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Magnetic Measurements for a MICE Spectrometer Solenoid

Identifieur interne : 000654 ( Main/Curation ); précédent : 000653; suivant : 000655

Magnetic Measurements for a MICE Spectrometer Solenoid

Auteurs : M. Buehler [États-Unis] ; A. Bross [États-Unis] ; C. Hess [États-Unis] ; D. Orris [États-Unis] ; R. Pilipenko [États-Unis] ; R. Preece [Royaume-Uni] ; C. Sylvester [États-Unis] ; M. Tartaglia [États-Unis] ; J. Tompkins [États-Unis] ; S. Virostek [États-Unis]

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RBID : Pascal:13-0241093

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Abstract

The goal of the Muon Ionization Cooling Experiment (MICE) is to demonstrate muon cooling for a future muon collider. In order to quantify this cooling effect with high precision, scintillating fiber trackers in a uniform 4 Tesla field are required. The MICE spectrometer solenoids were designed to meet these requirements. Based on superconducting niobium-titanium (Nb-Ti), each of the two MICE spectrometer solenoids consists of five separate coils contained in a vacuum vessel of 2.7 m length and 1.4 m diameter. In this paper, we report on results from first measurements to verify initial magnet performance at the manufacturer site using a portable Hall-probe-based measurement system. A comparison with theoretical expectations based on OPERA simulations will be discussed and design aspects of the measurement system will be presented.

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<div type="abstract" xml:lang="en">The goal of the Muon Ionization Cooling Experiment (MICE) is to demonstrate muon cooling for a future muon collider. In order to quantify this cooling effect with high precision, scintillating fiber trackers in a uniform 4 Tesla field are required. The MICE spectrometer solenoids were designed to meet these requirements. Based on superconducting niobium-titanium (Nb-Ti), each of the two MICE spectrometer solenoids consists of five separate coils contained in a vacuum vessel of 2.7 m length and 1.4 m diameter. In this paper, we report on results from first measurements to verify initial magnet performance at the manufacturer site using a portable Hall-probe-based measurement system. A comparison with theoretical expectations based on OPERA simulations will be discussed and design aspects of the measurement system will be presented.</div>
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