On the measurement of the proton-air cross section using longitudinal shower profiles
arXiv:astro-ph/0612205 · doi:10.1016/j.nuclphysbps.2007.10.019
Abstract
In this paper, we will discuss the prospects of deducing the proton-air cross section from fluorescence telescope measurements of extensive air showers. As it is not possible to observe the point of first interaction directly, other observables closely linked to must be inferred from the longitudinal profiles. This introduces a dependence on the models used to describe the shower development. The most straightforward candidate for a good correlation to is the depth of shower maximum . We will discuss the sensitivity of an -based analysis on and quantify the systematic uncertainties arising from the model dependence, parameters of the reconstruction method itself and a possible non-proton contamination of the selected shower sample.
4 pages, Proceedings for ISVHECRI Weihei 2006