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LCLS Conceptual Design Report - Stanford Synchrotron Radiation ...

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L C L S C O N C E P T U A L D E S I G N R E P O R T<br />

To estimate the wake, realistic parameters of roughness, i.e. h0 = 0.28 µm (corresponding to<br />

the rms roughness of 0.2 µm), g = 2π/κ = 100 µm, and b = 2.5 mm, are used. This gives a value<br />

of r ≡ h0 3<br />

bκ/2<br />

= 0.11. The corresponding loss-factor parameter is<br />

−6<br />

U ≈4.5⋅ 10 , (8.56)<br />

which indicates that the effect of the wake in this regime will be negligibly small.<br />

Figure 8.34 Synchronous mode dispersion relation.<br />

It is important to emphasize here that the wakefield generated by the roughness is very<br />

sensitive to the geometry of the surface profile. The models which do not take into account the<br />

large aspect ratio of the real roughness — the ratio of the characteristic size along the surface<br />

(correlation length) and the typical height of the bumps — tend to overestimate the impedance<br />

and lead to very tight tolerances for the surface smoothness. The latest models that include the<br />

large aspect ratio into consideration predict much smaller impedance which is below the tolerable<br />

level for the <strong>LCLS</strong> undulator, if the typical height ~ 100 nm and g ~ 100 µm. The surface<br />

measurements [25] show that roughness with such characteristics can be achieved in a pipe with a<br />

good surface finish.<br />

8.10 Ion Effects<br />

In this section the number of ions generated during a bunch passage in the 121 m long<br />

undulator line of the <strong>LCLS</strong> x-ray FEL is calculated, emittance dilution caused by these ions is<br />

discussed, and the acceptable vacuum pressure is estimated.<br />

8.10.1 Introduction<br />

This section investigates ion production by the beam and by the synchrotron-radiation<br />

photons during a bunch passage in the <strong>LCLS</strong> undulator [38], and three different mechanisms of<br />

emittance dilution induced by these ions. The acceptable vacuum pressure for FEL operation is<br />

estimated from the calculated emittance growth.<br />

8-62 ♦ U N D U L A T O R

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