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March 5, 1857.

The LORD WROTTESLEY, President, in the Chair.

In accordance with the Statutes, the Secretary read the following list of Candidates for Election into the Society :

Thomas Graham Balfour, M.D.

Robert Ball, LL.D.

Henry Foster Baxter, Esq.
Lionel Smith Beale, M.B.
Samuel Husbands Beckles, Esq.
Charles Tilstone Beke, Ph.D.
George Boole, Esq.
Edward M. Boxer, Capt. R.A.
Samuel Brown, Esq.

George Bowdler Buckton, Esq.
Thomas William Burr, Esq.
William Dingle Chowne, M.D.
William Coulson, Esq.
Thomas Russell Crampton, Esq.
Richard Cull, Esq.
Thomas Davidson, Esq.
Hugh Welch Diamond, M.D.
James Dixon, Esq.

S. W. Fullom, Esq.

William Bird Herapath, M.D.
Rowland Hill, Esq.
George Grote, Esq.

Rev. Thomas Kirkman.

Henry Letheby, M.B.

Waller Augustus Lewis, M.B.
George Macilwain, Esq.
David Macloughlin, M.D.
William Marcet, M.D.
John Marshall, Esq.
John Penn, Esq.
William Peters, Esq.
Lieut. Bedford Pim, R.N.
Andrew Smith, M.D.
Robert Angus Smith, Esq.
Warington Wilkinson Smyth,
Esq.

Charles Piazzi Smyth, Esq.
Henry Clifton Sorby, Esq.
John Welsh, Esq.
Thomas Williams, M.D.
Joseph Whitworth, Esq.

Forbes Benignus Winslow, M.D.
Bennet Woodcroft, Esq.
James Young, Esq.

VOL. VIII.

2 H

The following communication was read:

"On what the Colonial Magnetic Observatories have accomplished." By Major-General SABINE, R.A., Treas. and V.P.R.S. Received February 26, 1857.

It has been suggested to me, that a brief review of what has been accomplished by the Colonial Magnetic Observatories, instituted on the joint recommendation of the Royal Society and British Association, would be acceptable; and that the officer who has been entrusted with the superintendence of these establishments is the person from whom such a review may most properly be expected. Fully assenting to both propositions, I have readily undertaken the task; and have availed myself of the occasion to add a few remarks and suggestions on the measures which appear to be required for the further prosecution of the objects for which the observatories were recommended.

The magnetic investigations designed to be carried into execution by the Colonial Observatories recommended by the Royal Society embraced a much wider scope than had been contemplated by any previous institutions, or than had been provided for by the arrangements or instrumental means of any then existing establishment, whether national or private. Not, as previously, limited to observations of a single element (the Declination),-or combining at the most one only of the components of the magnetic force,—the instructions of the Royal Society, and the instrumental means prepared under its direction, provided for the examination, in every branch of detail, of each of the three elements which, taken in combination, represent, not partially but completely, the whole of the magnetic affections experienced at the surface of the globe, classed under the several heads of absolute values, secular changes, and variations either periodical or occasional,-and proceeding from causes either internal or external. To meet the requirements of inductive reasoning, it was needful that the results to be obtained should comprehend all particulars under these several heads, attainable by an experimental inquiry of limited duration. That no uncertainty might exist as to the objects to which, in so novel an undertaking, attention

was to be directed, the Report of the Committee of Physics, approved and adopted by the President and Council of the Royal Society, stated in a very few sentences, remarkable alike for their comprehensiveness and conciseness, the desiderata of magnetical science. It may be convenient to reproduce these, when desiring to show the degree in which the Observatories have fulfilled their contemplated purposes :-"The observations will naturally refer themselves to two chief branches, into which the science of terrestrial magnetism in its present state may be divided. The first comprehends the actual distribution of the magnetic influence over the globe, at the present epoch, in its mean or average state, when the effects of temporary fluctuations are either neglected, or eliminated by extending the observations over a sufficient time to neutralise their effects. The other comprises the history of all that is not permanent in the phenomena, whether it appear in the form of momentary, daily, monthly, or annual change and restoration; or in progressive changes not compensated by counter-changes, but going on continually accumulating in one direction, so as in the course of many years to alter the mean amount of the quantities observed."-Report, pp. 1, 2.

With reference to the first of these two branches, viz. the actual distribution of the magnetic influence over the globe at the present epoch, the Report goes on to state :-"The three elements, viz. the horizontal direction, the dip, and the intensity of the magnetic force, require to be precisely ascertained, before the magnetic state of any given station on the globe can be said to be fully determined . . and as all these elements are at each point now ascertained to be in a constant state of fluctuation, and affected by transient and irregular changes, the investigation of the laws, extent, and mutual relations of these changes is now become essential to the successful prosecution of magnetic discovery."

With reference to the second branch, viz. the secular and periodical variations, it is observed that-"The progressive and periodical being mixed up with the transitory changes, it is impossible to separate them so as to obtain a correct knowledge and analysis of the former, without taking express account of and eliminating the latter;" and with reference to the secular changes in particular, it is remarked "These cannot be concluded from comparatively shortseries of observations without giving to those observations extreme

nicety, so as to determine with perfect precision the mean state of the elements at the two extremes of the period embraced; which, as already observed, presupposes a knowledge of the casual deviations."

It is clear from these extracts that in the discussion of the observations the first point, in the order of time, ought necessarily to be an investigation into "the laws, extent, and mutual relations of the transient and," (as they were called at the time the Report was written,) "irregular changes," as a preliminary step to the elimination of their influence on the observations from which a correct knowledge and analysis of the progressive and periodical changes were to be obtained. It will be proper to show therefore, in the first place, what the Observatories have accomplished in regard to the socalled casual or transitory variations.

Casual Variations.-All that was known regarding these phenomena at the period when the Report of the Committee of Physics was written, was, that there occurred occasionally, and, as it was supposed, irregularly, disturbances in the horizontal direction of the needle, which were known to prevail, with an accord which it was impossible to ascribe to accident, simultaneously over considerable spaces of the earth's surface, and were believed to be in some unknown manner connected, either as cause or effect, with the appearances of the aurora borealis. The chief feature by which the presence of a disturbance of this class could be recognized at any instant of observation, or by which its existence might be subsequently inferred independently of concert or comparison with other Observatories,-appeared to be, the deflection of the needle from its usual or normal position to an amount much exceeding what might reasonably be attributed to irregularities in the ordinary periodical fluctuations. The observations which had been made on the disturbances anterior to the institution of the Colonial Observatories had been chiefly confined to the declination. A few of the German Observatories had recently begun to note the disturbances of the horizontal force; but as yet no conclusions whatsoever had been obtained as to their laws: in the words of the Committee's Report, the disturbances "apparently observe no law." By the instructions cited above, the field of research was enlarged, being made to comprehend the disturbance-phenomena of the three elements; and the importance of their examination was urged, not

alone as a means of eliminating their influence on the periodic and progressive changes, but also on the independent ground, that "the theory of the transitory changes might prove itself one of the most interesting and important points to which the attention of magnetic inquirers can be turned, as they are no doubt intimately connected with the general causes of terrestrial magnetism, and will probably lead us to a much more perfect knowledge of those causes than we now possess."

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The feature which has been referred to as furnishing the principal if not the only certain characteristic of a disturbance of this class, viz. the magnitude of the departure from the usual or normal state at the instant of observation, has, in the discussion of the observations, been made available for the investigation of their laws it has afforded the means of recognizing and separating from the entire mass of hourly observations, taken during several years, a sufficient body of observations to furnish the necessary data for investigating at three points of the earth's surface-one in the temperate zone of the northern hemisphere, a second in the temperate zone of the southern hemisphere, and a third in the tropics-the laws or conditions regulating or determining the occurrence of the magnetic disturbances. The method by which this separation has been effected has been explained on several recent occasions, and will be found fully described in the Phil. Trans. for 1856, Art. XV. By processes of this description, the disturbances of principal magnitude in each of the three elements, the Declination, Inclination and Total Force, have been separated from the other observations, at the three observatories of Toronto, Hobarton and St. Helena, and submitted to an analysis of which the full particulars will be found in the preliminary portions of the volumes which record the observations. By the adoption of a uniform magnitude as constituting a disturbance throughout the whole period comprised by the analysis, the amount of disturbance in the several years, months, and hours is rendered intercomparable. The result of this investigation (which could not be otherwise than a very laborious operation, since the observations at a single one of these stations, Toronto, considerably exceeded 100,000 in number, each of which had to be passed through several distinct processes,) has made known to us that the phenomena of this class, which may in future with propriety

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