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As the superluminal wave encounters the wind's termination shock, it locally affects the state of the hot, radiative plasma in the shock interior and the downstream medium, possibly with an observable signature.
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In 1976 it was shown that a linearly polarized laser beam interacting with hot magnetized plasma produces a radiative force along the electric field of laser beam.
Providing continuous day and night sub-ambient cooling and dissipation of low grade heat from renewable power systems without use of water or external energy under direct sunlight and other applications have made clear sky radiative cooling a hot research topic.
The paper provides a first-stage, simplified, theoretical analysis to show how receiverefficiency (from a radiative perspective) and hot-spot temperatureare affected by the number of heat transfer layers and the degree to which each layer blocks the radiation.
Then having computed the energy deposition rates vs. altitude we compute the hydrodynamic and radiative expansion of the hot wake material in the radial direction, along with the associated air chemistry.
These large n-alkane droplets exhibited radiative extinction of the hot flame, followed by quasi-steady low-temperature burning, which terminated with diffusive extinction accompanied by the formation of a vapor cloud, while small droplets did not exhibit radiative extinction but instead burned to completion or disruptively extinguished.
Because hot star winds are driven radiatively, the modified ionization equilibrium affects the radiative force.
To obtain the total hot-bed-to-surface coefficients, a radiative component is then added.
No radiative heat transfer at the hot side was assumed.
Heat conduction in the solid plates and radiative heat transfer from the hot catalytic surfaces were accounted for in the model.
Results demonstrate that radiative heat transfer from a hot downstream environment to the porous plug significantly increases maximum attainable mass fluxes.
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