Data Rates
Revision as of 22:23, 3 March 2015 by MaximPotekhin (talk | contribs) (Created page with "= Disclaimer = This page is in initial stages of construction. = Overview = According to the physics goals of the experiment, we need to consider the following main sources o...")
Disclaimer
This page is in initial stages of construction.
Overview
According to the physics goals of the experiment, we need to consider the following main sources of signal:
- The "beam neutrino" signal
- The Supernova Burst (SNB) signal
- Proton Decay
- Solar neutrinos
All these signals have distinct energy scales, topologies and other characteristics. In terms of buffering and processing data in real or near time, they pose different requirements.
