Additional file 4: of Feasibility of sun and magnetic compass mechanisms in avian long-distance migration

Figure S4. (A) The time-compensated sunset compass route is deflected near the geographic North Pole because of the rapid changes in absolute directions that the bird is experiencing when flying across longitudes near the poles. Red crosses give the positions of a putative bird departing from Alaska...

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Bibliographic Details
Main Authors: Muheim, Rachel, Schmaljohann, Heiko, Alerstam, Thomas
Format: Text
Language:unknown
Published: figshare 2018
Subjects:
Medicine
Microbiology
FOS Biological sciences
Evolutionary Biology
59999 Environmental Sciences not elsewhere classified
FOS Earth and related environmental sciences
Ecology
Sociology
FOS Sociology
110309 Infectious Diseases
FOS Health sciences
North Pole
Alaska
Online Access:https://dx.doi.org/10.6084/m9.figshare.6449213
https://springernature.figshare.com/articles/Additional_file_4_of_Feasibility_of_sun_and_magnetic_compass_mechanisms_in_avian_long-distance_migration/6449213
Description
Summary:Figure S4. (A) The time-compensated sunset compass route is deflected near the geographic North Pole because of the rapid changes in absolute directions that the bird is experiencing when flying across longitudes near the poles. Red crosses give the positions of a putative bird departing from Alaska along a time-compensated sunset compass route towards the North Pole, reorienting every 200 km. Gnomonic map projection. (B) Sun position (azimuth) at the equator (0° latitude, 0° longitude) over a 24-h period on spring equinox (21 March). Birds starting near the equator close to spring equinox on a time-compensated sunset compass route will run into problems because of the sudden shift of the sun from the east to the west over the course of about 15 min. See also Additional file 6: Figure S6. (PDF 141 kb)

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