View source for Electronics We Need to Collect

[[Image:50 nsec.jpg|left|125 px|Electron Pulse]]

It'll hit our target and neutrons will be collected.

B <sub>n <sup>o</sup> </sub> = .1

P <sub> n </sub> = 1.04 MeV/c

1/V = 10nsec/foot => Detector must be > 5 feet from target.

==Discriminating Signals==
[[Image:what we'd like to see with d20.jpg|left|350 px|What we'd like to see with D20]]  [[Image:what we'd like to see with h20.jpg|right|350 px|What we'd like to see with H20 and our empty target]]





















==What We Need==

* n <sup>o</sup> detectors
* High voltage
* Splitters
* Discriminators
* Scalers
* NIM bin
* FAN
* Oscilloscope
* Delay
* Cables

==What Else Needs to be Done?==

* Round up electronics
* Set up electrons
* NIM bin
* Mounting system
* Polarization
* Find as many scalers as possible.
* Check Dr. Dale's calculations
** Given the collimator's 17" -> can the electron which makes a neutron get through the collimator?
* Will it burn a hole through the collimator?
** 1 KH
** 50 nsec pulse width
** 80 MA peak current
** 1 mm beam size
** No Conduction
** Radiated cooling


-These are the notes from the July 15th, 2008 meeting.

[http://wiki.iac.isu.edu/index.php/PhotoFission_with_Polarized_Photons_from_HRRL Go Back]