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- W52600413 abstract "A cosmic-ray spectrograph is described for measuring the momentum spectrum and the positive excess in cosmic rays. The registration of the particles is done by parallelplate spark computers, three of which are placed above the magnetic field ard three below. When a coincidence occurs, the sparks will be intensified hy electroric means and photographed. The deflection of the panticles is done by a permanent magnet; the face area of the magnet is 5 x 20 cm/ sup 2/ and the distance between the poles is 2.5 cm; the strength of the magnetic field is 4000 gauss. The small error incurred in measurements of the single sparks (0.24 mm.), less expense, and smaller size gives this apparatus a certain advantege over the spectrographs which emplcy layers of G. M. counters to register the particles. (auth)" @default.
- W52600413 created "2016-06-24" @default.
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- W52600413 date "1959-10-01" @default.
- W52600413 modified "2023-09-24" @default.
- W52600413 title "A NEW TYPE OF COSMIC RADIATION PULSE SPECTROGRAPH" @default.
- W52600413 hasPublicationYear "1959" @default.
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