Difference between revisions of "Cosmic Data Analysis"
From Hall A Wiki
(New page: ==Motivation for cosmic ray analysis== Cosmic rays provide a good proxy for high energy charged particles that will be found in Hall A during the time of experimentation. The robust nature...) |
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Cosmic rays provide a good proxy for high energy charged particles that will be found in Hall A during the time of experimentation. The robust nature of cosmic rays allow for vertical track testing at any point of the day/year, which makes them ideal for continuous testing/debugging methodology used in CDet. | Cosmic rays provide a good proxy for high energy charged particles that will be found in Hall A during the time of experimentation. The robust nature of cosmic rays allow for vertical track testing at any point of the day/year, which makes them ideal for continuous testing/debugging methodology used in CDet. | ||
| − | ==DAQ Computer | + | ==DAQ Computer Access== |
| + | The current computer setup for the DAQ is sbs2 which is located in the test lab, under the user adaq. | ||
| + | it is recommended when setting up coda, to do so at the test lab setup, as remote ssh connections can be terminated periodically from the jlab host server. | ||
| + | |||
==Hall A Analyzer == | ==Hall A Analyzer == | ||
Revision as of 13:22, 3 July 2017
Motivation for Cosmic Ray Analysis
Cosmic rays provide a good proxy for high energy charged particles that will be found in Hall A during the time of experimentation. The robust nature of cosmic rays allow for vertical track testing at any point of the day/year, which makes them ideal for continuous testing/debugging methodology used in CDet.
DAQ Computer Access
The current computer setup for the DAQ is sbs2 which is located in the test lab, under the user adaq. it is recommended when setting up coda, to do so at the test lab setup, as remote ssh connections can be terminated periodically from the jlab host server.
