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D' Ardouin SUBATECH

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Characteristics of Radioelectric fields from air showers induced by UHECR ... variations for EAS: criteria of selection from others (fortuitous) sources of RF ... – PowerPoint PPT presentation

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Title: D' Ardouin SUBATECH


1
Characteristics of Radioelectric fields from
air showers induced by UHECR measured by
CODALEMA
  • D. Ardouin - SUBATECH
  • for the CODALEMA collaboration
  • SUBATECH, Nantes
  • Obs. de Paris-Meudon
  • Obs. de Nançay
  • LAL Orsay
  • ESEO Angers
  • LPSC Grenoble
  • LPCE OrleansLAOB Besançon
  • (FRANCE)

ECRS2006
2
CODALEMACOsmic ray Detection Array with
Logarithmic ElectroMagnetic Antennas
11 antennas, band-pass filtered (24-82 MHz) 608m
East-West-, 120 m SW-SE lines 4-fold
coinc.trigger from particle-detectors
ECRS2006
3
Radio-waves arrival times correlate with particle
front times identification of CR
ECRS2006
4
Field topologies
5
Field topologies field profiles
Characteristic shapes appear as genuine radio
signatures of EAS and enable a stand-alone
mode of characterization with an antenna array
ECRS2006
4 EAS typical events detected along the E-W
line
6
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7
In the ground coordinate system
Shower impact determination from EAS field
distributions
8
1 antenna
Background
MHz
ECRS2006
9
Specificity the large azimuthal acceptance
allows investigation of inclined showers
Under way detailed physical correlations with
impact parameter,energy, nature of
primaries,with higher statistics and a completed
set-up
ECRS2006
10
COMPLEMENTS
11
Skymap of radio coincidences ( ? 3 antennas)
12
Reconstructed arrival directions for EAS events
with antenna multiplicities ? 4
13
Cosmic ray counting rate vs zenith angle
14
Antenna acceptance/ particle acceptance for true
EAS events vs zenith angle
15
d0 width distributionfor 64 events M? 4
Mean extension of the field Indication for
designs of large arrays
16
  • NEW Trigger 13 particle detectors
  • counting rate 1 evt / 7 min
  • energy threshold 1x1016eV
  • 16 antennas new dipole array on the North
    South axis

ECRS2006
17
A dedicated LNA(ASIC)
Didier CHARRIER,
FWHM
Aluminium dipole antenna
Preamplifier ASIC
  • Constant directivity, No side lobes from 100kHz
    to 70MHz
  • H-plane half beamwidth120
  • E-plane half beamwidth90

High sensitivity and wide bandwidth
Short Waves
FM band 88-108MHz
10dB
15MHz
sky noise, ?6dB_at_75MHz
Dipole Preamplifier noise
Analyzer noise
Spectrum measured from 1MHz to 150MHz at Nançay
10th PISA meeting
18
Present developments New active dipole antenna
no side lobes from 100 KHz to 70 MHz,
dipole-Decametric array interference pattern with
Cas.A sourceVery good astronomical performances
on a wide band
ECRS2006
19
CODALEMA
  • NEW Trigger 5 particle detectors (13 soon)
  • counting rate 1 evt / 7 min
  • energy threshold 1x1016eV
  • New dipole array on the North South axis

20
Transient detection and datation
Datation t
Threshold n.s
Noise s
Triggering time tagging
Filtered band
Full band
21
(No Transcript)
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