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Oliver - slides on tolerances; crossing angle, beta beating, Q' etc. tolerances tine/Q1 interplay, dynamic aperture
After snapback and the first 100 GeV we expect things to quieten down considerably. Clearly the power converters will be driving the the machine up. RF following. Orbit and possibly tune feedback operational. Real-time correction available to operator. Multipole factory feeding forward for as long as necessary.
P(t) - 6 parameters
RF
Dampers, voltage and frequency driven by function generators, triggered by timing events. Details see here
Controlled longitudinal emittance blow-up at some pre-defined point in the ramp + monitoring thereof
Lattice Octupoles
For increased Landau damping - bring the octupoles up at some point in the ramp
Collimators
Left out during the ramp. Move to 7 sigma (or perhaps more) at the end of the ramp before starting the squeeze.
Orbit feedback
Discussed in detail elsewhere
Both global and local running. Lock angle and position in IRs to maintain beam separation at greater than 8 sigma throughout the ramp. Will have to be monitored all the way up the ramp.
At around 5 TeV (according to Stephane) the crossing scheme changes, he implied that a stop might be required.
Compensation bumps
Will be ramped
Electron cloud
Vacuum pressure and cryogenics heat load will need to be monitored. Scrubbing might be necessary at intermediate energies. Stop, move beam, monitor vacuum and heat load. Instabilities induced by electron cloud not expected to be a problem.