Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory

Identifieur interne : 000478 ( Istex/Checkpoint ); précédent : 000477; suivant : 000479

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Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory

Auteurs :

Source :

• Journal of Instrumentation [ 1748-0221 ] ; 2012-10-01.

RBID : ISTEX:1EE55C43610E960A24AE70CBC9F614B0B6A9E7C9

Descripteurs français

• Wicri :
  • geographic : Argentine.
  • topic : Enseignement supérieur, Niveau sonore, Physique nucléaire, Simulation.

English descriptors

• KwdEn :
  • Aachen germany, Absolute scale, Absolute value, Absolute values, Active bowtie antenna, Aera, Aera band, Aera site, Aire, Analyzer, Antenna, Antenna calculations, Antenna characteristics, Antenna directivity, Antenna gain, Antenna impedance, Antenna literature, Antenna model, Antenna models, Antenna response, Antenna sensitivity, Antenna sensor, Antenna structure, Antenna terminals, Antenna theory, Argentina, Argentinian pampa, Astron, Astroparticle physics, Attenuation loss, Auger, Auger engineering radio array, Autonomous detector stations, Band transmitters, Bandwidth, Beijing china, Beverage antenna, Biconical antenna, Buenos aires, Calibration, Calibration measurement, Calibration measurements, Calibration setup, Candidate antennas, Circuit diagram, Coaxial, Coaxial cable, Coaxial cables, Codalema, Codalema collaboration, Codalema experiment, Colorado state university, Common bandwidth, Complex functions, Complex propagation, Constant group delay, Continuous noise, Continuous radio signal, Convolution, Corresponding frequency, Cosmic rays, Czech republic, Detection techniques, Detector, Detector station, Detector stations, Different antennas, Different frequencies, Digital oscilloscopes, Dipole, Dipole antenna, Dipole antennas, Dipole loop, Dipole structure, Dirac pulse, Direct wave, Directional properties, Directivity, Dynamic spectra, Effective antenna length, Effective aperture, Electrical line length, Environmental conditions, European union, Framework program, Frequency, Frequency domain, Frequency range, Full frequency range, Galactic, Galactic background, Galactic noise, Galactic noise background, Galactic noise intensity, Galactic noise level, Galactic plane, Galactic radio background, Galactic signal, Galactic variation, Global phase, Ground plane, Group delay, Gure, Higher education, Highest frequencies, Ierre, Ierre auger collaboration, Impedance, Impedance mismatch, Incoming, Incoming direction, Incoming directions, Incoming signal, Incoming signals, Incoming voltage amplitude, Independent measurements, Infn, Input impedance, Instituto, Instrum, Intermediate transmission line, Intermediate transmission lines, Internal noise, Inverse fourier, Jinst, Jones antenna matrix, Karlsruhe, Karlsruhe institute, Large distances, Lawrence livermore, Load impedance, Logarithmic, Logarithmic scale, Loop antenna, Lower frequencies, Lpda, Lter elements, Maximum variation, Measurement bandwidth, Measurement equation, Measurement setup, Measurement simulation, Meth, Minor distortions, Mismatch, Multiple signal, Nacional, Nancay, Nancay radio observatory, Network analyzer, Next generation, Next setup stage, Noise level, Noise performance, Noise power, Noise ratio, Nucl, Nuclear physics, Numerical electromagnetics code, Observation direction, Observatorio pierre auger, Observatory, Ohmic resistor, Open circuit voltage, Other antennas, Parallel orientation, Partial gain, Partial response voltages, Particle detectors, Peak response, Phase difference, Phys, Physique nucl, Pierre auger collaboration, Pierre auger observatory, Plane gain, Plane wave, Polarization effects, Polarization factor, Polarization mismatch, Power calculation, Private communication, Radio astronomy, Radio background variation, Radio detection, Radio detector, Radio detector station, Radio detector stations, Radio emission, Radio polarimetry, Radio pulse, Radio pulses, Radio signal, Radio signals, Readout, Readout chain, Readout electronics, Readout impedance, Readout system, Receiver antenna, Relative permittivity, Relevant antenna characteristics, Response voltage, Right part, Rwth aachen university, Salla, Salla antenna, Salla antennas, Same hardware structure, Setup, Sezione, Sezione infn, Short periods, Shower axis, Shower signal, Shower signals, Side lobes, Sidereal, Sidereal time, Signal generator, Signal power, Signal shape, Simulation, Single frequencies, Single frequency, Single polarization direction, Slight changes, Software framework, Special interest, Spectral irradiance, Spider, Spider antenna, Spider lpda, Spider salla, Stations stage, Technical report, Technology campus, Terminal voltage, Test bench, Test measurements, Thevenin equivalent, Time delay, Time domain, Transfer factor, Transfer function, Transformer, Transient, Transient nature, Transient response, Transient response characteristics, Transient signal, Transient signals, Transmission line, Transmission line transformer, Transmission measurement, Transmitter, Transmitter antenna, Unit sphere, Unity vectors, Universidad, Universidade, Universidade estadual, Universit, Vector network analyzer, Vectorial, Vectorial phase information, Voltage amplitude, Voltage response, Wide frequency range, Zenith, Zenith angle, Zenith angle dependence, Zenith angle range, Zenith angles, Zenith direction, Zenith directions.
• Teeft :
  • Aachen germany, Absolute scale, Absolute value, Absolute values, Active bowtie antenna, Aera, Aera band, Aera site, Aire, Analyzer, Antenna, Antenna calculations, Antenna characteristics, Antenna directivity, Antenna gain, Antenna impedance, Antenna literature, Antenna model, Antenna models, Antenna response, Antenna sensitivity, Antenna sensor, Antenna structure, Antenna terminals, Antenna theory, Argentina, Argentinian pampa, Astron, Astroparticle physics, Attenuation loss, Auger, Auger engineering radio array, Autonomous detector stations, Band transmitters, Bandwidth, Beijing china, Beverage antenna, Biconical antenna, Buenos aires, Calibration, Calibration measurement, Calibration measurements, Calibration setup, Candidate antennas, Circuit diagram, Coaxial, Coaxial cable, Coaxial cables, Codalema, Codalema collaboration, Codalema experiment, Colorado state university, Common bandwidth, Complex functions, Complex propagation, Constant group delay, Continuous noise, Continuous radio signal, Convolution, Corresponding frequency, Cosmic rays, Czech republic, Detection techniques, Detector, Detector station, Detector stations, Different antennas, Different frequencies, Digital oscilloscopes, Dipole, Dipole antenna, Dipole antennas, Dipole loop, Dipole structure, Dirac pulse, Direct wave, Directional properties, Directivity, Dynamic spectra, Effective antenna length, Effective aperture, Electrical line length, Environmental conditions, European union, Framework program, Frequency, Frequency domain, Frequency range, Full frequency range, Galactic, Galactic background, Galactic noise, Galactic noise background, Galactic noise intensity, Galactic noise level, Galactic plane, Galactic radio background, Galactic signal, Galactic variation, Global phase, Ground plane, Group delay, Gure, Higher education, Highest frequencies, Ierre, Ierre auger collaboration, Impedance, Impedance mismatch, Incoming, Incoming direction, Incoming directions, Incoming signal, Incoming signals, Incoming voltage amplitude, Independent measurements, Infn, Input impedance, Instituto, Instrum, Intermediate transmission line, Intermediate transmission lines, Internal noise, Inverse fourier, Jinst, Jones antenna matrix, Karlsruhe, Karlsruhe institute, Large distances, Lawrence livermore, Load impedance, Logarithmic, Logarithmic scale, Loop antenna, Lower frequencies, Lpda, Lter elements, Maximum variation, Measurement bandwidth, Measurement equation, Measurement setup, Measurement simulation, Meth, Minor distortions, Mismatch, Multiple signal, Nacional, Nancay, Nancay radio observatory, Network analyzer, Next generation, Next setup stage, Noise level, Noise performance, Noise power, Noise ratio, Nucl, Nuclear physics, Numerical electromagnetics code, Observation direction, Observatorio pierre auger, Observatory, Ohmic resistor, Open circuit voltage, Other antennas, Parallel orientation, Partial gain, Partial response voltages, Particle detectors, Peak response, Phase difference, Phys, Physique nucl, Pierre auger collaboration, Pierre auger observatory, Plane gain, Plane wave, Polarization effects, Polarization factor, Polarization mismatch, Power calculation, Private communication, Radio astronomy, Radio background variation, Radio detection, Radio detector, Radio detector station, Radio detector stations, Radio emission, Radio polarimetry, Radio pulse, Radio pulses, Radio signal, Radio signals, Readout, Readout chain, Readout electronics, Readout impedance, Readout system, Receiver antenna, Relative permittivity, Relevant antenna characteristics, Response voltage, Right part, Rwth aachen university, Salla, Salla antenna, Salla antennas, Same hardware structure, Setup, Sezione, Sezione infn, Short periods, Shower axis, Shower signal, Shower signals, Side lobes, Sidereal, Sidereal time, Signal generator, Signal power, Signal shape, Simulation, Single frequencies, Single frequency, Single polarization direction, Slight changes, Software framework, Special interest, Spectral irradiance, Spider, Spider antenna, Spider lpda, Spider salla, Stations stage, Technical report, Technology campus, Terminal voltage, Test bench, Test measurements, Thevenin equivalent, Time delay, Time domain, Transfer factor, Transfer function, Transformer, Transient, Transient nature, Transient response, Transient response characteristics, Transient signal, Transient signals, Transmission line, Transmission line transformer, Transmission measurement, Transmitter, Transmitter antenna, Unit sphere, Unity vectors, Universidad, Universidade, Universidade estadual, Universit, Vector network analyzer, Vectorial, Vectorial phase information, Voltage amplitude, Voltage response, Wide frequency range, Zenith, Zenith angle, Zenith angle dependence, Zenith angle range, Zenith angles, Zenith direction, Zenith directions.

Url:

• https://api.istex.fr/document/1EE55C43610E960A24AE70CBC9F614B0B6A9E7C9/fulltext/pdf

DOI: 10.1088/1748-0221/7/10/P10011

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