Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?

A basic question concerning the monarch butterflies' fall migration is which monarchs succeed in reaching overwintering sites in Mexico, which fail—and why. We document the timing and pace of the fall migration, ask whether the sun's position in the sky is associated with the pace of the m...

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Main Authors: Orley R. Taylor, James P. Lovett, David L. Gibo, Emily L. Weiser, Wayne E. Thogmartin, Darius J. Semmens, James E. Diffendorfer, John M. Pleasants, Samuel D. Pecoraro, Ralph Grundel
Format: Article
Language:English
Published: Frontiers Media S.A. 2019-12-01
Series:Frontiers in Ecology and Evolution
Subjects:
Online Access:https://www.frontiersin.org/article/10.3389/fevo.2019.00442/full
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author Orley R. Taylor
James P. Lovett
David L. Gibo
Emily L. Weiser
Wayne E. Thogmartin
Darius J. Semmens
James E. Diffendorfer
John M. Pleasants
Samuel D. Pecoraro
Ralph Grundel
author_facet Orley R. Taylor
James P. Lovett
David L. Gibo
Emily L. Weiser
Wayne E. Thogmartin
Darius J. Semmens
James E. Diffendorfer
John M. Pleasants
Samuel D. Pecoraro
Ralph Grundel
author_sort Orley R. Taylor
collection DOAJ
description A basic question concerning the monarch butterflies' fall migration is which monarchs succeed in reaching overwintering sites in Mexico, which fail—and why. We document the timing and pace of the fall migration, ask whether the sun's position in the sky is associated with the pace of the migration, and ask whether timing affects success in completing the migration. Using data from the Monarch Watch tagging program, we explore whether the fall monarch migration is associated with the daily maximum vertical angle of the sun above the horizon (Sun Angle at Solar Noon, SASN) or whether other processes are more likely to explain the pace of the migration. From 1998 to 2015, more than 1.38 million monarchs were tagged and 13,824 (1%) were recovered in Mexico. The pace of migration was relatively slow early in the migration but increased in late September and declined again later in October as the migrating monarchs approached lower latitudes. This slow-fast-slow pacing in the fall migration is consistent with monarchs reaching latitudes with the same SASN, day after day, as they move south to their overwintering sites. The observed pacing pattern and overall movement rates are also consistent with monarchs migrating at a pace determined by interactions among SASN, temperature, and daylength. The results suggest monarchs successfully reaching the Monarch Butterfly Biosphere Reserve (MBBR) migrate within a “migration window” with an SASN of about 57° at the leading edge of the migration and 46° at the trailing edge. Ninety percent of the tags recovered in Mexico were from monarchs tagged within this window. Migrants reaching locations along the migration route with SASN outside this migration window may be considered early or late migrants. We noted several years with low overwintering abundance of monarchs, 2004 and 2011–2014, with high percentages of late migrants. This observation suggests a possible effect of migration timing on population size. The migration window defined by SASN can serve as a framework against which to establish the influence of environmental factors on the size, geographic distribution, and timing of past and future fall migrations.
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spelling doaj.art-0d13134d16af43fead91619aeb0a1f782022-12-21T20:06:37ZengFrontiers Media S.A.Frontiers in Ecology and Evolution2296-701X2019-12-01710.3389/fevo.2019.00442465514Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?Orley R. Taylor0James P. Lovett1David L. Gibo2Emily L. Weiser3Wayne E. Thogmartin4Darius J. Semmens5James E. Diffendorfer6John M. Pleasants7Samuel D. Pecoraro8Ralph Grundel9Department of Ecology and Evolutionary Biology, University of Kansas, Lawrence, KS, United StatesMonarch Watch, Kansas Biological Survey, University of Kansas, Lawrence, KS, United StatesDepartment of Biology, University of Toronto, Mississauga, ON, CanadaU.S. Geological Survey, Upper Midwest Environmental Sciences Center, La Crosse, WI, United StatesU.S. Geological Survey, Upper Midwest Environmental Sciences Center, La Crosse, WI, United StatesU.S. Geological Survey, Geosciences and Environmental Change Science Center, Denver, CO, United StatesU.S. Geological Survey, Geosciences and Environmental Change Science Center, Denver, CO, United StatesDepartment of Ecology, Evolution and Organismal Biology, Iowa State University, Ames, IA, United StatesU.S. Geological Survey, Great Lakes Science Center, Chesterton, IN, United StatesU.S. Geological Survey, Great Lakes Science Center, Chesterton, IN, United StatesA basic question concerning the monarch butterflies' fall migration is which monarchs succeed in reaching overwintering sites in Mexico, which fail—and why. We document the timing and pace of the fall migration, ask whether the sun's position in the sky is associated with the pace of the migration, and ask whether timing affects success in completing the migration. Using data from the Monarch Watch tagging program, we explore whether the fall monarch migration is associated with the daily maximum vertical angle of the sun above the horizon (Sun Angle at Solar Noon, SASN) or whether other processes are more likely to explain the pace of the migration. From 1998 to 2015, more than 1.38 million monarchs were tagged and 13,824 (1%) were recovered in Mexico. The pace of migration was relatively slow early in the migration but increased in late September and declined again later in October as the migrating monarchs approached lower latitudes. This slow-fast-slow pacing in the fall migration is consistent with monarchs reaching latitudes with the same SASN, day after day, as they move south to their overwintering sites. The observed pacing pattern and overall movement rates are also consistent with monarchs migrating at a pace determined by interactions among SASN, temperature, and daylength. The results suggest monarchs successfully reaching the Monarch Butterfly Biosphere Reserve (MBBR) migrate within a “migration window” with an SASN of about 57° at the leading edge of the migration and 46° at the trailing edge. Ninety percent of the tags recovered in Mexico were from monarchs tagged within this window. Migrants reaching locations along the migration route with SASN outside this migration window may be considered early or late migrants. We noted several years with low overwintering abundance of monarchs, 2004 and 2011–2014, with high percentages of late migrants. This observation suggests a possible effect of migration timing on population size. The migration window defined by SASN can serve as a framework against which to establish the influence of environmental factors on the size, geographic distribution, and timing of past and future fall migrations.https://www.frontiersin.org/article/10.3389/fevo.2019.00442/fullDanaus plexippusmigrationmonarch butterflyMonarch Watchphenologysun angle
spellingShingle Orley R. Taylor
James P. Lovett
David L. Gibo
Emily L. Weiser
Wayne E. Thogmartin
Darius J. Semmens
James E. Diffendorfer
John M. Pleasants
Samuel D. Pecoraro
Ralph Grundel
Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?
Frontiers in Ecology and Evolution
Danaus plexippus
migration
monarch butterfly
Monarch Watch
phenology
sun angle
title Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?
title_full Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?
title_fullStr Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?
title_full_unstemmed Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?
title_short Is the Timing, Pace, and Success of the Monarch Migration Associated With Sun Angle?
title_sort is the timing pace and success of the monarch migration associated with sun angle
topic Danaus plexippus
migration
monarch butterfly
Monarch Watch
phenology
sun angle
url https://www.frontiersin.org/article/10.3389/fevo.2019.00442/full
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