Physics307L:People/Josey/Rough Draft: Difference between revisions
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== | ==<center>Measuring and Predicting Background Radiation Using Poisson Statistics</center>== | ||
<center>''Author: Brian P. Josey'' | |||
''Experimentalists: Brian P Josey and Kirstin G G Harriger'' | |||
''Junior Lab, Department of Physics & Astronomy, University of New Mexico'' | |||
''Albuquerque, NM 87131'' | |||
''bjosey@unm.edu''</center> | |||
==Abstract== | |||
==Introduction== | |||
==Methods and Materials== | |||
For this experiment, a combined scintillator=photomultiplier tube (PMT) was used to collect data. To do this, every time the scintillator detected radiation, it would fire a beam of ultraviolet light to the PMT. The PMT would then convert this light signal into a single voltage. This voltage would be carried to an internal MCS card in a computer, where it would be analyzed by a UCS 30 software. This software counts each signal voltage and create a set of data containing the size of the window over which the data was collected, the time and the number of radiation events to occur in that window. In order for the scintillator to detect the radiation, it had to have a potential gradient that would pick up ions created in the radiation event. This potential was supplied by a Spectech Universal Computer Spectrometer power supply, and set to 1200 V throughout the course of the experiment. | |||
The collection of the data was carried out by using the UCS 30 software. It would create a consecutive series of windows of set interval of time, and count the number of signal currents, which represent the number of radiation events, that occurred within each window. This data was then saved into data file that could be manipulated and processed using MATLAB v. 2009a. To demonstrate the Poisson distribution, the scintillator-PMT, power supply, and computer were all turned on. The UCS 30 software was then uploaded, and the window size was set to various lengths of time. Data was collected over a series of sets of windows, the window sizes were set at 10, 20, 40, 80, 100, 200, 400 and then 800 ms. Each run contained 2046 windows of the given size. The data was then analyzed, see results and discussion below, to demonstrate that background radiation did follow a Poisson distribution. This data was then used to predict the behavior of a similar set of data that occurred for a 1 second window size. After predicting its behavior, the system was ran again, using a 2046 windows of 1 second length. This data was then compared to the predicted results form the initial data. | |||
==Results== | |||
==Discussion== | |||
==Conclusions== | |||
==Acknowledgments== | |||
==References== | |||
Revision as of 10:14, 13 November 2010
Measuring and Predicting Background Radiation Using Poisson Statistics
Experimentalists: Brian P Josey and Kirstin G G Harriger
Junior Lab, Department of Physics & Astronomy, University of New Mexico
Albuquerque, NM 87131
bjosey@unm.eduAbstract
Introduction
Methods and Materials
For this experiment, a combined scintillator=photomultiplier tube (PMT) was used to collect data. To do this, every time the scintillator detected radiation, it would fire a beam of ultraviolet light to the PMT. The PMT would then convert this light signal into a single voltage. This voltage would be carried to an internal MCS card in a computer, where it would be analyzed by a UCS 30 software. This software counts each signal voltage and create a set of data containing the size of the window over which the data was collected, the time and the number of radiation events to occur in that window. In order for the scintillator to detect the radiation, it had to have a potential gradient that would pick up ions created in the radiation event. This potential was supplied by a Spectech Universal Computer Spectrometer power supply, and set to 1200 V throughout the course of the experiment.
The collection of the data was carried out by using the UCS 30 software. It would create a consecutive series of windows of set interval of time, and count the number of signal currents, which represent the number of radiation events, that occurred within each window. This data was then saved into data file that could be manipulated and processed using MATLAB v. 2009a. To demonstrate the Poisson distribution, the scintillator-PMT, power supply, and computer were all turned on. The UCS 30 software was then uploaded, and the window size was set to various lengths of time. Data was collected over a series of sets of windows, the window sizes were set at 10, 20, 40, 80, 100, 200, 400 and then 800 ms. Each run contained 2046 windows of the given size. The data was then analyzed, see results and discussion below, to demonstrate that background radiation did follow a Poisson distribution. This data was then used to predict the behavior of a similar set of data that occurred for a 1 second window size. After predicting its behavior, the system was ran again, using a 2046 windows of 1 second length. This data was then compared to the predicted results form the initial data.
