Preliminary Agenda
| 8:00-9:00 | Registration | ||
| 9:00-10:40 | Introduction, History and Theory | Chair: R. Nahnhauer | |
| 5' | R. Nahnhauer | Welcome | |
| 20' | I. Zheleznykh | Early years of high energy ν-astronomy and development of alternative concepts of ν-detection | |
| 40' | A. Ringwald | EHE cosmic ν's and their impact on particle physics and cosmology | |
| 20' | D. Seckel | Comparison of GZK neutrino flux calculations | |
| 15' | J. Becker | Investigation of the event rate for different detector arrays and various UHE models | |
| 10:40-11:00 | Coffee Break and Registration | ||
| 11:00-12:55 | Target Material Properties | Chair: A.M. van den Berg | |
| 25' | M. Chiba | Measurement of the attenuation length for radio waves in natural rock salt concerning UHE ν detection | |
| 25' | B. Price | Acoustic wave propagation in ice and salt | |
| 25' | J. Eisenblaetter, J. Manthei |
Experience on acoustic wave propagation in rock salt in the frequency range 1-100 kHz and conclusions with respect to the feasibility of a rock salt dome as neutrino detector | |
| 25' | D. Williams | Radio signals from photon beams in sand and salt | |
| 15' | P. Miocinovic | Time domain analysis of Askaryan pulses | |
| 12:55-14:00 | Lunch Break | ||
| 14:00-15:40 | Simulation and Propagation of Signals | Chair: A. Karle | |
| 20' | L.G. Dedenko | The hybrid scheme of simulation of eγ and eh cascades in a dense medium at UHE energies | |
| 20' | Y. Watanabe | Structure function of excess charge in rock salt | |
| 20' | J. Alvarez-Muniz | Coherent radio emission in different dense media | |
| 20' | T. Huege | Simulation of radio emission from cosmic air showers | |
| 20' | A. Konstantinov | Simulation of radio signals from 1-10 TeV air showers using EGSnrc | |
| 15:40-16:00 | Coffee Break | ||
| 16:00-17:40 | Signal Processing and Background Reduction | Chair: A. Rostovtsev | |
| 20' | D. Seckel | Radiosignal pulse shape | |
| 40' | S. Danaher | Acoustic signal processing (a tutorial) | |
| 20' | J. Vandenbroucke | Experience from SAUND | |
| 20' | D. Zaborov | Analysis methods of ITEP Baikal data | |
| 9:00-10:40 | Sensors and Transmitters | Chair: G. Anton | |
| 20' | C. Naumann | Design studies of piezo based receivers for acoustic particle detection in water | |
| 20' | K. Salomon | Measurements and simulation studies of piezoceramics for acoustic detection | |
| 25' | C. Trono | Fiber laser hydrophones as pressure sensors | |
| 15' | A. Capone, G. De Bonis |
Preliminary results on hydrophones calibration with proton beam | |
| 20' | S. Böser | Developement of glaciophones and acoustic transmitters for ice | |
| 10:40-11:00 | Coffee Break | ||
| 11:00-13:00 | Results I (Acoustic) | Chair: J. Learned | |
| 20' | N. Budnev, M. Pan'kov |
High Frequency Noise in the Lake Baikal as a Background for Acoustic Detection of High Energy Neutrinos | |
| 20' | V. Lyashuk | ITEP investigations of acoustic phenomena from high energy particles | |
| 20' | K. Graf | Testing acoustic signals with a proton and laser beams in water | |
| 20' | J. Vandenbroucke | Results from the SAUND I experiment | |
| 20' | G. Riccobene | The NEMO acoustic test facility | |
| 20' | M. Ardid | First Activities in Acoustic Detection of Particles in UPV | |
| 13:00-14:00 | Lunch Break | ||
| 14:00-15:40 | Results II (Cherenkov Radio) | Chair: D. Saltzberg | |
| 20' | R. Dagkesamanskii | The upper limit to the EHE neutrino flux from the observations of the Moon with the Kalyazin radio-telescope | |
| 20' | J. Bacelar | Using the Westerbork Radio Observatory to detect UHE ν interactions on the moon | |
| 20' | D. Besson | Status of the RICE experiment | |
| 25' | P. Miocinovic | Status of the ANITA experiment | |
| 15' | A. Connolly | Simulation issues for radio detection in ice | |
| 15:40-16:00 | Coffee Break | ||
| 16:00-17:40 | Results III (Air Shower Radio) | Chair: B. Price | |
| 30' | H. Falcke | Radio Detection of Cosmic Rays | |
| 25' | A. Horneffer | Detecting radio pulses from air showers with LOPES | |
| 20' | A. Haungs | LOPES data analysis | |
| 25' | R. Dallier | CODALEMA: a cosmic ray air showers radio detection experiment | |
| 19:30 | Workshop Dinner | ||
| 9:00-10:40 | Future Projects I | Chair: A. Capone | |
| 20' | Y. Karlik, V. Svet |
Converted hydroacoustic antenna MG-10M as basic module for a deep water ν-telescope | |
| 20' | S. Danaher | The UK-ACORNE group present projects and future plans | |
| 20' | J. Perkin | ACORNE simulation work | |
| 20' | T. Karg | Design considerations and sensitivity estimates for an acoustic neutrino detector | |
| 20' | N. Budnev, M. Pan'kov |
A Device for Detection of Acoustic Signals from Super High Energy Neutrinos | |
| 10:40-11:00 | Coffee Break | ||
| 11:00-13:00 | Future Projects II | Chair: H. Falcke | |
| 15' | N. Kurahashi | SAUND II | |
| 20' | R. Lahmann | The integration of acoustic detection into ANTARES | |
| 25' | S. Böser | SPATS - a South Pole Acoustic Test Setup | |
| 20' | V.A. Tsarev | Overview of the the Lunar Orbital Radio Detector experiment - LORD | |
| 15' | A. Chechin | The concept of the LORD instrument | |
| 25' | H. Gemmeke, O. Krömer |
Advanced detection methods of radio signals from cosmic rays for KASKADE Grande and AUGER | |
| 13:00-14:00 | Lunch Break | ||
| 14:00-15:40 | Future Projects III | Chair: D. Besson | |
| 25' | A.M. van den Berg | Neutrino detection in salt domes under LOFAR | |
| 25' | P. Miocinovic | Radio-Cherenkov measurements in salt - towards salt based neutrino detectors | |
| 25' | D. Saltzberg | The SalSA project | |
| 25' | J. Vandenbroucke | Capabilities of an optic-radio-acoustic detector array at the South Pole | |
| 15:40-16:00 | Coffee Break | ||
| 16:00-17:00 | round table discussion on collaboration and networking | Chair: U. Katz | |
| 17:00-17:40 | Closing session | Chair: I. Zheleznykh | |
| 40' | J. Learned | Conference summary | |
last update: 17.05.2005,