Investigations of the radio signal of inclined showers with LOPES
Creators
- 1. National Institute of Physics and Nuclear Engineering, Bucharest (Romania)
- 2. Karlsruhe Institute of Technology (KIT), Institut für Kernphysik, 76021 Karlsruhe (Germany)
- 3. Karlsruhe Institute of Technology (KIT), Institut für Experimentelle Kernphysik, 76021 Karlsruhe (Germany)
- 4. Karlsruhe Institute of Technology (KIT), Institut für Prozessdatenverarbeitung und Elektronik, 76021 Karlsruhe (Germany)
- 5. Radboud University Nijmegen, Department of Astrophysics (Netherlands)
- 6. Dipartimento di Fisica Generale dell' Universita Torino (Italy)
- 7. Max-Planck-Institut für Radioastronomie Bonn (Germany)
- 8. Universität Siegen, Fachbereich Physik (Germany)
- 9. INAF Torino, Istituto di Fisica dello Spazio Interplanetario (Italy)
Description
We report in this paper on an analysis of 20 months of data taken with LOPES. LOPES is radio antenna array set-up in coincidence with the Grande array, both located at the Karlsruhe Institute of Technology, Germany. The data used in this analysis were taken with an antenna configuration composed of 30 inverted V-shape dipole antennas. We have restricted the analysis to a special selection of inclined showers - with zenith angle θ>40∘. These inclined showers are of particular interest because they are the events with the largest geomagnetic angles and are therefore suitable to test emission models based on geomagnetic effects.The reconstruction procedure of the emitted radio signal in EAS uses as one ingredient the frequency-dependent antenna gain pattern which is obtained from simulations. Effects of the applied antenna model in the calibration procedure of LOPES are studied. In particular, we have focused on one component of the antenna, a metal pedestal, which generates a resonance effect, a peak in the amplification pattern where it is the most affecting high zenith angles, i.e. inclined showers. In addition, polarization characteristics of inclined showers were studied in detail and compared with the features of more vertical showers for the two cases of antenna models, with and without the pedestal.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.nima.2010.11.141Additional details
Identifiers
- DOI
- 10.1016/j.nima.2010.11.141;
- PII
- S0168-9002(10)02688-4;
Publishing Information
- Journal Title
- Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
- Journal Volume
- 662
- Journal Issue
- Suppl.1
- Journal Page Range
- p. S85-S88
- ISSN
- 0168-9002
- CODEN
- NIMAER
Conference
- Title
- 4. international workshop on acoustic and radio EeV neutrino detection activities
- Acronym
- ARENA 2010
- Dates
- 29 Jun - 2 Jul 2010
- Place
- Nantes (France)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44002418
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- AIR; ANTENNAS; CALIBRATION; CONFIGURATION; COSMIC SHOWERS; DIPOLES; EMISSION; FREQUENCY DEPENDENCE; GAIN; MESONS; METALS; POLARIZATION; SIMULATION
- Descriptors DEC
- AMPLIFICATION; BOSONS; COSMIC RADIATION; ELECTRICAL EQUIPMENT; ELEMENTARY PARTICLES; ELEMENTS; EQUIPMENT; FLUIDS; GASES; HADRONS; IONIZING RADIATIONS; MULTIPOLES; RADIATIONS; SECONDARY COSMIC RADIATION; SHOWERS
Optional Information
- Copyright
- Copyright (c) 2010 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.