Performance of drift chambers in a magnetic rigidity spectrometer for measuring the cosmic radiation
1994; Elsevier BV; Volume: 345; Issue: 3 Linguagem: Inglês
10.1016/0168-9002(94)90516-9
ISSN1872-9576
AutoresM. Hof, M. Bremerich, W. Menn, C. Pfeifer, O. Reimer, M. Simon, J. W. Mitchell, L. Barbier, E. R. Christian, J. F. Ormes, R. E. Streitmatter, R. L. Golden, S. J. Stochaj,
Tópico(s)Solar and Space Plasma Dynamics
ResumoA drift chamber tracking system was developed and flown as part of the IMAX balloon-borne magnetic spectrometer. The drift chamber uses a hexagonal drift-cell structure and is filled with pure CO2 gas. It operated with high efficiency in the strong and inhomogenous field of a superconducting magnet, demonstrating a spatial resolution of better than 100 μm over most of the drift path for singly charged particles, as well as for helium and lithium nuclei. The drift chamber portion of the spectrometer achieved a maximum detectable rigidity of 175 and 250 GV/c for protons and helium respectively.
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