Difference between revisions of "Data Rates"
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(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...") |
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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. | 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. | ||
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| + | = Beam Neutrinos = | ||
| + | Because of the energy scale (~GeV range) neutrino interactions will be characterized by TPC signals well above radiological background. Zero-suppression will lead to significant reduction of data volume and rates (the detector will appear "empty" for the most part). | ||
| + | |||
| + | = SNB = | ||
Revision as of 22:33, 3 March 2015
Contents
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.
Beam Neutrinos
Because of the energy scale (~GeV range) neutrino interactions will be characterized by TPC signals well above radiological background. Zero-suppression will lead to significant reduction of data volume and rates (the detector will appear "empty" for the most part).
