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High Brightness Electron Beam Diagnostics and their ... - CASA

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Withr1=r+c(==cwhereisthemirrorsrelativeposition),r2=r,Eqn.(5.42)takesthe Itisimportanttonotethatthequantity,intheaboveequation,isoftheorderofthebunch form: image<strong>and</strong>thexedmirror,oftheorderof1m;hencereplacingr+cinEqn.(5.43)withrisa 5104eect.Therefore,withoutintroducingsignicanterrortheintensityonthedetectorcan planewithrespectofthepointofemissionwillresultinavalueofr,thedistancebetweenTR length(i.e.atmaximum500mforthepresentcase).A10%errorinthelocationofthefocal I()/1 r+c(0)()+cr((0)()) (5.43)<br />

abovecanbeusedtoextractinformationfromatransitionradiationinterferogram. 5.5.3RelatinganInterferogramMeasurementtoaBunchLengthMeasurement Bymeasuringthefull-widthhalf-maximum(FWHM)oftheautocorrelation,onecanveryeasily bewrittenasforaTEMwave,thatisI()/((0)());<strong>and</strong>thest<strong>and</strong>ardanalysispresented<br />

getanestimateofthebunchlength.Let'sanalyzehowtheFWHMisrelatedtotheRMSvalues oftwotypicalparticledistributions:anormaldistributionthatischaracterizedbyitsrmsvalue<br />

Table5.1:Relationshipsbetween\equivalent","RMS"<strong>and</strong>"FWHM"lengthsforagaussian<strong>and</strong> relatesFWHM,RMS<strong>and</strong>equivalentlengthforthesedistributions. (variance)z<strong>and</strong>asquaredistributionwhosecharacteristiclengthisitsfullwidthw.Table5.1<br />

squarelongitudinalbunchdensity. DistributionEqu.LengthRMSFWHM Gaussian Square p2z w w=p12 z2zpln(2) w<br />

CaseofaGaussi<strong>and</strong>istribution:<br />

CaseofaSquaredistribution: HencetheRMSvalueoftheconvolutionisp2timestheRMSvalueofthedistribution.Using Table5.1,wededucethat S(z)=1=p22zexp(z2=(2z)).Forsuchdistribution,theautocorrelationis()=1=(2pz)exp(2=(42z)).<br />

Wewritethisdistributionas:S(z)=((1=w)ifw=2

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