Abstract. We use a GEANT based Monte Carlo simulation to investigate the properties of electron induced electromag-netic showers in ice. Various shower parameters such as crit-ical energy, Moliere radius, and track lengths are studied. We look at the dependence of these quantities on the energy of the primary electron as well as the Monte Carlo threshold energy. We also study in detail the Cerenkov radiation asso-ciated with the charge excess in the shower. The radiation is coherent at frequencies on the order of GHz and can readily be detected by experiments such as the RICE at the South Pole.
A sufficient density of free electrons and strong electric fields are the basic requirements to star...
We derive that lightning can start if the electric field is 15% of the breakdown field, and if elong...
Multi-detector observations of individual air showers are critical to make significant progress to p...
Abstract. We use a GEANT based Monte Carlo simulation to investigate the properties of electron indu...
We present a semianalytical method for the calculation of coherent Askaryan radiation in showers ind...
High energy particle showers produce coherent Cherenkov radio emission in dense, radio-transparent m...
Radio Cherenkov radiation is arguably the most efficient mechanism for detecting showers from ultra-...
PeV neutrinos produce particle showers when they interact with the atomic nuclei in ice. We briefly ...
In this article we try to answer the question whether the radar detection technique can be used for ...
Recently the radar scattering technique to probe neutrino induced particle cascades above PeV energi...
We discuss the radar detection method as a probe for high-energy neutrino induced particle cascades ...
We study the Cherenkov radiopulses emitted in PeV and EeV neutrino interactions in ice. We discuss h...
A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interac...
Ionization showers are created in the Earths atmosphere by cosmic particles or by run-away electrons...
Emission of electromagnetic waves from high energy particle showers is a powerful tool that can be u...
A sufficient density of free electrons and strong electric fields are the basic requirements to star...
We derive that lightning can start if the electric field is 15% of the breakdown field, and if elong...
Multi-detector observations of individual air showers are critical to make significant progress to p...
Abstract. We use a GEANT based Monte Carlo simulation to investigate the properties of electron indu...
We present a semianalytical method for the calculation of coherent Askaryan radiation in showers ind...
High energy particle showers produce coherent Cherenkov radio emission in dense, radio-transparent m...
Radio Cherenkov radiation is arguably the most efficient mechanism for detecting showers from ultra-...
PeV neutrinos produce particle showers when they interact with the atomic nuclei in ice. We briefly ...
In this article we try to answer the question whether the radar detection technique can be used for ...
Recently the radar scattering technique to probe neutrino induced particle cascades above PeV energi...
We discuss the radar detection method as a probe for high-energy neutrino induced particle cascades ...
We study the Cherenkov radiopulses emitted in PeV and EeV neutrino interactions in ice. We discuss h...
A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interac...
Ionization showers are created in the Earths atmosphere by cosmic particles or by run-away electrons...
Emission of electromagnetic waves from high energy particle showers is a powerful tool that can be u...
A sufficient density of free electrons and strong electric fields are the basic requirements to star...
We derive that lightning can start if the electric field is 15% of the breakdown field, and if elong...
Multi-detector observations of individual air showers are critical to make significant progress to p...