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Principal Component Analysis (PCA) of the ultra high energy extensive air ... Fernando Catalani, Jun Takahashi e Jos Augusto Chinellato. DRCC IFGW. UNICAMP ... – PowerPoint PPT presentation

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Title: Apresentao do PowerPoint


1
Principal Component Analysis (PCA) of the ultra
high energy extensive air showers longitudinal
profile
Fernando Catalani, Jun Takahashi e José Augusto
Chinellato DRCC IFGW UNICAMP
2
  • Our knowledge of the mass composition of the
    cosmic rays of highest energy (above 0.1EeV) is
    deficient.
  • Measurement of the mass of this cosmic rays is
    necessary to understand their origin and
    propagation.
  • Top-Down models predict mainly photons and
    protons while Botton-Up models propose protons
    and heavy nuclei.

3
  • The detection of shower maximum depth via
    fluorescence is one method to study mass
    composition.
  • The study of Longitudinal Profile of extensive
    air showers with the fluorescent light technique
    was implemented by the Fly's eye experiment.
  • Recently the Fluorescence Detector (FD) of Pierre
    Auger has started to collect data.
  • A large amount of data will be produced and new
    and accurate data analysis procedures are
    welcome.

4
PCA Principal Component Analysis
  • The pca is a very useful tool widely used.
  • The basic idea is to project the raw data onto a
    few dominant eigenvectors with large variance in
    order to reduce the dimension, noise of the
    original data.
  • The new basis provides a simple description and
    can reveal underlying characteristics of the
    original data set.

5
Parameters Nmax number of particles at the
maximum. Xmax- depth of the shower maximum. s -
width of profile. Asymmetry of the
profile 4000 CORSIKA Showers
Nmax
s
Xmax
6
Distribution of Xmax
Energy 1.1018 eV
7
Distribution of Xmax and parameter f4 (PCA)
MF(?Fe- ?p)/sqrt(?fe2 ?p2)
Energy 1.1018 eV
8
Iron and Proton separation in 1018 eV and 1017 eV
p3 PCA applied over proton f4 PCA applied
over iron
9
Distribution of Xmax and parameter f4 (PCA)
Energy 1.1017 eV
10
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11
Xmax for different energies
12
f4 parameter for different energies
13
Merit Factor X Energy
14
Conclusions
  • PCA over FD parameters (Nmax, Xmax, ?, and
    assymetry) brings better results concerning mass
    composition than usual Xmax analysis.
  • Further improvements will take into account other
    primaries than iron and proton.
  • PCA over surface detector variables.

15
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16
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