Secure Coding for Type II Quantum Wiretap Channel

2018 ◽  
Vol 57 (11) ◽  
pp. 3318-3325
Author(s):  
Heling Xiao ◽  
Huifeng Wang
2012 ◽  
Vol 7 (4) ◽  
pp. 1414-1418 ◽  
Author(s):  
Won Taek Song ◽  
Jinho Choi ◽  
Jeongseok Ha

Author(s):  
Vaneet Aggarwal ◽  
Lifeng Lai ◽  
A. Robert Calderbank ◽  
H. Vincent Poor
Keyword(s):  
Type Ii ◽  

1994 ◽  
Vol 144 ◽  
pp. 283-284
Author(s):  
G. Maris ◽  
E. Tifrea

The type II solar radio bursts produced by a shock wave passing through the solar corona are one of the most frequently studied solar activity phenomena. The scientific interest in this type of phenomenon is due to the fact that the presence of this radio event in a solar flare is an almost certain indicator of a future geophysical effect. The origin of the shock waves which produce these bursts is not at all simple; besides the shocks which are generated as a result of a strong energy release during the impulsive phase of a flare, there are also the shocks generated by a coronal mass ejection or the shocks which appear in the interplanetary space due to the supplementary acceleration of the solar particles.


Author(s):  
Ronald S. Weinstein ◽  
N. Scott McNutt

The Type I simple cold block device was described by Bullivant and Ames in 1966 and represented the product of the first successful effort to simplify the equipment required to do sophisticated freeze-cleave techniques. Bullivant, Weinstein and Someda described the Type II device which is a modification of the Type I device and was developed as a collaborative effort at the Massachusetts General Hospital and the University of Auckland, New Zealand. The modifications reduced specimen contamination and provided controlled specimen warming for heat-etching of fracture faces. We have now tested the Mass. General Hospital version of the Type II device (called the “Type II-MGH device”) on a wide variety of biological specimens and have established temperature and pressure curves for routine heat-etching with the device.


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