T. Huege
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View article: Electric Field for Radio Detection of Inclined Air Showers in Three Polarizations
Electric Field for Radio Detection of Inclined Air Showers in Three Polarizations Open
View article: Cosmic-ray detection with LOFAR 2.0
Cosmic-ray detection with LOFAR 2.0 Open
View article: Overview of the CORSIKA 8 astroparticle simulation framework
Overview of the CORSIKA 8 astroparticle simulation framework Open
View article: Simulating radio emissions from particle showers in complex media with CORSIKA 8
Simulating radio emissions from particle showers in complex media with CORSIKA 8 Open
View article: Using SKA-low to detect PeV gamma-rays from Galactic Sources
Using SKA-low to detect PeV gamma-rays from Galactic Sources Open
View article: A Generative Neural Network for the Prediction of Radio Pulses from Extensive Air Showers
A Generative Neural Network for the Prediction of Radio Pulses from Extensive Air Showers Open
View article: Information Field Theory based Event Reconstruction for Cosmic Ray Radio Detectors
Information Field Theory based Event Reconstruction for Cosmic Ray Radio Detectors Open
View article: Reconstructing air showers using probabilistic forward modelling for LOFAR
Reconstructing air showers using probabilistic forward modelling for LOFAR Open
View article: Backtracking radio signals for the $X_\rm {max}$ measurement of extensive air showers: A new approach
Backtracking radio signals for the $X_\rm {max}$ measurement of extensive air showers: A new approach Open
View article: Fast and accurate simulation of the radio emission from cosmic ray air showers using template synthesis
Fast and accurate simulation of the radio emission from cosmic ray air showers using template synthesis Open
View article: From collider to cosmic rays: Pythia 8/Angantyr for air shower simulations in CORSIKA 8
From collider to cosmic rays: Pythia 8/Angantyr for air shower simulations in CORSIKA 8 Open
View article: Investigating double bump air showers with the SKA
Investigating double bump air showers with the SKA Open
Double-bump showers are a rare class of extensive air showers (EAS) predicted by Monte Carlo simulations. They occur when a high-energy secondary particle, the leading particle, travels significantly farther than the rest, creating a disti…
View article: Signal Model and Energy Reconstruction for the Radio Detection of Inclined Air Showers in the 50-200 MHz Frequency Band
Signal Model and Energy Reconstruction for the Radio Detection of Inclined Air Showers in the 50-200 MHz Frequency Band Open
View article: Simulating radio emission from extensive air showers with CORSIKA 8
Simulating radio emission from extensive air showers with CORSIKA 8 Open
View article: Determination of the energy scale of cosmic ray measurements using the Auger Engineering Radio Array
Determination of the energy scale of cosmic ray measurements using the Auger Engineering Radio Array Open
View article: Measuring the locations and properties of VHF sources emitted from an aircraft flying through high clouds
Measuring the locations and properties of VHF sources emitted from an aircraft flying through high clouds Open
We show that it is possible to locate the few places on the body of an airplane, while it is flying through high clouds, from which broad-band, pulsed, radiation is emitted at Very High Frequency (VHF) radio frequencies. This serendipitous…
View article: Information Field Theory based Event Reconstruction for Cosmic Ray Radio Detectors
Information Field Theory based Event Reconstruction for Cosmic Ray Radio Detectors Open
Detection of extensive air showers with radio antennas is an appealing technique in cosmic ray physics. However, because of the high level of measurement noise, current reconstruction methods still leave room for improvement. Furthermore, …
View article: The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC 2025)
The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC 2025) Open
The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses large surface arrays of antennas to look for the radio emissi…
View article: Generative Neural Network for Simulating Radio Emission from Extensive Air Showers
Generative Neural Network for Simulating Radio Emission from Extensive Air Showers Open
Cosmic ray shower detection using large radio arrays has gained significant traction in recent years. With massive improvements in signal modelling and microscopic simulations, the analysis of incoming events is still severely limited by t…
View article: Electric-Field Reconstruction for Radio Detection of Inclined Air Showers in Three Polarizations
Electric-Field Reconstruction for Radio Detection of Inclined Air Showers in Three Polarizations Open
Accurate reconstruction of the electric field produced by extensive air showers is essential for the radio-detection technique, as the key parameters of interest of the primary particles that generated the showers are the amplitude, polari…
View article: Signal Model and Energy Reconstruction for the Radio Detection of Inclined Air Showers in the 50-200 MHz Frequency Band
Signal Model and Energy Reconstruction for the Radio Detection of Inclined Air Showers in the 50-200 MHz Frequency Band Open
The radio emission of cosmic-ray air-showers changes significantly depending on parameters like signal frequency, magnetic field configuration and observing altitude. We use CoREAS simulations to adapt an existing signal model for the radi…
View article: LOFAR-style reconstruction of cosmic-ray air showers with SKA-Low
LOFAR-style reconstruction of cosmic-ray air showers with SKA-Low Open
Cosmic-ray air shower detection with the low-frequency part of the Square Kilometre Array (SKA) radio telescope is envisioned to yield very high precision measurements of the particle composition of cosmic rays between 1016 and 1018 eV. Th…
View article: SMIET: Synthesis Modelling In-air Emission using Templates
SMIET: Synthesis Modelling In-air Emission using Templates Open
The SMIET (Synthesis Modelling In-air Emission using Templates) software implements the template synthesis method. This method uses semi-analytical relations to synthesise the radio emission from cosmic ray air showers, using full Monte-Ca…
View article: Thunderstorm Charge Distribution Determination Using Cosmic Rays Induced Air Showers and Lightning Imaging at LOFAR
Thunderstorm Charge Distribution Determination Using Cosmic Rays Induced Air Showers and Lightning Imaging at LOFAR Open
The LOw Frequency ARray (LOFAR) radio telescope possesses the unique capability to measure ultra‐high energy cosmic rays as well as image lightning discharges. This study presents a comparison between the inferred thunderstorm charge struc…
View article: Ideas and Requirements for the Global Cosmic-Ray Observatory (GCOS)
Ideas and Requirements for the Global Cosmic-Ray Observatory (GCOS) Open
After a successful kick-off meeting in 2021. two workshops in 2022 and 2023 on the future Global Cosmic-Ray Observatory (GCOS) focused mainly on a straw man design of the detector and science possibilities for astro- and particle physics. …
View article: Electric field reconstruction with three polarizations for the radio detection of ultra-high energy particles
Electric field reconstruction with three polarizations for the radio detection of ultra-high energy particles Open
Accurate reconstruction of the electric field produced by Extensive Air Showers from the signals recorded by the antennas is essential for the radio detection technique, as the key parameters needed to retrieve information about the primar…
View article: Aperture correction for beamforming in the radiometric detection of ultrahigh energy cosmic rays
Aperture correction for beamforming in the radiometric detection of ultrahigh energy cosmic rays Open
For high-energy cosmic-ray physics, it is imperative to determine the mass and energy of the cosmic ray that initiated the air shower in the atmosphere. This information can be extracted from the longitudinal profile of the air shower. In …
View article: Aperture correction for Beamforming in radiometric detection of ultra-high energy cosmic rays
Aperture correction for Beamforming in radiometric detection of ultra-high energy cosmic rays Open
For high-energy cosmic-ray physics, it is imperative to determine the mass and energy of the cosmic ray that initiated the air shower in the atmosphere. This information can be extracted from the longitudinal profile of the air shower. In …
View article: Cosmic rays with LOFAR 2.0 - what’s next?
Cosmic rays with LOFAR 2.0 - what’s next? Open
The LOFAR radio telescope has been used to measure radio emission from cosmic-ray air showers in the $10^{16.5}-10^{18}$~eV range for over a decade. LOFAR is currently undergoing an upgrade (LOFAR 2.0) which will enable continuous observat…
View article: Applying template synthesis to the radio emission from air showers with generic geometries
Applying template synthesis to the radio emission from air showers with generic geometries Open