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Report on future detector requirements at ESRF

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Linearity:<br />

For the same reas<strong>on</strong>, linearity <strong>on</strong> an extended range of intensities has to be reached <strong>on</strong> both<br />

main <strong>detector</strong> and incident flux <strong>detector</strong>.<br />

Flux <strong>on</strong> <strong>detector</strong>:<br />

In order to optimise the use of the <strong>detector</strong> characteristics (linearity and signal to noise r<strong>at</strong>io),<br />

the flux is adjusted so th<strong>at</strong> the measured currents range from 0.1 pA and 1 µA. To give an<br />

equivalent in terms of phot<strong>on</strong>s <strong>on</strong> a Si diode, 0.1 pA corresp<strong>on</strong>ds to 3000 phot<strong>on</strong>s of 1 keV.<br />

Particular oper<strong>at</strong>ing c<strong>on</strong>diti<strong>on</strong>s:<br />

The <strong>detector</strong>s will be oper<strong>at</strong>ed in ultra-high vacuum, near high magnetic fields up to 6 T.<br />

Existing <strong>detector</strong>s<br />

ID12 is using Si pnn + photodiodes oper<strong>at</strong>ed in the photovoltaic mode and optimised for the<br />

beamline by Eurisys-Mesures [Goul<strong>on</strong> et al., 2005]. The dark current <strong>on</strong> both I and I0 is<br />

measured altern<strong>at</strong>ively with the fluorescence signal using a chopper <strong>at</strong> a typical frequency of<br />

67 Hz.<br />

Short term possibilities<br />

A p<strong>at</strong>ent (FR08/55566, Goul<strong>on</strong> et al.) has been registered c<strong>on</strong>cerning a <strong>detector</strong> for the<br />

measurement of ferromagnetic res<strong>on</strong>ances <strong>at</strong> GHz frequencies.<br />

Main required improvements<br />

The main expected improvement c<strong>on</strong>cerns the detecti<strong>on</strong> of signals of very low intensity <strong>at</strong><br />

high frequencies.<br />

Other types of <strong>detector</strong>s<br />

Circular Polariz<strong>at</strong>i<strong>on</strong> Beamline also uses an energy dispersive <strong>detector</strong> (see page 94).<br />

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