Anisotropy of ionospheric irregularities determined from the amplitude of satellite signals at a single receiver

Energy determination of cosmic ray showe

Energy determination of cosmic ray showers in surface arrays using signal inference at a single distance from the core

✍ G. Ros; G. Medina-Tanco; L. del Peral; J.C. D’Olivo; F. Arqueros; M.D. Rodríguez 📂 Article 📅 2009 🏛 Elsevier Science 🌐 English ⚖ 817 KB

In most high energy cosmic ray surface arrays, the primary energy is currently determined from the value of the lateral distribution function at a fixed distance from the shower core, r 0 . The value of r 0 is mainly related to the geometry of the array and is, therefore, considered as fixed indepen