Structure of Strong Plasma Shock Waves in a Transverse Magnetic Field

1962 ◽  
Vol 5 (12) ◽  
pp. 1590 ◽  
Author(s):  
G. G. Comisar
1979 ◽  
Vol 129 (11) ◽  
pp. 377 ◽  
Author(s):  
A.L. Velikovich ◽  
Mikhail A. Liberman

1979 ◽  
Vol 22 (11) ◽  
pp. 843-859 ◽  
Author(s):  
A L Velikovich ◽  
Mikhail A Liberman

1987 ◽  
Vol 115 ◽  
pp. 334-335
Author(s):  
David Hollenbach ◽  
C. McKee ◽  
D. Chernoff

The observed H2, CO, OI(63 μm), SiII(34.8 μm) and H51α emission line intensities in the BN-KL region of Orion are modeled as arising from two types of shock waves. The molecular emission arises from non-dissociative shocks with low peak postshock temperatures (< 3000 K), traveling at speeds of vs ∼ 40 km/s into ambient gas of density n0∼105-6 cm−3 and transverse magnetic field B0 ∼0.5 milligauss. The OI(63 μm), Sill(34.8 μm) and H51α emission arises in the cooling regions behind faster (∼80 km/s) dissociative shocks with high peak postshock temperatures (∼105 K) and with preshock densities n0 >3x104 cm−3.


2010 ◽  
Vol 46 (4) ◽  
pp. 393-402 ◽  
Author(s):  
F. Mokhtari ◽  
A. Bouabdallah ◽  
A. Merah ◽  
S. Hanchi ◽  
A. Alemany

2020 ◽  
Vol 58 (3) ◽  
pp. 400-409
Author(s):  
N. A. Luchinkin ◽  
N. G. Razuvanov ◽  
I. A. Belyaev ◽  
V. G. Sviridov

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