Abstract

The Electron Light Source(ELS) is a new light source for the absolute energy calibration of cosmic ray Fluorescence Detector(FD) telescopes. The ELS is a compact electron linear accelerator with a typical output of 109 electrons per pulse at 40 MeV. We fire the electron beam vertically into the air 100 m in front of the telescope. The electron beam excites the gases of the atmosphere in the same way as the charged particles of the cosmic ray induced extensive air shower. The gases give off the same light with the same wavelength dependence. The light passes through a small amount of atmosphere and is collected by the same mirror and camera with their wavelength dependence. In this way we can use the electron beam from ELS to make an end-to-end calibration of the telescope. In September 2010, we began operation of the ELS and the FD telescopes observed the fluorescence photons from the air shower which was generated by the electron beam. In this article, we will reort the status of analysis of the absolute energy calibration with data which was taken in September 2010, and beam monitor study in November 2011.

Highlights

  • OF Electron Light Source (ELS)Ultra-high energy cosmic rays (UHECR) are the highest energy charged particles coming from extragalactic sources

  • We used the data of two telescopes which are located in front of ELS

  • We used the FADC counts which are normalized with total FADC counts of these telescopes

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Summary

INTRODUCTION

Ultra-high energy cosmic rays (UHECR) are the highest energy charged particles coming from extragalactic sources. Their sources, chemical composition, and the mechanism of generation, acceleration, and propagation are not understood. One of which is the Telescope Array (TA) located in the west desert of Utah in the U.S and started taking data since May of 2008. PAO is a hybrid detector consisting of 1600 water cherenkov surface detectors and 24 FD[6][7][8][9]. At the Black Rock FD station, and can fire a upward going electron beam through the field of view of the telescopes. We started the beam operation from September 2010[13]

BEAM OPERATION
STATUS OF DATA ANALYSIS
Monte Carlo simulation
BEAM MONTOR STUDY
SUMMARY
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