The BESS-Polar Ultra-Thin Superconducting Solenoid Magnet and Its Operational Characteristics During Long-Duration Scientific Ballooning Over Antarctica

An ultra-thin superconducting solenoid has been developed for a cosmic-ray spectrometer ballooning over Antarctica, which is named BESS-Polar II. The coil with a diameter of 0.9 m, a length of 1.4 m and a thickness of 3.5 mm, is wound with high-strength aluminum stabilized superconductor and provide...

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Veröffentlicht in:IEEE transactions on applied superconductivity 2009-06, Vol.19 (3), p.1315-1319
Hauptverfasser: Makida, Y., Yamamoto, A., Yoshimura, K., Tanaka, K.-i., Suzuki, J., Matsuda, S., Hasegawa, M., Horikoshi, A., Shinoda, R., Sakai, K., Mizumaki, S., Orito, R., Matsukawa, Y., Kusumoto, A., Mitchell, J.W., Streitmatter, R.E., Hams, T., Sasaki, M., Thakur, N.
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Sprache:eng
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Zusammenfassung:An ultra-thin superconducting solenoid has been developed for a cosmic-ray spectrometer ballooning over Antarctica, which is named BESS-Polar II. The coil with a diameter of 0.9 m, a length of 1.4 m and a thickness of 3.5 mm, is wound with high-strength aluminum stabilized superconductor and provides 0.8 T in the spectrometer. Based on the experience at the BESS-Polar-I solenoid flight for nine days in 2004, the BESS-Polar-II solenoid, which was cryogenically improved, realized a persistent current mode operation for 25 days in the second flight campaign in December 2007 though January 2008. It has contributed to accumulate the cosmic-ray observation data with 4700 million events and 16 terabyte in a hard disk unit. This report will describe the second solenoid performance during the flight.
ISSN:1051-8223
1558-2515
DOI:10.1109/TASC.2009.2017946