A. Corstanje
YOU?
Author Swipe
View article: Cosmic-ray detection with LOFAR 2.0
Cosmic-ray detection with LOFAR 2.0 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: On the performance of air shower reconstruction with the SKA-Low radio telescope
On the performance of air shower reconstruction with the SKA-Low radio telescope Open
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: 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: Cosmic ray detection with the LOFAR radio telescope
Cosmic ray detection with the LOFAR radio telescope Open
The LOw Frequency ARray (LOFAR) has successfully measured cosmic rays for over a decade now. With its dense core of antenna fields in the Netherlands, it is an ideal tool for studying the radio emission from extensive air showers in the 10…
View article: Cosmic ray observations with the Square Kilometer Array
Cosmic ray observations with the Square Kilometer Array Open
The low-frequency part of the SKA, to be built in Australia, will have an extremely high antenna density of roughly 60,000 antennas within one square kilometer, and is the perfect site for high-resolution studies of air showers. Individual…
View article: Cosmic ray detection with the LOFAR radio telescope
Cosmic ray detection with the LOFAR radio telescope Open
The LOw Frequency ARray (LOFAR) has successfully measured cosmic rays for over a decade now. With its dense core of antenna fields in the Netherlands, it is an ideal tool for studying the radio emission from extensive air showers in the $1…
View article: LOFAR discovery of a quiet emission mode in PSR B0823+26
LOFAR discovery of a quiet emission mode in PSR B0823+26 Open
PSR B0823+26, a 0.53-s radio pulsar, displays a host of emission phenomena over time-scales of seconds to (at least) hours, including nulling, subpulse drifting, and mode-changing. Studying pulsars like PSR B0823+26 provides further insigh…
View article: Monte-carlo simulation of the effective lunar aperture for detection of ultra-high energy neutrinos with LOFAR
Monte-carlo simulation of the effective lunar aperture for detection of ultra-high energy neutrinos with LOFAR Open
View article: Reconstructing air shower parameters with MGMR3D
Reconstructing air shower parameters with MGMR3D Open
Contains fulltext : 297891.pdf (Publisher’s version ) (Open Access)
View article: A high-precision interpolation method for pulsed radio signals from cosmic-ray air showers
A high-precision interpolation method for pulsed radio signals from cosmic-ray air showers Open
Analysis of radio signals from cosmic-ray induced air showers has been shown to be a reliable method to extract shower parameters such as primary energy and depth of shower maximum. The required detailed air shower simulations take 1 to 3 …
View article: Using pulse-shape information for reconstructing cosmic-ray air showers and validating antenna responses with LOFAR and SKA
Using pulse-shape information for reconstructing cosmic-ray air showers and validating antenna responses with LOFAR and SKA Open
The Low Frequency Array (LOFAR) is capable of measuring extensive air showers through their radio emission in the frequency range of 30–80 MHz, while the Square Kilometer Array (SKA) will be able to expand this range to 50–350 MHz. A very …
View article: High-resolution air shower observations with the Square Kilometer Array
High-resolution air shower observations with the Square Kilometer Array Open
The low-frequency part of the Square Kilometer Array will have an extremely high antenna density of roughly 60.000 antennas within one square kilometer, offering exciting new possibilities for high-resolution studies of air showers. Observ…
View article: Simulations of radio detection of cosmic rays with SKA-Low
Simulations of radio detection of cosmic rays with SKA-Low Open
Contains fulltext : 295239.pdf (Publisher’s version ) (Open Access)
View article: Measuring cosmic rays with the LOFAR radio telescope
Measuring cosmic rays with the LOFAR radio telescope Open
The LOFAR radio telescope has been used to measure radio emission from cosmic-ray air showers in the $10^{16}-10^{18}$ eV range for over a decade. LOFAR’s uniquely dense array of hundreds of antennas measuring from 30-80 MHz is ideal for p…
View article: A higher-order interpolation method for simulated radio signals of air showers
A higher-order interpolation method for simulated radio signals of air showers Open
\n Contains fulltext :\n 295232.pdf (Publisher’s version ) (Open Access)\n
View article: Prospects for measuring the longitudinal particle distribution of cosmic-ray air showers with SKA
Prospects for measuring the longitudinal particle distribution of cosmic-ray air showers with SKA Open
We explore the possibilities of measuring the longitudinal profile of individual air showers beyond Xmax when using very dense radio arrays such as SKA. The low-frequency part of the Square Kilometre Array, to be built in Austra…
View article: The NuMoon experiment: Preliminary results and upper limits on UHE particles
The NuMoon experiment: Preliminary results and upper limits on UHE particles Open
The main goal of the NuMoon experiment is study ultra-high energy cosmic rays and neutrinos interacting with the Moon using ground-based radio telescopes. Ultra-high energy (UHE) particles interacting with the Moon produce particle showers…
View article: A high-precision interpolation method for pulsed radio signals from cosmic-ray air showers
A high-precision interpolation method for pulsed radio signals from cosmic-ray air showers Open
Analysis of radio signals from cosmic-ray induced air showers has been shown to be a reliable method to extract shower parameters such as primary energy and depth of shower maximum. The required detailed air shower simulations take 1 to 3 …
View article: Reconstructing air shower parameters with MGMR3D
Reconstructing air shower parameters with MGMR3D Open
Measuring the radio emission from cosmic-ray particle cascades has proven to be a very efficient method to determine their properties such as the mass composition. Efficient modeling of the radio emission from air showers is crucial in ord…
View article: The Relationship of Lightning Radio Pulse Amplitudes and Source Altitudes as Observed by LOFAR
The Relationship of Lightning Radio Pulse Amplitudes and Source Altitudes as Observed by LOFAR Open
When a lightning flash is propagating in the atmosphere it is known that especially the negative leaders emit a large number of very high frequency (VHF) radio pulses. It is thought that this is due to streamer activity at the tip of the g…
View article: The relationship of lightning radio pulse amplitudes and source altitudes as observed by LOFAR
The relationship of lightning radio pulse amplitudes and source altitudes as observed by LOFAR Open
When a lightning flash is propagating in the atmosphere it is known that especially the negative leaders emit a large number of Very High Frequency (VHF) radio pulses. It is thought that this is due to streamer activity at the tip of the g…
View article: Sub-arcsecond imaging with the International LOFAR Telescope I. Foundational calibration strategy and pipeline
Sub-arcsecond imaging with the International LOFAR Telescope I. Foundational calibration strategy and pipeline Open
[abridged] The International LOFAR Telescope is an interferometer with stations spread across Europe. With baselines of up to ~2,000 km, LOFAR has the unique capability of achieving sub-arcsecond resolution at frequencies below 200 MHz, al…
View article: Sub-arcsecond imaging with the International LOFAR Telescope: II. Completion of the LOFAR Long-Baseline Calibrator Survey
Sub-arcsecond imaging with the International LOFAR Telescope: II. Completion of the LOFAR Long-Baseline Calibrator Survey Open
The Low-Frequency Array (LOFAR) Long-Baseline Calibrator Survey (LBCS) was conducted between 2014 and 2019 in order to obtain a set of suitable calibrators for the LOFAR array. In this paper we present the complete survey, building on the …
View article: A distinct negative leader propagation mode
A distinct negative leader propagation mode Open
View article: Processed Data for "The relationship of lightning radio pulse amplitudes and source altitudes as observed by LOFAR"
Processed Data for "The relationship of lightning radio pulse amplitudes and source altitudes as observed by LOFAR" Open
This set contains text data from the paper "The relationship of lightning radio pulse amplitudes and source altitudes as observed by LOFAR". Particularly for figures 2, 3, and 4.