Difference between revisions of "General Meeting Agenda 3/7/19"
Jump to navigation
Jump to search
| (2 intermediate revisions by the same user not shown) | |||
| Line 6: | Line 6: | ||
::* [https://wiki.jlab.org/cuawiki/images/e/e3/IMG_2275.jpg Magnet photo 3] | ::* [https://wiki.jlab.org/cuawiki/images/e/e3/IMG_2275.jpg Magnet photo 3] | ||
::* [https://wiki.jlab.org/cuawiki/images/2/2b/IMG_2276.jpg Magnet photo 4] | ::* [https://wiki.jlab.org/cuawiki/images/2/2b/IMG_2276.jpg Magnet photo 4] | ||
| + | ::* Questions: | ||
| + | :::*Do we care about Sweep-magnet polarity (do we need to switch during experiments)? | ||
| + | ::::* DVCS maybe: Helicity correlated sin(phi) (up-down) is critical observable | ||
| + | :::* Is Sweep-Magnet power supply remotely reversible? | ||
| + | |||
* HV bases and amplifiers | * HV bases and amplifiers | ||
Latest revision as of 09:22, 7 March 2019
Discussion topics:
- Magnet Assembly and testing
- Magnet photo 1
- Magnet photo 2
- Magnet photo 3
- Magnet photo 4
- Questions:
- Do we care about Sweep-magnet polarity (do we need to switch during experiments)?
- DVCS maybe: Helicity correlated sin(phi) (up-down) is critical observable
- Is Sweep-Magnet power supply remotely reversible?
- HV bases and amplifiers
- Frame and simulations
- Crystals and prototype
- NPS ERR preparations
- Other