Difference between revisions of "General Meeting Agenda 3/7/19"
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* Magnet Assembly and testing | * Magnet Assembly and testing | ||
+ | ::* [https://wiki.jlab.org/cuawiki/images/e/e9/IMG_2273.jpg Magnet photo 1] | ||
+ | ::* [https://wiki.jlab.org/cuawiki/images/5/5d/IMG_2274.jpg Magnet photo 2] | ||
+ | ::* [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] | ||
+ | ::* 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 | ||
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* NPS ERR preparations | * NPS ERR preparations | ||
+ | ::* [https://wiki.jlab.org/cuawiki/index.php/NPS_ERR NPS ERR] | ||
+ | ::* [https://wiki.jlab.org/cuawiki/index.php/NPS_Subsystems NPS subsystems] | ||
* Other | * Other |
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