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NONEQUILIBRIUM FLOWS WITH POPULATION INVERSION IN SHOCK WAVES V. M. Kuznetsov UDC 533.6.011.72 The effect of incident flow parameters and composition of a CO 2 + N 2 + H20( He ) mixture on population inversion ...
). We assume that gas cools behind the shock at the optically thin rate, \begin{eqnarray*} \dot{q} = \Lambda (T)n_\text{e} n_\text{p}, \end{eqnarray*} ( 2 ) where ne and np are the number densities of free ...
in the cooling layers of the shocks is slightly overestimated, which results in slightly longer relaxation scales behind the adiabatic fronts (by 30 per cent on a shock of about 2 km s−1). For a fair comparison ...
and 833 are HR. 4254 have had active lipid management in the preceding 2 years. In all patients the low-density lipoprotein control rates are 59% in the VHR population and 72% in the HR population ...
\left(\omega _i (t-P/ 2 ) - \frac{3\pi }{4}\right)\right.\nonumber\\ -\left.i\omega \ cos \left(\omega _i (t-P/ 2 )-\frac{3\pi }{4}\right)\right]. \end{eqnarray*}$$(37) Clearly this solution describes a wave ...
of grains formed in Population III supernovae. The second method of modelling dust formation in supernovae is kinetic nucleation theory (KNT). In the KNT, the number densities cn of clusters of n ≥ 2 atoms ...
impact of directed shock propagation on risk premia depends on the tradeoff between these channels. We disentangle the three channels for arbitrary directed networks. However, the intuition behind them ...
to strain accumulation on the low-angle thrusts along its margins may modulate the slip history of the normal faults within the plateau. 2 OBSERVATIONS OF ACTIVE NORMAL FAULTING The high Andes in southern ...
tabDownload slide Kaplan–Meier curves for death. Table 1. Endpoint . Total population ( n =101) . Normal coronary flow ( n =83) . Coronary slow flow ( n =18) . P . Intra-hospital complications, n (%) 40 (39.6) 28 ...
$$\boldsymbol {v}_{\rm d} = 1 \, {\rm km} \, {\rm s}^{-1} \, \boldsymbol {\hat{z}}$$, and gas has uniform density ρg = 2 × 107 M⊙ kpc−3, corresponding to an ISM-like number density n ∼ 1 cm−3. The uniform dust ...
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