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Measuring the Electron Beam Energy in a Magnetic Bunch ... - DESY

Measuring the Electron Beam Energy in a Magnetic Bunch ... - DESY

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not possible to disentangle which energy change was caused by <strong>in</strong>com<strong>in</strong>g arrival-time<br />

jitter and which energy change was caused by accelerat<strong>in</strong>g gradient and phase jitter<br />

unless <strong>the</strong> arrival-time jitter generated upstream of <strong>the</strong> accelerator section has been<br />

measured.<br />

There are two different strategies to deal with this problem. One could use an<br />

accelerator section upstream of each chicane <strong>in</strong> order to stabilize <strong>the</strong> arrival-time after<br />

each chicane, regardless of how much <strong>the</strong> beam energy jitter is <strong>in</strong>creased. One would<br />

<strong>the</strong>n need to stabilize <strong>the</strong> beam energy us<strong>in</strong>g an accelerator section located after <strong>the</strong><br />

chicanes. Alternatively, one could use a s<strong>in</strong>gle accelerator section gradient setpo<strong>in</strong>t to<br />

simultaneously stabilize <strong>the</strong> beam energy and arrival-time after each chicane. The endresult<br />

of both schemes would, <strong>in</strong> pr<strong>in</strong>ciple, be <strong>the</strong> same.<br />

For <strong>the</strong> sake of mach<strong>in</strong>e stability, <strong>the</strong> author believes that <strong>the</strong> latter option is<br />

better: a feedback on <strong>the</strong> first accelerator section should not respond to changes <strong>in</strong> <strong>the</strong><br />

<strong>in</strong>jector jitter and a feedback on <strong>the</strong> second accelerator section should not respond to<br />

changes <strong>in</strong> <strong>the</strong> first accelerator section. To simultaneously stabilize beam energy and<br />

arrival-time after a bunch compressor, one could execute a comb<strong>in</strong>ation of <strong>the</strong> follow<strong>in</strong>g:<br />

• use measurements of <strong>the</strong> arrival-time jitter upstream of a bunch compressor to<br />

keep <strong>the</strong> energy/arrival-time feedback from respond<strong>in</strong>g to <strong>the</strong> energy/arrival-time<br />

jitter that it creates.<br />

• stabilize <strong>the</strong> arrival-time jitter upstream of <strong>the</strong> bunch compressor before<br />

correct<strong>in</strong>g <strong>the</strong> energy/arrival-time jitter downstream.<br />

3.3 <strong>Beam</strong>-Based Feedback Strategy<br />

Two schematics of <strong>the</strong> synchronization sensitive components <strong>in</strong> <strong>the</strong> mach<strong>in</strong>e are<br />

shown <strong>in</strong> Fig. 3.3.1 [27]. An optimal feedback setup is depicted <strong>in</strong> Fig. 3.3.1(a.) and a<br />

more quickly realizable architecture is depicted <strong>in</strong> Fig. 3.3.1(b.). The <strong>in</strong>jector laser<br />

(Laser), <strong>the</strong> <strong>in</strong>jector RF (Gun), <strong>the</strong> super-conduct<strong>in</strong>g accelerator sections (ACC1-7) and<br />

<strong>the</strong> third-harmonic module (third-) are depicted <strong>in</strong> block diagram format with arrows<br />

connect<strong>in</strong>g various optical cross-correlators (OCC), chicane beam position monitors<br />

(EBPM), bunch length monitors (EO-1D, THz-1D), and beam arrival-time monitors<br />

(BAM) to <strong>the</strong> digital process<strong>in</strong>g boards (μTCA or SIMCON-DSP) with which <strong>the</strong>y<br />

would be connected <strong>in</strong> a beam-based feedback system that controls, on a bunch-to-bunch<br />

basis, <strong>the</strong> amplitude and phase (A, φ) of a normal-conduct<strong>in</strong>g RF cavity (3GHz NRF<br />

cavity), <strong>the</strong> 1.3 GHz super conduct<strong>in</strong>g acceleration cavities (1.3GHz SRF ACC1(2&3))<br />

and <strong>the</strong> super conduct<strong>in</strong>g third- harmonic l<strong>in</strong>earization cavity (3.9GHz SRF).<br />

The reason that <strong>the</strong> system shown <strong>in</strong> Fig 3.3.1(b.) will be built before that shown<br />

<strong>in</strong> Fig 3.3.1(a.) is that <strong>the</strong> μTCA crate system, shown <strong>in</strong> blue <strong>in</strong> <strong>the</strong> figures below, along<br />

with <strong>the</strong> correspond<strong>in</strong>g ADC and FPGA boards will not be available <strong>in</strong> 2010. VME is <strong>the</strong><br />

crate system that has been used at FLASH s<strong>in</strong>ce its <strong>in</strong>ception but will be phased out as<br />

μTCA crates become viable. In <strong>the</strong> currently available VME crate <strong>in</strong>frastructure, <strong>the</strong><br />

beam arrival-time is calculated on an <strong>in</strong>-house built Analog Carrier Board (labeled ACB<br />

<strong>in</strong> <strong>the</strong> figure) that conta<strong>in</strong>s ADCs, delay-chips and FPGAs. <strong>Beam</strong> arrival-time<br />

<strong>in</strong>formation from this board is delivered to <strong>the</strong> cavity controller via an optical Gigal<strong>in</strong>k.<br />

The cavity controllers reside on VME based SIMCON-DSP boards that each have ADCs,<br />

DSPs, DACs, and an FPGA.<br />

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