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ks then undertook the work.--I attended the meeting of the British Association held at York (principally in compliment to the President, Dr Peacock), and gave an oral account of my work on Irish Tides.--At the Oxford Commemoration in June, the honorary degree of D.C.L. was conferred on M. Struve and on me, and then a demand was made on each of us for _L6. 6s._ for fees. We were much disgusted and refused to pay it, and I wrote angrily to Dr Wynter, the Vice-Chancellor. The fees were ultimately paid out of the University Chest. "In this year the longitude of Altona was determined by M. Struve for the Russian Government. For this purpose it was essential that facilities should be given for landing chronometers at Greenwich. But the consent of the customhouse authorities had first to be obtained, and this required a good deal of negotiation. Ultimately the determination was completed in the most satisfactory manner. The chronometers, forty-two in number, crossed the German Sea sixteen times. The transit observers were twice interchanged, in order to eliminate not only their Personal Equation, but also the gradual change of Personal Equation. On Sept. 30th Otto Struve formally wrote his thanks for assistance rendered. "For the determination of the longitude of Valencia, which was carried out in this year, various methods were discussed, but the plan of sending chronometers by mail conveyance was finally approved. From London to Liverpool the chronometers were conveyed by the railways, from Liverpool to Kingstown by steamer, from Dublin to Tralee by the Mail Coaches, from Tralee to Cahersiveen by car, from Cahersiveen to Knightstown by boat, and from Knightstown to the station on the hill the box was carried like a sedan-chair. There were numerous other arrangements, and all succeeded perfectly without a failure of any kind. Thirty pocket chronometers traversed the line between Greenwich and Kingstown about twenty-two times, and that between Kingstown and Valencia twenty times. The chronometrical longitudes of Liverpool Observatory, Kingstown Station, and Valencia Station are 12m 0.05s, 24m 31.17s, 41m 23.25s; the geodetic longitudes, computed from elements which I published long ago in the Encyclopaedia Metropolitana, are 12m 0.34s, 24m 31.47s, 41m 23.06s. It appears from this that the elements to which I have alluded represent the form of the Earth here as nearly as is possible. On the whole, I think it probable that
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