Seasonal variation of bioluminescence in the Mediterranean Sea Jessica Craig, Alan Jamieson, Jessica Craig, Alan Jamieson, Phil Bagley & Monty Priede Phil Bagley & Monty Priede Oceanlab, University of Aberdeen, Scotland, UK Oceanlab, University of Aberdeen, Scotland, UK www.oceanlab.abdn.ac.uk www.oceanlab.abdn.ac.uk
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Seasonal variation of bioluminescence in the Mediterranean Sea Jessica Craig, Alan Jamieson, Phil Bagley & Monty Priede Oceanlab, University of Aberdeen,
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Seasonal variationof bioluminescence in the
Mediterranean Sea
Jessica Craig, Alan Jamieson, Jessica Craig, Alan Jamieson, Phil Bagley & Monty PriedePhil Bagley & Monty Priede
Oceanlab, University of Aberdeen, Scotland, UKOceanlab, University of Aberdeen, Scotland, UKwww.oceanlab.abdn.ac.ukwww.oceanlab.abdn.ac.uk
1. Is there seasonal variation in BL at NEMO and NESTOR?
2. Is there a difference in BL between NEMO and NESTOR?
Generalised Additive Modelling (GAM)
- models non-linear relationships
Seasonal variation
Table 2. GAM analysis results - difference between spring and autumn BL density in the E and W Ionian Sea.
W Ionian Sea (NEMO) E Ionian Sea (NESTOR)
p-value <0.001 0.07
NEMO NESTOR
Seasonal variationNEMO
NE Atlantic Ocean- Observation of autumnal deep maxima
(Gillibrand et al. 2007)
Autumnal deep maxima attributed to enhanced biomass fed by export of spring surface primary productivity to deeper water
Difference in BL between sites
Table 2. GAM analysis results - difference between BL density in the E and W Ionian Sea in the spring and autumn
Spring Autumn
p-value <0.001 <0.001
Seasonal difference between sitesNEMO NESTOR
(Mean BL sources. m-3 )
Autumn 12.96 1.78
Spring 4.35 3.17
500 - 2500 m
2500 - 3500 mNEMO NESTOR
(Mean BL sources.m-3 )
Autumn 0.42 0.24
Spring 0.63 0.17
NEMO NESTORMean Flashes.hour-1
Autumn 4 2
Spring 6 2
2
animalsphere1
2
ø
2
ø.simpacts
Impacts with OM (Priede et al. 2008)
Summary
Significant seasonal variation at the NEMO site- BL density 3x higher in autumn 500-2500 m cf. spring
- What is the fate of this deep peak?
BL decreases towards the East MS
- consistent with previous studies where ANTARES and NESTOR sites
were compared (Priede et al. 2008, Craig et al. 2009)
Significant difference in BL between NEMO & NESTOR- 2-3x higher at the NEMO site at depth 2500-3500 m
Thanks to:
Harilaos Kontoyiannis (HCMR) and crew of the RV Aegaeo
Gian Pietro Gasparini (CNR-ISMAR) and crew of RV Urania
Francesc Sarda (ICM-CSIC) and crew of RV Sarmiento de Gamboa
KM3NeT Project
UK Natural Environment Research Council
Thank you!
Acknowledgements
References
Craig J, Jamieson A, Heger A, Priede I G (2009) Distribution of bioluminescent organisms in the Mediterranean Sea and predicted effects on a deep-sea neutrino telescope, Nuclear Instruments and Methods in Physics Research Section A, 602(1):224-226 doi:10.1016/j.nima.2008.12.043
Dussart B.H. , Les différentes catégories de plancton, Hydrobiologia 26 (1965), pp. 72–74.
Gillibrand E.J.V., Jamieson A.J., Bagley P.M., Zuur A.F., Priede I.G. (2007) Seasonal development of a deep pelagic bioluminescent layer in the temperate Northeast Atlantic Ocean. Marine Ecology Progress Series. 341: 37-44
Heger, A. 2007. In situ observations of bioluminescence in the deep sea: benthic and pelagic measurements in the Atlantic Ocean and Mediterranean Sea. PhD, University of Aberdeen
Priede I G, Jamieson A, Heger A, Craig J, Zuur A F (2008) The potential influence of bioluminescence from marine animals on a deep sea underwater neutrino telescope array in the Mediterranean Sea, Deep Sea Research Part I, 55:1474-1483. doi:10.1016/j.dsr.2008.07.001
Sieburth J.McN. , V. Smetacek and J. Lenz, Pelagic ecosystem structure: heterotrophic compartments of the plankton and their relationship to plankton size fractions, Limnology and Oceanography 23 (1978), pp. 1256–1263.