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Technical Design Report Super Fragment Separator

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DRAFT<br />

Figure 2.4.17: Spectrometer mode of the LEB Energy-Buncher. 132 Sn fission fragments impinge on the<br />

secondary target (C 50 mg/cm 2 ) placed at MF10. The secondary fragments ( 129,130,131 Sn) are analyzed by<br />

the spectrometer in combination with particle detectors. The example calculated with the MOCADI program<br />

demonstrates the achieved mass resolving power of 185, assuming a time-of-flight resolution of about 80 ps<br />

over the flight path of 13 m.<br />

2.4.2 Magnets<br />

<strong>Super</strong>conducting magnets<br />

The <strong>Super</strong>-FRS has to accept fragment beams with a large phase-space volume. Therefore, it requires<br />

large aperture magnets. Furthermore, the magnets have to provide high magnetic pole-tip<br />

flux densities to guide the 20 Tm ion beams. The dipole magnets of the separator will have a deflection<br />

radius of 12.5 m, a maximum field of 1.6 T, and a gap of 170 mm. Most of the quadrupole<br />

lenses require a good field aperture of 380 mm with a pole tip flux density of up to 2.4 T. These<br />

specifications favour the use of superconductivity. The magnet design will make use of superferric<br />

technology with iron-dominated lenses where the magnetic field is formed by shaped iron yokes<br />

driven by superconducting coils. This technology is already successfully applied at the A1900<br />

in-flight fragment separator at MSU, USA [8], at the BigRIPS fragment separator at RIKEN, Japan<br />

[9] and will be also applied at the future in-flight separators for RIA in the USA [10]. However, all<br />

of these facilities will work at much lower beam energies and hence the magnets are much smaller<br />

compared to those of the <strong>Super</strong>-FRS.<br />

Radiation resistant magnets<br />

Besides the operation of the large aperture magnets the other main challenge is the high radiation<br />

level in the target area and the first dipole stage of the Pre-<strong>Separator</strong> where the non-reacted primary<br />

23

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