ICALEPCS2011 - List of Authors (Plouviez, E.)

Paper

Title

Page

Fast Orbit Correction for the ESRF Storage Ring

177

J.M. Koch, F. Epaud, E. Plouviez, K.B. Scheidt
ESRF, Grenoble, France

Up to now, at the ESRF, the correction of the orbit position has been performed with two independent systems: one dealing with the slow movements and one correcting the motion in a range of up to 200Hz but with a limited number of fast BPMs and steerers. These latter will be removed and one unique system will cover the frequency range from DC to 200Hz using all the 224 BPMs and the 96 steerers. Indeed, thanks to the procurement of Libera Brilliance units and the installation of new AC power supplies, it is now possible to access all the Beam positions at a frequency of 10 kHz and to drive a small current in the steerers in a 200Hz bandwidth. The first tests of the correction of the beam position have been performed and will be presented. The data processing will be presented as well with a particular emphasis on the development inside the FPGA.

MOPKS014

Architecture and Control of the Fast Orbit Correction for the ESRF Storage Ring

189

F. Epaud, J.M. Koch, E. Plouviez
ESRF, Grenoble, France

Two years ago, the electronics of all the 224 Beam Position Monitors (BPM) of the ESRF Storage Ring were replaced by the commercial Libera Brilliance units to drastically improve the speed and position resolution of the Orbit measurement. Also, at the start of this year, all the 96 power supplies that drive the Orbit steerers have been replaced by new units that now cover a full DC-AC range up to 200Hz. We are now working on the replacement of the previous Fast Orbit Correction system. This new architecture will also use the 224 Libera Brilliance units and in particular the 10 KHz optical links handled by the Diamond Communication Controller (DCC) which has now been integrated within the Libera FPGA as a standard option. The 224 Liberas are connected together with the optical links to form a redundant network where the data are broadcast and are received by all nodes within 40 μS. The 4 corrections stations will be based on FPGA cards (2 per station) also connected to the FOFB network as additional nodes and using the same DCC firmware on one side and are connected to the steerers power supplies using RS485 electronics standard on the other side. Finally two extra nodes have been added to collect data for diagnostics and to give BPMs positions to the beamlines at high rate. This paper will present the network architecture and the control software to operate this new equipment.

Poster MOPKS014 [3.242 MB]

Paper	Title	Page
MOPKS010	Fast Orbit Correction for the ESRF Storage Ring	177
	J.M. Koch, F. Epaud, E. Plouviez, K.B. Scheidt ESRF, Grenoble, France
	Up to now, at the ESRF, the correction of the orbit position has been performed with two independent systems: one dealing with the slow movements and one correcting the motion in a range of up to 200Hz but with a limited number of fast BPMs and steerers. These latter will be removed and one unique system will cover the frequency range from DC to 200Hz using all the 224 BPMs and the 96 steerers. Indeed, thanks to the procurement of Libera Brilliance units and the installation of new AC power supplies, it is now possible to access all the Beam positions at a frequency of 10 kHz and to drive a small current in the steerers in a 200Hz bandwidth. The first tests of the correction of the beam position have been performed and will be presented. The data processing will be presented as well with a particular emphasis on the development inside the FPGA.

MOPKS014	Architecture and Control of the Fast Orbit Correction for the ESRF Storage Ring	189
	F. Epaud, J.M. Koch, E. Plouviez ESRF, Grenoble, France
	Two years ago, the electronics of all the 224 Beam Position Monitors (BPM) of the ESRF Storage Ring were replaced by the commercial Libera Brilliance units to drastically improve the speed and position resolution of the Orbit measurement. Also, at the start of this year, all the 96 power supplies that drive the Orbit steerers have been replaced by new units that now cover a full DC-AC range up to 200Hz. We are now working on the replacement of the previous Fast Orbit Correction system. This new architecture will also use the 224 Libera Brilliance units and in particular the 10 KHz optical links handled by the Diamond Communication Controller (DCC) which has now been integrated within the Libera FPGA as a standard option. The 224 Liberas are connected together with the optical links to form a redundant network where the data are broadcast and are received by all nodes within 40 μS. The 4 corrections stations will be based on FPGA cards (2 per station) also connected to the FOFB network as additional nodes and using the same DCC firmware on one side and are connected to the steerers power supplies using RS485 electronics standard on the other side. Finally two extra nodes have been added to collect data for diagnostics and to give BPMs positions to the beamlines at high rate. This paper will present the network architecture and the control software to operate this new equipment.
	Poster MOPKS014 [3.242 MB]