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Latest results of the Codalema Experiment
                                                                                                                                              Rebai Ahmed
                                                                                                                     Subatech Laboratoire de physique subatomique et des technologies
                                                                                                                                 associées Nantes France IN2P3/CNRS
                                                                                                                                  On behalf the Codalema Collaboration
                                                                                                                                     ahmed.rebai@subatech.in2p3.fr




                                   Codalema Detectors                                                                                                                            Emission Mechanism
                Since 2002, Codalema experience located                                                                                                  Observation: NS asymmetry
                on the radio observatory site at Nançay
                                                                                                                                                         Codalema observes a large asymmetry in the
                (France) (47.3°N, 2.1°E and 137 m above
                                                                                                                                                         arrival directions between the North and the
                sea level) aims to study the potential of the
                                                                                                                                                         South.
                radiodetection technique of cosmic rays in

                                                                            400 m
                the 1016 eV energy range (detection                                                                                                       N                           322
                                                                                                                                                              South    Events
                                                                                                                                                                                            0 . 188
                threshold) to 1018 eV (upper limit imposed                                                                                                N                          1708
                                                                                                                                                              North    Events
                by the area surface).
                                                                                                                                                         This ratio is stable in time, with increasing
                In this regard, Codalema contains:                                                              600 m                                    statistics (see [1]).
                Scintillator array: (17 scintillator)                                                                                                   This effect can not be due to a detector
                gives the trigger signal for the                                                                                                         bias the scintillator array has a flat azimuthal
                experiment and an estimation of                                                                                                          distribution
                primary particle energy.
                                                                                                                                                        Geomagnetic effect
                Short active antennas array: 21
                                                                                                                                                        The local geomagnetic field may be the main
                antennas with E-W polarization & 3                                                                                                      cause of this asymmetry through the action of
                antennas with NS polarization. The                                                                                                      Lorentz force on the charged particles.
                main array.
                                                                                                                                                        Suppose 2 EAS initiated by 2 primary
                Decametric array: 18 groups of 8       Dipole antenna: 2*60 cm                                                                         particles of the same energy interacted in the
                                                        Al arms, simple and                                       Log-periodic antenna
                                                                                                                                                        same altitude. The shower from the North is ┴
                log-periodic phased antennas            cheap, isotropic pattern
                                                                                                                                                        to the geomagnetic field which gives a
                studies the electric field topology at                                                                                                  maximum |v^B|  strong radio signal that
                small scale (< 100 m).            Numeric filter in the                                                                                 exceeds the Codalema detection threshold.
                                                          23-83 MHz band
                                                          AM
                                                                                         FM
                                                                                                                   + some
                                                                                                                   Corrections :
                                                                                                                                                          Geomagnetic Model
                                                                                                                   Time delay
                                                                                                                                                        E (v  B)eEW    sin( )  cos2 ( )  LobeEW
                                                                                                                                                                               
Amplitude [V]




                                                                                                                   Attenuation
                                                                                                                   Antennas gain



                                                    1 event = 2 physical quantities per
                             Time [s]                 antenna ( amplitude Vi , time ti)



                                    Energy Calibration                                                                                                                            Radius of Curvature
                                                                                                                                                          The radius of curvature of the radio wave front can be a very good
                                                                                                                                                          discriminant variables that permet to distinguish between shower initiated by
                                                                                                                                                          protons, heavy ions, photons and neutrinos.


                                                                                                                                                        Approximation 0  a plane wave front
                                                                                                                                                        Approximation 1 Non planar wave front
                                                                                                                                                                +Emission center in a distance R




            Radio signal lateral profil in the groundAllan formula : E = E0.exp(-d/d0)                                                                We use a parabolic model to fit the radius
                                                                                                                                                       of curvature.
                                                                                                                                                       Our reconstruction is not based upon
                E0 on the shower axis
                                                                                                                                                       adjusting the wavefront shape which has a
                d0 distance of the
                                                                                                                                                       complicated geometry dependent on the
                shower decay                                                        Calibration depends on :
                                                                                    E0 errors                                                         shower developpement.
                (X0, Y0) shower core                                              Ep errors
                                                           E (v  B )eEW    sin( )  cos 2 ( )  LobeEW
                1 event = (E0, d0, X0, Y0)                                          ΔEp/Ep ~ 30 %
                                                                                    ΔE0/E0 < 10 %


The energy of the primary particle is                                                                                                                     Radius of Curvature distribution
estimated with the CIC method                                                                                                                             maximum ~ 4 km …
(Constant intensity Cut)                                                                                                                                  … But interpretations difficulties (Very
                                                                                                                      N
                                                                                                                 2  
                                                                                                                            yi  (b  a  xi )2         large Radius observed)
                                                                                                                     i 1     y  a 2   x2
                                                                                                                               2
                                                                                                                                 i           i

                   E0 ~ Epα avec α ~ 1.0 
                  linear dependency                                                                                                                        … Next step: Chemical composition of
                                                                                                                                                           UHECR ? …

                          E0 =a Ep + b  Radio calibration EShower =(1/a)*E0 – b/a



                                                                                 Faisability of radiodedection with CODALEMA 2:                                   References:

                   Conclusions &                                                 
                                                                                 
                                                                                           Detection of the radio signal induced by the shower developpement
                                                                                           Emission mechanism : geomagnetic effect
                                                                                                                                                                  [1] D.Ardouin & al., Astro Ph 31 2009
                                                                                                                                                                  pages 192-200 Goemagnetic origin of

                   Perspectives                                                           Energy Correlation                                                     the radio emission …
                                                                                          New analysis method : Rc
                                                                                          Exploration of CODALEMA 3 (autonomous station) (see Diego Torres poster)

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  • 1. Latest results of the Codalema Experiment Rebai Ahmed Subatech Laboratoire de physique subatomique et des technologies associées Nantes France IN2P3/CNRS On behalf the Codalema Collaboration ahmed.rebai@subatech.in2p3.fr Codalema Detectors Emission Mechanism Since 2002, Codalema experience located Observation: NS asymmetry on the radio observatory site at Nançay Codalema observes a large asymmetry in the (France) (47.3°N, 2.1°E and 137 m above arrival directions between the North and the sea level) aims to study the potential of the South. radiodetection technique of cosmic rays in 400 m the 1016 eV energy range (detection N 322 South  Events   0 . 188 threshold) to 1018 eV (upper limit imposed N 1708 North  Events by the area surface). This ratio is stable in time, with increasing In this regard, Codalema contains: 600 m statistics (see [1]). Scintillator array: (17 scintillator) This effect can not be due to a detector gives the trigger signal for the bias the scintillator array has a flat azimuthal experiment and an estimation of distribution primary particle energy. Geomagnetic effect Short active antennas array: 21 The local geomagnetic field may be the main antennas with E-W polarization & 3 cause of this asymmetry through the action of antennas with NS polarization. The Lorentz force on the charged particles. main array. Suppose 2 EAS initiated by 2 primary Decametric array: 18 groups of 8 Dipole antenna: 2*60 cm particles of the same energy interacted in the Al arms, simple and Log-periodic antenna same altitude. The shower from the North is ┴ log-periodic phased antennas cheap, isotropic pattern to the geomagnetic field which gives a studies the electric field topology at maximum |v^B|  strong radio signal that small scale (< 100 m). Numeric filter in the exceeds the Codalema detection threshold. 23-83 MHz band AM FM + some Corrections : Geomagnetic Model Time delay E (v  B)eEW    sin( )  cos2 ( )  LobeEW  Amplitude [V] Attenuation Antennas gain 1 event = 2 physical quantities per Time [s] antenna ( amplitude Vi , time ti) Energy Calibration Radius of Curvature The radius of curvature of the radio wave front can be a very good discriminant variables that permet to distinguish between shower initiated by protons, heavy ions, photons and neutrinos. Approximation 0  a plane wave front Approximation 1 Non planar wave front +Emission center in a distance R Radio signal lateral profil in the groundAllan formula : E = E0.exp(-d/d0) We use a parabolic model to fit the radius of curvature. Our reconstruction is not based upon E0 on the shower axis adjusting the wavefront shape which has a d0 distance of the complicated geometry dependent on the shower decay Calibration depends on : E0 errors shower developpement. (X0, Y0) shower core Ep errors E (v  B )eEW    sin( )  cos 2 ( )  LobeEW 1 event = (E0, d0, X0, Y0) ΔEp/Ep ~ 30 % ΔE0/E0 < 10 % The energy of the primary particle is Radius of Curvature distribution estimated with the CIC method maximum ~ 4 km … (Constant intensity Cut) … But interpretations difficulties (Very N 2   yi  (b  a  xi )2 large Radius observed) i 1  y  a 2   x2 2 i i E0 ~ Epα avec α ~ 1.0  linear dependency … Next step: Chemical composition of UHECR ? … E0 =a Ep + b  Radio calibration EShower =(1/a)*E0 – b/a Faisability of radiodedection with CODALEMA 2: References: Conclusions &   Detection of the radio signal induced by the shower developpement Emission mechanism : geomagnetic effect [1] D.Ardouin & al., Astro Ph 31 2009 pages 192-200 Goemagnetic origin of Perspectives  Energy Correlation the radio emission …  New analysis method : Rc  Exploration of CODALEMA 3 (autonomous station) (see Diego Torres poster)