Data Rates

From DUNE
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...")
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigation Jump to search

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.