NEMO Status Report - Institute for Nuclear Theory · NEMO Status Report Antonio Capone - INFN -...
Transcript of NEMO Status Report - Institute for Nuclear Theory · NEMO Status Report Antonio Capone - INFN -...
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 1
NEMO Status Report
Antonio Capone - INFN - Romaon behalf of the
NEMO Collaborationhttp://nemoweb.lns.infn.it/
Neutrinos and Subterranean Science - NeSS02Washington, DC - USA - 19÷21 September 2002
-A Km3 scale high-energy Neutrino Telescope-Site selection and characterization in Mediterranean Sea-R&D program for the “KM3” neutrino detector construction-Present detector design: sensitivity and resolutions-The “test site” close to Catania (Sicily, Italy)-Construction plans
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 2
NEMO Collaboration
INFN:Bari, Bologna, Cagliari, Catania, Genova, LNF, LNS, Messina, Roma - ITALY
CNR:Istituto di Oceanografia Fisica (La Spezia)Istituto di Biologia del Mare (Venezia)Istituto Talassografico (Messina)Istituto GEOMARE-SUD (Napoli)
Istituto Nazionale di Geofisica e Vulcanologia
Istituto Nazionale di Oceanorafia e Geofisica Sperimentale (Trieste)
Centro Interdisciplinare di Bioacustica e Ricerche Ambientali (Pavia)
Marina Militare Italiana
Saclant NATO Undersea Research Centre
Universities of:Bari, Bologna, Cagliari, Catania, Genova, Messina, Roma - ITALY
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 3
Site selection for a Km3 Undersea Cherenkov High-Energy Neutrino Telescope
in Mediterranean at depth >3000m (1998-2000)
35° 50’ N, 16° 10’ E (3350m) in the Ionian Sea (Capo Passero) 39° 05’ N, 13° 20’ E (3400m) in the Tyrrhenian Sea (Ustica)39° 05’ N, 14° 20’ E (3400m) in the Tyrrhenian Sea (Alicudi)40° 40’ N, 12° 45’ E (3500m) in the Tyrrhenian Sea (Ponza)
Selected as “Test Site”
20km from shore2000m depth
Best site for the Best site for the “km“km33 Telescope”Telescope”
80 km from shore80 km from shore3300m depth3300m depth
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 4
Depth and atmospheric Muon Flux reduction
Φµ(
cm-2
sr-1
sec-1
)
AMANDA
ANTARES
NEMO
NESTOR
(B&W plot from Moscoso)
Φµ(
cm-2
sr-1
sec-1
)
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 5
Capo Passero deep sea currentsCollected ~ 3 years of deep-sea current data in Capo Passero “KM4” site.
---> average current intensity: 3.1 cm/sec (rms 2.1)---> maximum current intensity: < 16 cm/sec
RCM8: Mechanical current meterRCM11: Doppler current meter
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 6
Capo Passero: sedimentation rateSe
dim
ent f
lux
(mg
m-2
d-1)
time
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 7
In situ Measurements of Inherent Optical PropertiesAC9: absorption(a), scattering (b) and attenuation (c=a+b) for
9 wavelengths: 412, 440, 488, 510, 532, 555, 650, 676, 715 nm
Ia(x)=I0e-a•x
Ic(x)=I0e-c•x
absorbing “Flow tube” “c” measurement
angular acceptance 0.7°
25cm long flow tube
Deep sea set-up:AC9, CTD,
battery pack,PC on ship deck
reflecting “Flow tube” “a” measurement
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 8
Site Selection: Light transmission in Capo Passero Seasonal characterisation of optical and oceanographic parameters in Capo Passero “KM4”.
The column water shows at large depths homogeneity and negligible variations
spring
summerwinter
La Lc
a cT s
AC9 data
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 9
Absorption lengths in NEMO sites and in Baikal lake
Baikal March 2001
V. Balkanov et al.Baikal & Nemo Coll.
astro-ph/0207553
A. Capone et al., NEMO Collaboration,Nucl. Inst. & Methods A, 487 (2002) 423-424.
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 10
Attenuation lengths in NEMO sites and in Baikal lake
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 11
Measurements of light scattering function in deep-sea water
β(λ,ϑ) and <cos(λ,ϑ) > soon available
angular resolution ~0.1°incident light beam not detected
50 cm
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 12
Capo Passero: Biofouling on optical surfaces at 3200m depth (short term measurement)
22/12/99
0.60
0.70
0.80
0.90
1.00
1.10
1.20
1.30
0 5 10 15 20 25 30 35 40
days
transparency
theta 75° theta 60° theta 45° theta 30° theta 15° theta 5°
Negligible effect of fouling after 40 days
Transparency =(PD/reference)t / (PD/reference)day#1
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 13
Capo Passero biological analyses: luminescent bacteria
Luminescent bacteria
Optical background measurement consistent with 40K rate and no bioluminescence: measured 360±40 photons/cm2·s at 0.3 p.e. level
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 14
Capo Passero NEMO site characteristics
• distance from the coast ~ 80 km
• distance from shelf break >40 km
• close to ports, international airport, INFN LNS
• depth > 3300 m
• bathymetric profile is flat over 10 km2
• average current Intensity ~ 3 cm/sec (max < 15 cm/s)
• low biological activity
• at λ=440nm: light attenuation length ~ 35÷40 m (42 m in March)
• at λ=440nm: light absorption length ~ 70÷100 m (100 m in March)
• measured sedimentation rate and fouling rate are low
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 15
Montecarlo studies for the possible configuration of the Km3 detector
4096 optical modules (upward and downward looking)
64 semi-rigid vertical structures:
600m high and displaced at ≥150 m distance
>1km2 effective area for TeV muons
<0.3° median reconstruction angle
Opnemo fast MC code:
Estimate the telescope response as a function of:
-detector geometry-PMT Area, Q.E. and TTS-water optical properties
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 16
Coordinated Feasibility Study for a Km3 detector
coordinated by INFN in collaboration with NATO SACLANTcen, CNR, INOGS
Cable construction and deployment
NEXANS, Pirelli
Detector:deployment and recovery
ENI Consortium
Data/power transmissionsystem
ALCATEL, Pirelli
UnderwaterconnectionsOcean Design
Detector:design and construction
ENI Consortium
ROV/AUVoperations
ENI Consortium
ENI Consortium: SAIPEM, SASP ENG., SONSUB Artist’s view
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 17
40 mdistance between arms
Ti or fiberglassMaterials for construction
20 marm length
150 m750 m
lowest arm (distance rom seabed)
highest arm (distance from seabed)
64OM per tower
4OM per arm
16number of arms
750 mtotal height
The proposed Km3 project: towers à la NEMO
750
m
Optical Module
Electronics module
Electro optical cable
Non mechanical !!!
Dynema fiber
tensioning cable
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 18
Deployment details
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 19
The proposed Km3 project: detector layout
64 VERTICAL STRUCTURES (4096OM)
8 ROWS
8 COLUMNS
200m Distance between VERTICAL STRUCTURES
Bases of vert. structures
plan view of the detector
100 kmE.O. Cable from the shore
8 JUNCTION BOXES
8 BRANCHING UNITS
Backbone Solution
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 20
The proposed Km3 project: main electro optical cable
Optical fibers
Studied with: Nexans and Pirelli
Different solutions evaluated taking into account:mechanical and electrical aspects, complete cable designs, cable cost,manufacture time, ..
Main characteristics of the EOC:• Length 100 km• Power load 80 kW• Optical fibers 48• Electrical conductors 3 or 4
Proposed solutions for power transmission :• AC voltage • DC voltage – monopolar system (sea return)• DC voltage – bipolar system (cable return)
AC voltage
DC voltage – bipolar system
Electrical wire
Optical fibers
Electrical wire
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 21
The proposed Km3 project: Aeff and <∆θ> vs light abs. length
Towers height = 600 mNtowers = 64NOM = 4096
––––
La(450 nm) = 30 mLa(450 nm) = 40 mLa(450 nm) = 55 mLa(450 nm) = 75 m
Effective Area (km2) Median angle (deg)
Median angle (deg)Effective Area (km2)
Nstring/tower= 64 - Hstring/tower= 600m - NPMT = 4096 - DPMT = 10” - σPMT = 2.5 ns - dxy = 180 m
∆θ=|θµrec- θµtrue|
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 22
Tower a la NEMO: different values of the “arm” length
Nstring/tower= 64 - Hstring/tower= 600m - NPMT = 4096 - DPMT = 10” - σPMT = 2.5 ns - dxy = 180 m
Median angle (deg)Effective Area (km2)
Median angle (deg)Effective Area (km2)
∆θ=|θµrec- θµtrue|
L = 40 m –L = 20 m –L = 1 m –String a la ANTARES
Tower a la NEMO
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 23
The proposed Km3 project: underwater connectors and jumpers
Studied with Ocean Design
OD is a leading company in the manufacture of underwater wet mateable connectors, JB – JB jumper and JB – BU jumpers.
Wet-mateable hybrid [optical / electrical]
Mate up to 8 optical fibers and/or electrical circuits underwater. Available in ROV, manual and stab-plate versions with single and/or multi-mode optical fiber. In a single connector, multiple channels allow for higher fiber count, maintenance flexibility and expansion.
Specifications
•100 mate cycles without refurbishment•< 0.5 dB attenuation/optical contact•10 amps at 1,000 volts electrical circuit•10,000 psi operation, •80 lbs mating force for ROV format
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 24
The proposed Km3 project: data transmission system
ALCATEL Italiaproposed a data transmission system according to NEMO specifications.
System characteristics :
• standard telecom system;• redundancy;• high MTBF;• auto-reconfiguration in case of fails; • high transmission rate;• low power consumption
(< 500 W each string tower)
One module for each plane of the string.This Optical Module (S-1.1) will be used as Electrical/Optical converter within the customerequipment in both sides, under sea and in the landing station.
one (STM1 + ST1.1)per each arm
one 1660 SM per tower
One module for each tower of the detector. Each 1660SM will collect all the data coming from the 16 STM 1 of the string. The module will be closed inside a small Junction Box at the base of the string.
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 25
The proposed Km3 project: data transmission rate
1 arm (4 OM)STM1
155 Mbps
1 tower (16 arms)1660-SM
2.5 Gbps (1 wavelength)
16 towers1686-WM
DWDM40 Gbps per channel(16 wavelengths)
48 fibers available:8x1686WM - 2 fiber each16 needed for transmission32 fibers free
100 km cable to shore
JB
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 26
The proposed Km3 project: data transmission system
KM3
Main
Redundancy
100 km
Shore LAB
A L C T E L
1660SM
STM-1 & ST 1.1
1686WM 1686WM
1660SM
1686WM1686WM
STM-1 & ST 1.1
DWDM technology
plus the network manager system
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 27
The Test Site at the port of Catania
Geostar (INGV):Oceanographic and environmental survey.
Permanent on-line seismic monitoring connected to POSEIDON network.
Deep sea (2000 m) test for:• electronics• connectors• optical modules, acoustic modules• deployment and recovery procedures
From the shore lab to the Test site28 km of optical fibres
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 28
The Test Site at the port of Catania: an INFN-LNS facility
Catania
LNS
Port
Test site Laboratory
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 29
The Test Site at the port of Catania: the electro optical cable
10 Optical Fiber standard G-652( 6 to NEMO, 4 to GEOSTAR)
6 Electrical Conductors Φ 4 mm2
( 4 to NEMO, 2 to GEOSTAR)
2.330 m of doubly armed cable
20.595 m of single armed cable
JB BU
JB
JB5.000 m drop cable for recovery
SHORE
GEOSTAR
NEMO test
NEMO connections tested !
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 30
The Test Site at the port of Catania: advanced R&D for the Km3
MAIN JUNCTION BOX
SECONDARY JB
NEMO TOWER
CABLE from SHORE
The Test Site at the port of Cataniaunderwater multidisciplinary laboratory
TestSite
POSEIDON – GEOSTARSubmarine seismic survey
CREEP (UCL)Rock creeping
CIBRAAcoustic survey
20/09/02 Antonio Capone - Neutrinos and Subterranean Science - Washington, DC - USA 32
Summary• NEMO R&D successful:
• Optimal installation site for the “km3” in Capo Passero area
• Long term site characterization activity continues
• Technological feasibility study for the km3 (INFN-Industries-Marine
Research Institutes)
• Test Site at 2000m depth available for advanced R&D
• Large participation to ANTARES 0.1 km2 detector
construction (Mechanical structures, instrumentation, software)
• Definitive km3 design in the framework of an international
collaboration