Difference between revisions of "2012 NSF Proposal"
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[[File:09142012_C_slide3.pdf]] | [[File:09142012_C_slide3.pdf]] | ||
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| + | ==Budget Justification Table== | ||
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| + | {| border="1" |cellpadding="20" cellspacing="0 | ||
| + | |- | ||
| + | | 3 year Costs|| Description | ||
| + | |- | ||
| + | |500 || Ar/Co2 detector gases, LN2 coolant for target tests | ||
| + | |- | ||
| + | | 4500 || VME based module | ||
| + | |- | ||
| + | | 5000 || NIM bin electronics | ||
| + | |- | ||
| + | | 15000 || PMTs and bases | ||
| + | |- | ||
| + | | 9000 || raw construction materials for R & D tests | ||
| + | |- | ||
| + | | 6000 || | ||
| + | |- | ||
| + | |20000 || | ||
| + | |} | ||
Revision as of 20:45, 23 October 2012
The competition
000416256
JeV
| Institution | 2 year Budget | Physics |
| ASU | 340 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969201 |
| Rutgers | 800 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969239 |
| CS LA | 264 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969380 |
| Catholic | 328 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969434 |
| Catholic | 311 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=1019521 |
| Ohio U | 484 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969297 |
| Hampton | 509 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=1002644 |
| RPI | 520 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0965606 |
| Kent State | 465 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969129 |
| Ohio Univ | 327 | http://www.nsf.gov/awardsearch/showAward.do?AwardNumber=0969788 |
Physics topics
Introduction
In order to fully understand nature's strong force, Nuclear physics has sought to describe physics systems ranging in size from a sun to the constituents of a nucleon. We propose to perform measurements using electromagnetic probes at Jefferson Lab that will
CLAS Polarized Structure Function
Projects Table
| Project | Personnel | Status | pgs |
| Polarization | Forest | Approved | 2 |
| N* | Cole | Approved | 3 |
| Khandaker , McNulty | Approved | 2 | |
| PV (nucleus size, weak mixing angle, astro physics) | McNulty | Cond. Approved | 3 |
Budget Justification Table
| 3 year Costs | Description |
| 500 | Ar/Co2 detector gases, LN2 coolant for target tests |
| 4500 | VME based module |
| 5000 | NIM bin electronics |
| 15000 | PMTs and bases |
| 9000 | raw construction materials for R & D tests |
| 6000 | |
| 20000 |
Stuff
5 students
Section on training our JLab students in Hardware
Student do physics at JLab and gain experience with hardware using ISU facilities.
CLAS can also be categorized as a bunch of "One off" experiments. Perhaps review publication record of the experiments. PV experiments take 10 years from construction to publication some CLAS experiments took less.