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Some Results of the Codalema
   Experiment at Nançay
              Ahmed Rebai
        Subatech Laboratory Nantes
                  JED le Mans 30 June 2011


   •   Introduction
   •   North-South Asymmetry
   •   Energy Calibration
   •   Reconstruction of the radio wave emission center
Motivations
                                                      Auger data 2008
  Many unanserewed questions about cosmic rays with
  energies in the range of joule (~ 1019 eV )


   Nature of those particles ?
   Astrophysical Sources ?
   A limit in their energies ?


Radio-detection as a complementary detection
technique ?
Surface
Duty Cycle
Cost, simplicity
Angular resolution , Energetic resolution ?
Nature of the cosmic rays ?

    Since 2003 installation of CODALEMA
    experiment at Nançay: as demonstration of
    the feasibility and potential of this method
Motivations
Cosmic rays spectrum

                       CODALEMA energy
                       range




                            Energy Threshold : 5.1015 eV
                            Trigger Rate : 1 evt/ 7 mn
                            Analysis Threshold : 5.1016 eV
                            Counting rate : 1 good evt/3 days
                            Detection surface : 0.25 km2
CODALEMA Experiment@Nançay
Codalema actual setup                   Array of short antennas
                                        -21 dipole antennas E-W
                                        - 3 dipole antennas N-S




                                                  Decametric array
                                                  18 groups of 8 log-periodic
                                                  phased antennas
Scintillator array
17 scintillator
=>Experiment Trigger
=> Energy Estimator
Radio Emission

10% e-,e+
                                           e-/e+ deflection under the geomagnectic field
                                           effect  dipole emission, transverse
                                           current, synchrotron radiation
                           +           -   Time variation of the negatif charge excess
                                           monopole emission
                                           Time variation of the charged particles
                                           number
            Radio Signal



                                                 Frequency ~ 100 MHz
                                                 Amplitude ~ 100 µV.m-1
                                                 Duration ~ 1 ns – 100 ns
                           Xmax
                   Maximum shower
                   development Nmax
                   maximum particles
                   number
Detection method
                                                                   Numeric filter in the 23-83
                                                                         MHz band

                                                                  AM
                                                                                 FM
Amplitude [V]




                                                       + Corrections : time delay,
                          Time [s]                     attenuation, antennas gain


                1 event = 2 physical quantities / antenna ( amplitude Vi , time ti , … )
Arrivals direction reconstruction
                                  •Hypothesis: plane wave front Ux.x+Uy.y+Uz.z + cte =0
                                  •Maximum amplitude time ti on antennas




           IG11      ID32   IA1
                                                   σ = 1.6°


ITrigger          ID98




                                  Arrival direction
                                  Θ : Zenithal angle
                                  Φ : Azimuthal angle
North
                               Emission mechanism

                               Detection threshold correlated
                               with arrivals directions
                                Geomagnetic Effect


                  B
                           Radio Signal Amplitude ~ |VxB|E-W

          South                D.Ardouin & al Astro.ph 31 2009
  Polarization E-O                                                   CODALEMA Model
|VxB|E-W minimum      Zenith      |VxB|E-W maximum               (also SELFAS2, ReAIRES)




                  B
                                                         confirmed at RAuger@Auger
                         θ=27°
                                               North     Argentina (magnetic field
 South                                                   inversed in the southern
                                                         hemisphere)
Lateral Profil Distribution
                    Radio signal lateral profil in the ground
                    => Allan formula : E = E0.exp(-d/d0)




                                   E0 on the shower axis
                                   d0 distance of the shower decay
                                   (X0, Y0) shower core
                                   1 event = (E0, d0, X0, Y0)




 Use of E0 as an energy estimator of the primary particle
Energy Correlation


                                         Ep estimated with the CIC
                                       method (Constant intensity Cut)


                                               ΔEp/Ep ~ 30 %
                                               ΔE0/E0 < 10 %



                           E0 ~ Epα avec α ~ 1.0 
                          linear dependency
                                                Calibration depends on :
                                                E0 errors
                                                Ep errors


E0 =a Ep + b  Radio calibration Egerbe =(1/a)*E0 – b/a
Radius of Curvature
Approximation 0  a plane
  wave front
                                 Approximation 1 
                                 Non planar wave front +
                                 Emission center in a distance R




               Time [s]
Radius of Curvature
                              Systematic gap / planewave front  Non planar
                                  wavefront
                                 U x  x  U y  y  U z  z  (U x  x fta  U y  y fta  U z z fta )  0
σt= 10 ns                              U x  x  U y  y  (U x  x fta  U y  y fta )
                                 d
                                                     U x U y Uz
                                                         2       2       2

               Data
                                 tth  d
                                           c
                                 First tagged antenna t0 .
                                tth – t0 = Expected delay
                                tps – t0 = Experimental delay

  Simulation


                           Example of a simulation (spherical wave front):
                           Delay decrease  R increase  Far emission center 
                            planewave front
                           Delay increase  R decrease  Near emission center 
                            Curved front
Radius of curvature Estimation : Fitting of the
                                                   waveplan front gap
 •Hypothesis = parabolic gap

  
c. t   i
        max
              t   i
                    pred
                               a      
                                    1  r r2 r r2 r r
                                                            
                                    2.R . xi  xc  yi  yc  zi  zc
                                                                         
                                                                          2

                                    c

       5 free parameter model :
                                                                                        σ = 3m

       Shower Core coordinate xc, yc et zc
       Radius of curvature Rc  Emission center




                               4 km




                                                     ?                         Radius of Curvature distribution
                                                                               maximum ~ 4 km …
                                                                               … But interpretations difficulties
                                                                               (Very large Radius observed)
Towards a direct shower energy estimator
z
             radio             Hypothesis : Emission Center = Xmax
         X   max



                                                  f Linsley ( Rc . cos( ))
                                        X max 
                                                         cos( )
    θ   Rc
                     sol


                              Greisen Model  Shower of only e-/e+
                              Xmax = X0ln (Ep/E0)  Ep
                              X0 = 36.7 g.cm-2
                              E0 = 83 MeV
Towards a autonomous radiodetection array : CODALEMA3


60 automous stations to be installed at Nançay during 2011
    Array with 1 km2 of surface
Exploration in continuity of the Codalema physic
programme
Conclusions
Faisability of radiodedection with CODALEMA 2:
 Detection of the radio signal induced by the shower
  developpement
 Emission mechanism : geomagnetic effect
 Energie Correlation
New analysis method : Rc
Exploration of CODALEMA 3 (autonomous station)



                     Thank you

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3MPL Graduate School Days presentation

  • 1. Some Results of the Codalema Experiment at Nançay Ahmed Rebai Subatech Laboratory Nantes JED le Mans 30 June 2011 • Introduction • North-South Asymmetry • Energy Calibration • Reconstruction of the radio wave emission center
  • 2. Motivations Auger data 2008 Many unanserewed questions about cosmic rays with energies in the range of joule (~ 1019 eV ) Nature of those particles ? Astrophysical Sources ? A limit in their energies ? Radio-detection as a complementary detection technique ? Surface Duty Cycle Cost, simplicity Angular resolution , Energetic resolution ? Nature of the cosmic rays ? Since 2003 installation of CODALEMA experiment at Nançay: as demonstration of the feasibility and potential of this method
  • 3. Motivations Cosmic rays spectrum CODALEMA energy range Energy Threshold : 5.1015 eV Trigger Rate : 1 evt/ 7 mn Analysis Threshold : 5.1016 eV Counting rate : 1 good evt/3 days Detection surface : 0.25 km2
  • 4. CODALEMA Experiment@Nançay Codalema actual setup Array of short antennas -21 dipole antennas E-W - 3 dipole antennas N-S Decametric array 18 groups of 8 log-periodic phased antennas Scintillator array 17 scintillator =>Experiment Trigger => Energy Estimator
  • 5. Radio Emission 10% e-,e+ e-/e+ deflection under the geomagnectic field effect  dipole emission, transverse current, synchrotron radiation + - Time variation of the negatif charge excess monopole emission Time variation of the charged particles number Radio Signal Frequency ~ 100 MHz Amplitude ~ 100 µV.m-1 Duration ~ 1 ns – 100 ns Xmax Maximum shower development Nmax maximum particles number
  • 6. Detection method Numeric filter in the 23-83 MHz band AM FM Amplitude [V] + Corrections : time delay, Time [s] attenuation, antennas gain 1 event = 2 physical quantities / antenna ( amplitude Vi , time ti , … )
  • 7. Arrivals direction reconstruction •Hypothesis: plane wave front Ux.x+Uy.y+Uz.z + cte =0 •Maximum amplitude time ti on antennas IG11 ID32 IA1 σ = 1.6° ITrigger ID98 Arrival direction Θ : Zenithal angle Φ : Azimuthal angle
  • 8. North Emission mechanism Detection threshold correlated with arrivals directions  Geomagnetic Effect B  Radio Signal Amplitude ~ |VxB|E-W South D.Ardouin & al Astro.ph 31 2009 Polarization E-O CODALEMA Model |VxB|E-W minimum Zenith |VxB|E-W maximum (also SELFAS2, ReAIRES) B confirmed at RAuger@Auger θ=27° North Argentina (magnetic field South inversed in the southern hemisphere)
  • 9. Lateral Profil Distribution Radio signal lateral profil in the ground => Allan formula : E = E0.exp(-d/d0) E0 on the shower axis d0 distance of the shower decay (X0, Y0) shower core 1 event = (E0, d0, X0, Y0)  Use of E0 as an energy estimator of the primary particle
  • 10. Energy Correlation Ep estimated with the CIC method (Constant intensity Cut) ΔEp/Ep ~ 30 % ΔE0/E0 < 10 % E0 ~ Epα avec α ~ 1.0  linear dependency Calibration depends on : E0 errors Ep errors E0 =a Ep + b  Radio calibration Egerbe =(1/a)*E0 – b/a
  • 11. Radius of Curvature Approximation 0  a plane wave front Approximation 1  Non planar wave front + Emission center in a distance R Time [s]
  • 12. Radius of Curvature Systematic gap / planewave front  Non planar wavefront U x  x  U y  y  U z  z  (U x  x fta  U y  y fta  U z z fta )  0 σt= 10 ns U x  x  U y  y  (U x  x fta  U y  y fta ) d U x U y Uz 2 2 2 Data tth  d c First tagged antenna t0 . tth – t0 = Expected delay tps – t0 = Experimental delay Simulation  Example of a simulation (spherical wave front):  Delay decrease  R increase  Far emission center  planewave front  Delay increase  R decrease  Near emission center  Curved front
  • 13. Radius of curvature Estimation : Fitting of the waveplan front gap •Hypothesis = parabolic gap  c. t i max t i pred   a   1  r r2 r r2 r r      2.R . xi  xc  yi  yc  zi  zc   2  c 5 free parameter model : σ = 3m Shower Core coordinate xc, yc et zc Radius of curvature Rc  Emission center 4 km ? Radius of Curvature distribution maximum ~ 4 km … … But interpretations difficulties (Very large Radius observed)
  • 14. Towards a direct shower energy estimator z radio Hypothesis : Emission Center = Xmax X max f Linsley ( Rc . cos( )) X max  cos( ) θ Rc sol Greisen Model  Shower of only e-/e+ Xmax = X0ln (Ep/E0)  Ep X0 = 36.7 g.cm-2 E0 = 83 MeV
  • 15. Towards a autonomous radiodetection array : CODALEMA3 60 automous stations to be installed at Nançay during 2011 Array with 1 km2 of surface Exploration in continuity of the Codalema physic programme
  • 16. Conclusions Faisability of radiodedection with CODALEMA 2:  Detection of the radio signal induced by the shower developpement  Emission mechanism : geomagnetic effect  Energie Correlation New analysis method : Rc Exploration of CODALEMA 3 (autonomous station) Thank you