1949
DOI: 10.1364/josa.39.000891
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The Photographic Action of X-Rays in the 13 to 001A Range*

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1953
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Cited by 10 publications
(1 citation statement)
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“…The emission of a high energy photon depends on a highly inelastic collision before much ionization energy loss occurs and is very improbable. Nevertheless, the contribution of x-rays may not be negligible, for it is well established that a single absorbed photon of energy greater than a few key will produce a developable grain [15][16][17][18] and the emulsion has a high stopping power for x-rays below about 30 kev. It is only necessary for x-rays to be produced with a probability of the same order as the relevant value of M. quoted in table 1 for a contribution to be apparent.…”
Section: M(a)da= (2 ) Moa2 a ) 9(a) Damentioning
confidence: 99%
“…The emission of a high energy photon depends on a highly inelastic collision before much ionization energy loss occurs and is very improbable. Nevertheless, the contribution of x-rays may not be negligible, for it is well established that a single absorbed photon of energy greater than a few key will produce a developable grain [15][16][17][18] and the emulsion has a high stopping power for x-rays below about 30 kev. It is only necessary for x-rays to be produced with a probability of the same order as the relevant value of M. quoted in table 1 for a contribution to be apparent.…”
Section: M(a)da= (2 ) Moa2 a ) 9(a) Damentioning
confidence: 99%