If the summit of the arc pass beyond the zenith of the observer, the latter is surrounded by the matter of the aurora borealis. This matter is nothing else than aqueous vapors traversed by the discharges, and which are in general luminous only at a certain height from the ground, either because the air is there more rarefied, or because they are themselves congealed, and more capable, consequently, of liberating their electric light. Then it is, that, from being nearer to the spot where the phenomenon is taking place, the observer hears the crepitation, or whizzing, of which we have spoken, especially if he be in an open country and in a quiet place. But if the arc do not attain to his zenith, he is situated beyond the region in which the meeting of the electric currents takes place; he sees only an arc a little more elevated to the north or the south, according as he is situated in one hemisphere or the other; and he hears no noise, on account of his too great distance. The crepitation is the result of the action of a powerful magnetic pole upon luminous electric jets in its immediate neighborhood. With regard to the sulphurous odor which some observers have perceived, it arises, as does that which accompanies the fall of lightning, from the conversion into ozone of the oxygen of the air, by the passage of electric discharges. Gisler says, that on the high mountains of Sweden the traveller is sometimes suddenly enveloped in a very transparent fog, of a whitish-gray color inclining a little to green, which rises from the ground, and is transformed into an aurora borealis. The cirro-cumulus and the hazes become luminous when they are traversed by sufficiently energetic discharges of electricity, and when the light of day is no longer present to overcome their more feeble light. Dr. Usher describes an aurora borealis seen in the open day, at noon, May 24, 1778. MM. Cornulier and Verdier are convinced, after carefully studying the subject, that there are almost always aurorae boreales in the high polar latitudes, and that their brilliancy alone is variable. This conviction is in accordance with the very careful observations which have now been made for four years in the northern hemisphere. It appears, as the result of these, that the aurora borealis is visible almost every clear night, but it does not show itself at all the stations at the same time. From October to March there is scarcely a night in which it may not be seen; but it is in February that it is most brilliant. In 1850 it was observed two hundred and sixty-one nights, and during 1851 two hundred and seven. The proportion of nights in which the aurora is seen is much greater the nearer we are to the magnetic pole.