Future spaceborne spectrometers for astroparticle detection need high bending power therefore, the use of superconducting magnets is the sole applicable solution. Space magnets require high reliability that, in turn, requires high stability. Avoiding liquid helium cryogenics is also an attractive feature. The use of high temperature superconductors (HTS) or magnesium diboride (MgB2) combines both the requirements. The paper describes an HTS magnet operating at about 30 K that will be one of the main components of a space antimatter spectrometer. The magnet is a large toroid that will host a silicon tracker inside its internal volume and a 3D isotropic calorimeter in the center. The inner and outer diameters are 1 m and 4.3 m, respectively. The magnet mass is about 1200 kg.

A Proposal for a Superconducting Space Magnet for an Antimatter Spectrometer / Musenich R.; Adriani O.; Baudouy B.; Calvelli V.; Farinon S.; Papini P.; Bertucci B.. - In: IEEE TRANSACTIONS ON APPLIED SUPERCONDUCTIVITY. - ISSN 1051-8223. - ELETTRONICO. - 30:(2020), pp. 1-5. [10.1109/TASC.2020.2976970]

A Proposal for a Superconducting Space Magnet for an Antimatter Spectrometer

Adriani O.;Papini P.;
2020

Abstract

Future spaceborne spectrometers for astroparticle detection need high bending power therefore, the use of superconducting magnets is the sole applicable solution. Space magnets require high reliability that, in turn, requires high stability. Avoiding liquid helium cryogenics is also an attractive feature. The use of high temperature superconductors (HTS) or magnesium diboride (MgB2) combines both the requirements. The paper describes an HTS magnet operating at about 30 K that will be one of the main components of a space antimatter spectrometer. The magnet is a large toroid that will host a silicon tracker inside its internal volume and a 3D isotropic calorimeter in the center. The inner and outer diameters are 1 m and 4.3 m, respectively. The magnet mass is about 1200 kg.
2020
30
1
5
Musenich R.; Adriani O.; Baudouy B.; Calvelli V.; Farinon S.; Papini P.; Bertucci B.
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1239442
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