A Study of Electrothermal Launcher Efficiencies and Gas Dynamics

Author(s):  
Doyle Motes ◽  
Janet Ellzey ◽  
Scott Levinson ◽  
Jerry Parker ◽  
Francis Stefani ◽  
...  
2009 ◽  
Vol 45 (1) ◽  
pp. 568-573 ◽  
Author(s):  
D. Motes ◽  
J. Ellzey ◽  
S. Levinson ◽  
J. Parker ◽  
F. Stefani ◽  
...  

2011 ◽  
Vol 39 (2) ◽  
pp. 802-808
Author(s):  
D. Motes ◽  
M. Crawford ◽  
J. Ellzey ◽  
F. Stefani ◽  
D. Wetz

1967 ◽  
Vol 31 ◽  
pp. 117-119
Author(s):  
F. D. Kahn ◽  
L. Woltjer

The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to maintain the random motions in the interstellar gas is estimated as 1051·4±1ergs.


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