The Fluorescence Detector of the Pierre Auger Observatory (CALOR2010 Proceedings)

TL;DR

The Pierre Auger Observatory's fluorescence detector uses ultraviolet light from air showers to measure ultra-high energy cosmic rays, enabling precise, model-independent energy calibration through hybrid detection methods.

Contribution

This paper details the design and key measurements of the fluorescence detector, highlighting its role in calibrating cosmic ray energy measurements.

Findings

Successful detection of air fluorescence signals.

Hybrid events enable model-independent energy calibration.

Enhanced understanding of ultra-high energy cosmic rays.

Abstract

The Pierre Auger Observatory is a facility designed for the study of ultra-high energy cosmic rays. The Observatory combines two different types of detectors: a surface array of 1600 water Cherenkov stations placed on a 1.5 km triangular grid covering over 3000 km$^2$; and a fluorescence detector of 24 telescopes located in 4 buildings at the perimeter of the surface array. The fluorescence telescopes, each consisting of 440 photomultipliers, collect the ultraviolet light produced when the charged secondary particles in an air shower excite nitrogen molecules in the atmosphere. Because the intensity of the nitrogen fluorescence is proportional to the energy deposited in the atmosphere during the air shower, the air fluorescence measurements can be used to make a calorimetric measurement of the cosmic ray primary energy. Showers observed independently by the surface array and fluorescence telescopes, called hybrid events, are critical to the function of the Observatory, as they allow for a model-independent calibration of the surface detector. In this paper I describe the detector and the most important measurements.