11–14 Oct 2016
Kyoto Research Park
Japan timezone

Session

Oct.12AM1

Oct.12AM1
12 Oct 2016, 09:00
Kyoto Research Park

Kyoto Research Park

Chudouji Awatacho 93, Shimogyo-ku Kyoto , Japan, 600-8815

Conveners

Oct.12AM1

  • Takashi Sako (Nagoya University (JP))

Presentation materials

There are no materials yet.

  1. Matthias Plum
    12/10/2016, 09:00

    As a hybrid cosmic ray detector, the Pierre Auger Observatory can measure the longitudinal air shower
    development with the fluorescence detector, and the lateral distribution of particles reaching the ground
    with the surface detector. We report on the measurements of the first two moments of the Xmax
    distributions measured as a function of energy with the fluorescence detector and convert them...

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  2. John Belz (University of Utah)
    12/10/2016, 09:25

    The chemical composition of ultrahigh energy cosmic rays (UHECR) is studied primarily through observations of the depth of airshower maximum (Xmax), as seen by nitrogen fluorescence telescopes. The Telescope Array (TA) observatory measures Xmax using both stereo fluorescence detectors and fluorescence/ground array hybrid detection to accurately determine extensive air shower geometry. We...

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  3. William Hanlon (University of Utah)
    12/10/2016, 09:45
  4. Dr Darko Veberic (Karlsruhe Institute of Technology (DE))
    12/10/2016, 10:05

    The muon content of extensive air showers produced by the ultra-high energy cosmic rays is an observable sensitive to the composition of the primary particle and to the properties of hadronic interactions driving the air-shower cascade. We present different methods to estimate the muon number at the ground and the muon production depth using measurements of the longitudinal, lateral, and...

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