scholarly journals Competitive thermal and photochemical processes in cyclopropylketone rearrangements. II. Thermal isomerization of spiro[n.2]alkan-2-ones

1978 ◽  
Vol 56 (6) ◽  
pp. 808-813 ◽  
Author(s):  
Prabhaker G. Khazanie ◽  
Edward Lee-Ruff

Conformationally-rigid methyl-substituted cyclopropyl ketones with a suitably disposed γ-hydrogen undergo thermal type II reactions efficiently. Comparison of yields of these rearrangements with their photochemical analogs suggest that photochemical type II reactions arise from excited vibrational states. In the absence of a suitably disposed γ-hydrogen, and if strain factors permit, such systems undergo oxovinylcyclopropane to dihydrofuran rearrangement. The inertness of these systems to undergo such thermal rearrangement increased on going from cyclohexanone to the cyclopentanone series.

1978 ◽  
Vol 56 (6) ◽  
pp. 803-807 ◽  
Author(s):  
Edward Lee-Ruff ◽  
Prabhakar Govind Khazanie

The series of cyclopropyl ketones 1–6 was irradiated in methanol. Cyclopentanones 1 and 2 gave mainly products of type I reaction whereas ketones 3, 5, and 6 gave type II products. Formation of type II products can arise by two different mechanisms. One involves the intermediacy of a dienol which can be trapped with methanol-OD. Photochemical degradation of the cyclopentanones was slower than the corresponding cyclohexanones.


Heterocycles ◽  
1977 ◽  
Vol 6 (9) ◽  
pp. 1569 ◽  
Author(s):  
Hideo Nemoto ◽  
Hideharu Seto ◽  
Tetsuji Kametani

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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