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Distribution of bioluminescence in the Mediterranean Sea and predicted effects on a neutrino telescope. Jessica Craig, Alan Jamieson, Amy Heger, Alain Zuur & Monty Priede Oceanlab, University of Aberdeen, Scotland, UK www.oceanlab.abdn.ac.uk. Talk outline. Bioluminescent sources (BL).
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Distribution of bioluminescence in the Mediterranean Sea and predicted effects on a neutrino telescope Jessica Craig, Alan Jamieson, Amy Heger, Alain Zuur & Monty Priede Oceanlab, University of Aberdeen, Scotland, UK www.oceanlab.abdn.ac.uk
Talk outline • Bioluminescent sources (BL) • Measurement methods • BL Distribution in the Mediterranean Sea • BL Distribution at neutrino telescope sites • Modelling the frequency of BL • BL around the PMT optical module
Bioluminescent sources • ANIMALS - Non steady-state flashes • BACTERIA - Steady baseline source of light • Centred on 480nm • Mesoplankton – 0.2-20 mm • (e.g. copepods) • Macroplankton – 20-200 mm • (e.g. euphausiids) • Megaplankton – 200-2000 mm • (e.g. medusae & large colonial • organisms (e.g. pyrosomes)) • (Dussart et al. 1965, Sieburth et al. 1978)
Bioluminescent sources • Quantum emission (photons.flash-1) • Mechanical, chemical and visual stimulation (Heger 2007)
Measurement method • ISIT profiler • ISIT camera – 5 x 10-6 lux (min faceplate sens.) • ‘Splat screen’ – 500 x 375 mm A B C D A – Ultra-low-light camera B – Power/control unit C – Lamp D – Splat-screen (Priede et al. 2006, Heger et al. 2008)
Mediterranean BL distribution • Sampling stations from 4 cruises • ANTARES • - Jan 2004 • ANTARES • - May 2004 • RV Meteor 60-1 • October 2006 • NESTOR • RV Aegeao • - May 2007
Mediterranean BL distribution • Sampling stations from 4 cruises • ANTARES • - Jan 2004 • ANTARES • - May 2004 • RV Meteor 60-1 • October 2006 • NESTOR • RV Aegeao • - May 2007
Mediterranean BL distribution • Sampling stations from 4 cruises ANTARES - Jan 2004 ANTARES - May 2004 RV Meteor 60-1 - October 2006 NESTOR RV Aegeao - May 2007
Mediterranean BL distribution • Sampling stations from 4 cruises • ANTARES • - Jan 2004 • ANTARES • - May 2004 • RV Meteor 60-1 • October 2006 • NESTOR • RV Aegeao • - May 2007
Mediterranean BL distribution • Sampling stations from 4 cruises ANTARES - Jan 2004 ANTARES - May 2004 RV Meteor 60-1 - October 2006 NESTOR RV Aegeao - May 2007
Mediterranean Sea productivity • High surface productivity High abundance bioluminescent sources January April July October MODIS monthly composites Chlorophyll a (2006) (Ocean Colour Portal: http://marine.jrc.cec.eu.int)
Near seafloor BL density • Near-bottom BL density decreases with increasing seafloor depth BL density (sources.m-3) R2 = 0.92 NEMO site not yet sampled Seafloor depth (m) At seafloor depth of 3500m Estimate: 0.05 sources.m-3
Modelling BL frequency • Impacts on detector • Background • Predicted number of bioluminescent flashes in vicinity of OM (Priede et al. submitted; Heger 2007; Buskey & Swift 1990)
BL around the PMT module (Latz et al. 1987; Bowlby & Case 1991)
BL around the PMT module (Latz et al. 1987; Bowlby & Case 1991; Bowlby et al. 1990)
Summary • Low surface productivity Low BL density • Deeper site Low BL density More detailed info: Priede et al. (submitted) The potential influence of bioluminescence from marine animals on a deep sea underwater neutrino telescope array in the Mediterranean Sea. DSR I.
Thanks to: John Carr, the ANTARES collaboration and crew of the GGIX fast catamaran Andre Freiwald, (University of Erlangen) and crew of the FS Meteor (cruise M70 leg-1) Spyros Stavrakakis (HCMR) and crew of the RV Aegaeo UK Natural Environment Research Council Luxembourgish Ministry of Culture Thank you!