and replace one another, as usual in auroras, but disappeared from the south-east quarter, and became broader in the northern hemisphere; the longest beams were near the north and north-east horizon. At half-past 10, a dark belt, 4 degrees broad, appeared in the luminous arch, bearing from N. 55 degrees W. to N. 10 degrees W.; its upper limb was 10 degrees above the horizon: it then gradually dilated, and thus appeared to break up the arch. This appeared to be the commencement of the dispersion of the phenomenon. At 10.50 p.m. the dark band had increased so much in breadth that the arch was broken up in the north-west, and no beams appeared there. Eighteen linear beams rose from the eastern part of the arch, and bore from north to N. 20 degrees E.