Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank

Author Posting. © American Geophysical Union, 2015. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research: Oceans 120 (2015): 2555–2570, doi:10.1002/2014JC010564. We te...

Full description

Bibliographic Details
Published in:Journal of Geophysical Research: Oceans
Main Authors: Pineda, Jesus, Starczak, Victoria R., da Silva, Jose C. B., Helfrich, Karl R., Thompson, Michael A., Wiley, David N.
Format: Article in Journal/Newspaper
Language:English
Published: John Wiley & Sons 2015
Subjects:
Online Access:https://hdl.handle.net/1912/7338
id ftwhoas:oai:darchive.mblwhoilibrary.org:1912/7338
record_format openpolar
spelling ftwhoas:oai:darchive.mblwhoilibrary.org:1912/7338 2023-05-15T16:36:11+02:00 Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank Pineda, Jesus Starczak, Victoria R. da Silva, Jose C. B. Helfrich, Karl R. Thompson, Michael A. Wiley, David N. 2015-04-02 application/pdf https://hdl.handle.net/1912/7338 en_US eng John Wiley & Sons https://doi.org/10.1002/2014JC010564 Journal of Geophysical Research: Oceans 120 (2015): 2555–2570 https://hdl.handle.net/1912/7338 doi:10.1002/2014JC010564 Journal of Geophysical Research: Oceans 120 (2015): 2555–2570 doi:10.1002/2014JC010564 Humpback whales Nonlinear internal waves Shallow temperate bank Ecological hotspots Article 2015 ftwhoas https://doi.org/10.1002/2014JC010564 2022-05-28T22:59:21Z Author Posting. © American Geophysical Union, 2015. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research: Oceans 120 (2015): 2555–2570, doi:10.1002/2014JC010564. We tested the hypothesis that humpback whales aggregate at the southern flank of Stellwagen Bank (SB) in response to internal waves (IWs) generated semidiurnally at Race Point (RP) channel because of the presence of their preferred prey, planktivorous fish, which in turn respond to zooplankton concentrated by the predictable IWs. Analysis of synthetic aperture radar (SAR) images indicates that RP IWs approach the southern flank of SB frequently (∼62% of the images). Published reports of whale sighting data and archived SAR images point to a coarse spatial coincidence between whales and Race Point IWs at SB's southern flank. The responses of whales to IWs were evaluated via sightings and behavior of humpback whales, and IWs were observed in situ by acoustic backscatter and temperature measurements. Modeling of IWs complemented the observations, and results indicate a change of ∼0.4 m/s in current velocity, and ∼1.5 Pa in dynamic pressure near the bottom, which may be sufficient for bottom fish to detect the IWs. However, fish were rare in our acoustic observations, and fish response to the IWs could not be evaluated. RP IWs do not represent the leading edge of the internal tide, and they may have less mass-transport potential than typical coastal IWs. There was large interannual variability in whale sightings at SB's southern flank, with decreases in both numbers of sightings and proportion of sightings where feeding was observed from 2008 to 2013. Coincidence of whales and IWs was inconsistent, and results do not support the hypothesis. We would also like to acknowledge funding from the National Oceanic and Atmospheric Administration Sea Grant (Woods Hole), the Woods Hole Oceanographic Institution, the ESA, and the ... Article in Journal/Newspaper Humpback Whale Woods Hole Scientific Community: WHOAS (Woods Hole Open Access Server) Journal of Geophysical Research: Oceans 120 4 2555 2570
institution Open Polar
collection Woods Hole Scientific Community: WHOAS (Woods Hole Open Access Server)
op_collection_id ftwhoas
language English
topic Humpback whales
Nonlinear internal waves
Shallow temperate bank
Ecological hotspots
spellingShingle Humpback whales
Nonlinear internal waves
Shallow temperate bank
Ecological hotspots
Pineda, Jesus
Starczak, Victoria R.
da Silva, Jose C. B.
Helfrich, Karl R.
Thompson, Michael A.
Wiley, David N.
Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank
topic_facet Humpback whales
Nonlinear internal waves
Shallow temperate bank
Ecological hotspots
description Author Posting. © American Geophysical Union, 2015. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research: Oceans 120 (2015): 2555–2570, doi:10.1002/2014JC010564. We tested the hypothesis that humpback whales aggregate at the southern flank of Stellwagen Bank (SB) in response to internal waves (IWs) generated semidiurnally at Race Point (RP) channel because of the presence of their preferred prey, planktivorous fish, which in turn respond to zooplankton concentrated by the predictable IWs. Analysis of synthetic aperture radar (SAR) images indicates that RP IWs approach the southern flank of SB frequently (∼62% of the images). Published reports of whale sighting data and archived SAR images point to a coarse spatial coincidence between whales and Race Point IWs at SB's southern flank. The responses of whales to IWs were evaluated via sightings and behavior of humpback whales, and IWs were observed in situ by acoustic backscatter and temperature measurements. Modeling of IWs complemented the observations, and results indicate a change of ∼0.4 m/s in current velocity, and ∼1.5 Pa in dynamic pressure near the bottom, which may be sufficient for bottom fish to detect the IWs. However, fish were rare in our acoustic observations, and fish response to the IWs could not be evaluated. RP IWs do not represent the leading edge of the internal tide, and they may have less mass-transport potential than typical coastal IWs. There was large interannual variability in whale sightings at SB's southern flank, with decreases in both numbers of sightings and proportion of sightings where feeding was observed from 2008 to 2013. Coincidence of whales and IWs was inconsistent, and results do not support the hypothesis. We would also like to acknowledge funding from the National Oceanic and Atmospheric Administration Sea Grant (Woods Hole), the Woods Hole Oceanographic Institution, the ESA, and the ...
format Article in Journal/Newspaper
author Pineda, Jesus
Starczak, Victoria R.
da Silva, Jose C. B.
Helfrich, Karl R.
Thompson, Michael A.
Wiley, David N.
author_facet Pineda, Jesus
Starczak, Victoria R.
da Silva, Jose C. B.
Helfrich, Karl R.
Thompson, Michael A.
Wiley, David N.
author_sort Pineda, Jesus
title Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank
title_short Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank
title_full Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank
title_fullStr Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank
title_full_unstemmed Whales and waves : humpback whale foraging response and the shoaling of internal waves at Stellwagen Bank
title_sort whales and waves : humpback whale foraging response and the shoaling of internal waves at stellwagen bank
publisher John Wiley & Sons
publishDate 2015
url https://hdl.handle.net/1912/7338
genre Humpback Whale
genre_facet Humpback Whale
op_source Journal of Geophysical Research: Oceans 120 (2015): 2555–2570
doi:10.1002/2014JC010564
op_relation https://doi.org/10.1002/2014JC010564
Journal of Geophysical Research: Oceans 120 (2015): 2555–2570
https://hdl.handle.net/1912/7338
doi:10.1002/2014JC010564
op_doi https://doi.org/10.1002/2014JC010564
container_title Journal of Geophysical Research: Oceans
container_volume 120
container_issue 4
container_start_page 2555
op_container_end_page 2570
_version_ 1766026492392767488