THE EMISSION OF RADIOACTIVE NUCLEI IN COSMIC RAY STARS

1951 ◽  
Vol 29 (4) ◽  
pp. 263-273 ◽  
Author(s):  
E. Pickup ◽  
L. Voyvodic

It has been found that a certain proportion of the fragments emitted in cosmic ray stars formed at about 85,000 ft. consists of radioactive nuclei, i.e., in electron sensitive photographic emulsions, tracks of electrons with energies of several mega electron volts can be seen originating at the end of the track of the fragment. Details of such events are given, together with energy measurements for the disintegration electrons made by the multiple Coulomb scattering method. The significance of the results, and possible identification of the fragments, are discussed.


2012 ◽  
Vol 14 (1) ◽  
pp. 013026 ◽  
Author(s):  
N Agafonova ◽  
A Aleksandrov ◽  
O Altinok ◽  
A Anokhina ◽  
S Aoki ◽  
...  


1951 ◽  
Vol 83 (4) ◽  
pp. 850-850 ◽  
Author(s):  
Martin J. Berger ◽  
J. J. Lord ◽  
Marcel Schein


1952 ◽  
Vol 88 (6) ◽  
pp. 1431-1432 ◽  
Author(s):  
Meera Backus ◽  
J. J. Lord ◽  
Marcel Schein


2019 ◽  
Vol 63 (10) ◽  
pp. 3420-3427 ◽  
Author(s):  
A.A. Leonov ◽  
A.M. Galper ◽  
N.P. Topchiev ◽  
A.V. Bakaldin ◽  
O.D. Dalkarov ◽  
...  


Author(s):  
S.A. Akimenko ◽  
V.I. Belousov ◽  
A.M. Blik ◽  
G.I. Britvich ◽  
V.N. Kolosov ◽  
...  


1968 ◽  
Vol 46 (10) ◽  
pp. S201-S203
Author(s):  
V. V. Guzhavin ◽  
I. P. Ivanenko ◽  
B. E. Samosudov

An analytical solution of the angular problem to the approximation of middle angles which is valid for any angles of particle deviation in an elementary event of Coulomb scattering has been obtained using the approximate operator (Vaskin et al. 1966). The proposed method makes it possible to evaluate the accuracy of the resulting expressions and the contribution from non-multiple and multiple Coulomb scattering.



Author(s):  
Hermann Fuchs ◽  
Stanislav Vatnitsky ◽  
Markus Stock ◽  
Dietmar Georg ◽  
Loïc Grevillot


1954 ◽  
Author(s):  
L.N. Cooper ◽  
J. Rainwater


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