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180 results on '"O. Scholten"'

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1. Monte-carlo simulation of the effective lunar aperture for detection of ultra-high energy neutrinos with LOFAR

2. Searching for intra-cloud positive leaders in VHF

3. In situ, broadband measurement of the radio frequency attenuation length at Summit Station, Greenland

4. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory

5. A Strong Pulsing Nature of Negative Intracloud Dart Leaders Accompanied by Regular Trains of Microsecond‐Scale Pulses

6. Small‐Scale Discharges Observed Near the Top of a Thunderstorm

7. Reconstructing the neutrino energy for in-ice radio detectors

8. The energy spectrum of cosmic rays beyond the turn-down around $$\varvec{10^{17}}$$ 10 17 eV as measured with the surface detector of the Pierre Auger Observatory

9. A distinct negative leader propagation mode

10. Direct measurement of the muonic content of extensive air showers between $$\mathbf { 2\times 10^{17}}$$ 2×1017 and $$\mathbf {2\times 10^{18}}~$$ 2×1018 eV at the Pierre Auger Observatory

11. Search for Ultra-high-energy Photons from Gravitational Wave Sources with the Pierre Auger Observatory

12. A Catalog of the Highest-energy Cosmic Rays Recorded during Phase I of Operation of the Pierre Auger Observatory

13. Timing Calibration and Windowing Technique Comparison for Lightning Mapping Arrays

14. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory

15. Multi-Messenger Physics With the Pierre Auger Observatory

16. Evidence for a mixed mass composition at the ‘ankle’ in the cosmic-ray spectrum

17. Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

18. Triboelectric backgrounds to radio-based polar ultra-high energy neutrino (UHEN) experiments

20. Determining Atmospheric Electric Fields using MGMR3D

21. Interferometric imaging of intensely radiating negative leaders

22. Erratum: Design and sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)

24. The energy spectrum of cosmic rays beyond the turn-down around 1017 eV as measured with the surface detector of the Pierre Auger Observatory

25. Multi-Messenger Physics With the Pierre Auger Observatory

26. The nature and origin of ultra high-energy cosmic rays

27. Use of Interference Tests to Constrain the Spacing of Hydraulically Fractured Wells in Neuquen Shale Oil Reservoirs

28. A search for point sources of EeV neutrons

29. Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory

30. Corrigendum: A large light-mass component of cosmic rays at 10

31. A Model for Evaluating Risk Reporting

32. Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

33. Measurement of the proton-air cross-section at sqrt(s) = 57 TeV with the Pierre Auger Observatory

34. Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory

35. Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

36. Anisotropy and chemical compositionof ultra-high energy cosmic rays usingarrival directions measured by thePierre Auger Observatory

37. The Lateral Trigger Probability function for UHE Cosmic Rays Showers detected by the Pierre Auger Observatory

38. Measurement of the Depth of Maximum of Extensive Air Showers above 10(18) eV

39. A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

40. The Northen Site of the Pierre Auger Observatory

41. Correlations and Clustering Phenomena in Subatomic Physics

42. Perspectives in the Structure of Hadronic Systems

43. Particle Production Spanning MeV and TeV Energies

44. Corrigendum: A large light-mass component of cosmic rays at 1017–1017.5 electronvolts from radio observations

45. Old ties from a new(s) perspective: diversity in the Dutch press coverage of the 2006 general election campaign

46. Improved flux limits for neutrinos with energies above 10(22) eV from observations with the Westerbork Synthesis Radio Telescope

47. Physics Performance Report for: PANDA. Strong Interaction Studies with Antiprotons

48. Developing functional seafood products

49. Politieke kennis en effecten van nieuws

50. High-energy-resolution inelastic electron and proton scattering and the multiphonon nature of mixed-symmetry 2+ states in 94Mo

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