scholarly journals No evidence for the use of magnetic declination for migratory navigation in two songbird species

PLoS ONE ◽  
2020 ◽  
Vol 15 (4) ◽  
pp. e0232136
Author(s):  
Nikita Chernetsov ◽  
Alexander Pakhomov ◽  
Alexander Davydov ◽  
Fedor Cellarius ◽  
Henrik Mouritsen
Keyword(s):  

The paper deals with the phenomena exhibited by the magnetic declination at Kew from 1890 to 1900. The magnetograph curves have been measured on every day of this period, whether disturbed or undisturbed, and the data from days of the different species are contrasted. Diurnal inequalities are got out for ordinary days, excluding those of large disturbance, and separately for the highly disturbed days, and the differences between these, and the points wherein they differ from the corresponding inequalities from quiet days, are investigated. The disturbed days show a well-marked regular diurnal variation, which differs in many notable respects from that observed on ordinary days.


1872 ◽  
Vol 7 ◽  
pp. 756-758
Author(s):  
J. A. Broun

The author gives the results derived from different discussions of nearly eighty thousand observations, made hourly during the eleven years 1854 to 1864. They are as follows:—1. That the lunar diurnal variation consists of a double maximum and minimum in each month of the year.2. That in December and January the maxima occur near the times of the moon's upper and lower passages of the meridian; while in June and July they occur six hours later, the minima then occurring near the times of the two passages.3. The change of the law for December and January to that for June and July does not happen, as in the case of the solar diurnal variations, by leaps in the course of a month (those of March and October), but more or less gradually for the different maxima and minima.


In the first letter, dated from Alford, Dec. 15, 1829, the author gives a description of the instrument which was furnished to him by the Royal Society for measuring the variation of the magnetic needle, and also the magnetic intensity; and of his mode of using it. The needle was so delicately suspended as to render changes in the declination as small as 10'´ very sensible. In his experiments on the magnetic intensity, the intervals of time occupied in the needle’s performing 50 oscillations, commencing with an arc of 12°, were noted by a stop-watch, in which the stop, being applied on the ba­lance, is instantaneous in its operation. The watch is again released from the stop at the commencement of a new observation; thus com­pensating, on the principle of the repeating circle, for any inaccuracy in the reading off, or any inequality in the divisions of the dialplate. The observations made on an Aurora borealis which appeared on the night of the 14th of December, are particularly detailed. On that occasion, the disturbance of the magnetic declination was so great, and so frequently changing from east to west, and the reverse, as to leave no doubt in the mind of the author of the reality of this influence. The needle, however, was affected at those times only when the fringes of the aurora were in such a position as to include the needle in their planes. It appeared to him, also, that the side towards which the needle declined, was the quarter where the aurora gave out the most vivid light.


1851 ◽  
Vol 2 ◽  
pp. 144-145
Author(s):  
J. A. Broun

The absolute westerly declination at Makerstoun, for the mean epoch, June 1844 = 25° 17′·12.The annual motion of the north end of the needle towards the east = 5′·67.The annual periodof magnetic declination consists of a double oscillation, having nearly the following epochs of maxima and minima.


1999 ◽  
Vol 42 (1) ◽  
Author(s):  
D. R. Barraclough ◽  
S. R. C. Malin

he dominant feature in the magnetic declination record at all European sites for which adequate data are available is a minimum between 1750 and 1860. The time of minimum at different sites correlates well with longitude and implies a westward drift rate of 0.61 ± 0.08° yr-1. This is greatly in excess of the widely adopted value of 0.18° yr-1 for global westward drift.


2017 ◽  
Vol 6 (2) ◽  
pp. 257-261
Author(s):  
Jean L. Rasson ◽  
Olivier Hendrickx ◽  
Jean-Luc Marin

Abstract. The determination of magnetic declination angle entails finding two directions: geographic north and magnetic north. This paper deals with the former. The known way to do it by using the sun's calculable orientation in the sky is improved by using a device based on a WIDIF DIflux theodolite and split photocells positioned on its telescope ocular. Given the WIDIF accurate timing and location provided by the onboard GPS receiver, an astronomical computation can be effected to accurately and quickly determine the sun's azimuth and an auxiliary mark's azimuth. The precise sun's crossing of the split photocell, amplified by the telescope's magnification, allows azimuth accuracies of a few seconds of arc.


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