Se p 20 04 Determination of the calorimetric energy in extensive air showers Henrique

نویسندگان

  • Fernando Catalani
  • José A. Chinellato
  • Carola Dobrigkeit
چکیده

The contribution of different components of an air shower to the total energy deposit in the atmosphere, for different angles and primary particles, was studied using the CORSIKA air shower simulation code. The amount of missing energy, parameterized in terms of the calorimetric energy, was calculated. The results show that this parameterization varies less than 1% with angle or observation level. The dependence with the primary mass is less than 5% and, with the high energy hadronic interaction model, less than 2%. The systematic error introduced by the use of just one parameterization of the missing energy correction function, for an equal mixture of proton and iron at 45, was calculated to be below 3%. We estimate the statistical error due to shower-to-shower fluctuations to be about 1%.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

A study on the lateral distribution of Cherenkov light in extensive air showers

The dependence of the lateral distribution of Cherenkov light in simulated extensive air showers to the energy and the mass of the primary cosmic rays has been studied. It has been shown that a previous claim about mass independent proportionality of shower energy to the total Cherenkov photon number is not valid in energies below EEAS ~ 1014 eV. We have found that the core distance of the so c...

متن کامل

Angular deviation of secondary charge particles in 1014-1016 eV extensive air showers: Constrains on application of hodoscopes

  Deviation angles of secondary electrons and muons in simulated extensive air showers were studied. The angles have wide distribution, whose width depends on energy cuts imposed on shower particles. In this work, variation of deviation angles with the energy of secondary particles, shower energy, primary direction, and core distance was investigated. The results put limitations on application ...

متن کامل

ar X iv : a st ro - p h / 04 02 30 0 v 1 1 2 Fe b 20 04 Properties of Extensive Air Showers ∗

Extensive air showers (EAS) are known for about 70 years to be cascades initiated by primary cosmic rays in the atmosphere. As such, they serve as connection to the highest particle energies nature is offering, especially at energies exceeding 10 eV where direct measurements of cosmic rays are hampered by the low primary flux. EAS can be viewed as tools for astroparticle physics. The main task ...

متن کامل

مشاهده ی پرتوهای کیهانی با آرایه ی البرز 1

The first phase of the Alborz Observatory Array (Alborz-1) consists of 20 plastic scintillation detectors each one with surface area of 0.25  spread over an area of  realized to the study of Extensive Air Showers around the knee at the Sharif University of Technology campus. The first stage of the project including construction and operation of a prototype system has now been completed and the ...

متن کامل

Fluorescence emission induced by extensive air showers in dependence on atmospheric conditions

Charged particles of extensive air showers (EAS), mainly electrons and positrons, initiate the emission of fluorescence light in the Earth’s atmosphere. This light provides a calorimetric measurement of the energy of cosmic rays. For reconstructing the primary energy from an observed light track of an EAS, the fluorescence yield in air has to be known in dependence on atmospheric conditions, li...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2004