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On a novel phenomenon in the diurnal inequality of terrestrial magnetism at certain stations
Author(s) -
Robert B. Sangster
Publication year - 1910
Publication title -
proceedings of the royal society of london series a containing papers of a mathematical and physical character
Language(s) - English
Resource type - Journals
eISSN - 2053-9150
pISSN - 0950-1207
DOI - 10.1098/rspa.1910.0032
Subject(s) - midnight , declination , geodesy , magnetism , physics , geology , meteorology , mathematics , atmospheric sciences , geophysics , astrophysics , condensed matter physics , astronomy
In this research the author dealt with data from the Magnetic Observatories at Greenwich, Falmouth, and Pawlowsk (Russia). The declination, the horizontal, and the vertical, forces of terrestrial magnetism are denoted by D, H, and Z respectively, and the horizontal force in the astronomical meridian by X. Diurnal inequality increments are designated by the prefix Δ. The formula for obtaining ΔX is ΔH cos D - HΔD sin D = ΔX, and the unit of force employed is 1 x 10-5 C. G. S. (1γ ). The factor for conversion of ΔD from minutes of arc to units ofγ (HΔD) is H sin 1′; hours are counted continuously from midnight to midnight, and in the attached diagrams the scale value employed is 1·85 mm. = 1γ .

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