A prototype radiation-chemistry system based on an ELV-2 electron accelerator

1990 ◽  
Vol 69 (3) ◽  
pp. 768-769
Author(s):  
M. É. Veis ◽  
V. A. Pechenin ◽  
A. S. Pecherkin ◽  
A. N. Polivanov ◽  
R. A. Salimov ◽  
...  
1970 ◽  
Vol 48 (19) ◽  
pp. 3029-3033 ◽  
Author(s):  
C. Willis ◽  
O. A. Miller

Carbon monoxide has been irradiated with single intense pulses from an electron accelerator at a dose rate of ~ 2 × 1027 eV g−1 s−1. The yield of carbon dioxide obtained was G(CO2) = 0.7 ± 0.1 with a very small yield of carbon suboxide, G(C3O2) ≤ 0.02.Addition of propene reduces the carbon dioxide yield to almost zero while addition of propane has no effect. This suggests that propene is acting as an oxygen atom scavenger rather than as a quencher of an excited state of carbon monoxide. However, rate constant data do not support this suggestion and it is concluded that the residual yield of carbon dioxide observed at high dose rates arises from reaction 9[Formula: see text]where CO+ is in an A2Π or B2Σ+ state.


Author(s):  
A. Strojnik ◽  
J.W. Scholl ◽  
V. Bevc

The electron accelerator, as inserted between the electron source (injector) and the imaging column of the HVEM, is usually a strong lens and should be optimized in order to ensure high brightness over a wide range of accelerating voltages and illuminating conditions. This is especially true in the case of the STEM where the brightness directly determines the highest resolution attainable. In the past, the optical behavior of accelerators was usually determined for a particular configuration. During the development of the accelerator for the Arizona 1 MEV STEM, systematic investigation was made of the major optical properties for a variety of electrode configurations, number of stages N, accelerating voltages, 1 and 10 MEV, and a range of injection voltages ϕ0 = 1, 3, 10, 30, 100, 300 kV).


1987 ◽  
Vol 48 (C9) ◽  
pp. C9-95-C9-98
Author(s):  
W. LOTZ ◽  
H. GENZ ◽  
A. RICHTER ◽  
W. KNÜPFER ◽  
J. P.F. SELLSCHOP

1975 ◽  
Vol 94 (4-6) ◽  
pp. 333-333
Author(s):  
K.-D. Asmus
Keyword(s):  

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