Sea Operations for “km3” neutrino telescope

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Presentation transcript:

Sea Operations for “km3” neutrino telescope Title Sea Operations for “km3” neutrino telescope E.G. Anassontzis University of Athens NESTOR COLLABORATION   5-8 October 2003 NIKHEF - Amsterdam

Deployment considerations Modular system with built in redundancy Detector configuration Towers (NEMO, NESTOR) Strings with many light sensor points per deployment per depth level Strings (ANTARES) Strings with several light sensor points per deployment Connections to be made in air (NESTOR) in underwater (ANTARES, NEMO) Use ships of opportunity and non highly specialized surface vessels for deployment Use locally available transport vessels Retrievable and expandable VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

…. Deployment considerations Use ships of opportunity and non highly specialized surface vessels for deployment Use locally available transport vessels Use of bathyscaphs or ROVs ? NO (NESTOR) YES (ANTARES, NEMO) Dynamic positioning Vessels with dynamic positioning Short base line detector positioning Sea state working conditions up to 4+ beaufort VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Energy threshold as low as 4 GeV NESTOR tower NESTOR TOWER with positioning transponders 32 m diameter 30 m between floors 144 PMTs 20 000 m2 Effective Area for E>10TeV Energy threshold as low as 4 GeV NESTOR TOWER Anchor Unit with VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Folded star VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Typical cable-laying ships VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Some of DELTA VERENIKI’s heavy deployment equipment VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Under Construction: to be commissioned at Pylos next spring VERENIKI DELTA VERENIKI Central well-ballasted platform Dynamic position, keeping station 5m Operational up to wind/sea state force 4 beaufort Heave compensating winches Each side 51m long Height 2,3m, barrel height 6,3+1,2m, diameter 4,4 and 6,8 VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Anchor Unit on deck and just above the surface, during deployment VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Star on the surface and just below, during deployment VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Series of towers and/or strings During deployment, we have to make less connections with towers than with strings Series of towers and/or strings Dynamically position of each system VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Deployment of a tower 150 m 3 900 m VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Deployment of a tower 150 m 3 900 m VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Deployment of a tower 150 m 3 900 m VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Deployment of a tower 4 000 m VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Deployment schematic of towers Shore Station Electro-optical cable Several km long Main Buoy Detector Anchor REBU » 4000m MARO RERO Depth, e/o cable and rope lengths not in scale Deployment schematic VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

Simulation of deployment Simulation of deployment or recovery of a NESTOR tower by Makai, Hawaii Simulation of deployment ANTARES strings by ANTARES MAKAI simulation snap shot MAKAI simulation snap s VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

We can deploy jointly the km3 Very Large Volume v Telescope Conclusions ANTARES (with IFREMER) have shown that they can deploy string like detector with success NEMO believe that they can deploy tower like detector NESTOR have shown that they can deploy tower like detector with sucess We can deploy jointly the km3 Very Large Volume v Telescope VLVνT Workshop – 5-8 October 2003 – NIKHEF, Amsterdam NESTOR

NESTOR INSTITUTE

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