no code implementations • 10 Mar 2021 • M. Mikhailova, E. Bondarev, A. Nozdrina, H. Landsman, D. Z. Besson
We find that such backgrounds are evident in the several neutrino experiments considered, and are generally characterized by: a) a threshold wind velocity which likely depends on the experimental signal trigger threshold and layout; for the experiments considered herein, this value is typically O(10 m/s), b) frequency spectra generally shifted to the low-end of the frequency regime to which current radio experiments are typically sensitive (100-200 MHz), c) for the strongest background signals, an apparent preference for discharges from above-surface structures, although the presence of more isotropic, lower amplitude triboelectric discharges cannot be excluded.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
