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Titlebook: Energetic Charged-Particle Interactions with Atmospheres and Surfaces; Robert E. Johnson Book 1990 Springer-Verlag Berlin Heidelberg 1990

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Pore Structure and Pore Types of Shales,ts and neutral gases. Therefore, an understanding of the interaction of energetic plasma particles with solids and gases may be required in order to interpret remote sensing observations both in our solar system and in the interstellar media. The nature of the energetic, charged-particle radiations
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F. Watchorn,G. J. Nichols,D. W. J. Bosenceities such as penetration depths scale very nearly with the atomic (molecular) density of the material. This is true even for metals, for which the electrons in the solid state show cooperative (plasma) effects absent in gases and insulating solids. Notable exceptions are crystalline solids in which
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Collision Physics,lness of classical or semi-classical methods can be established: collision energies much greater than a Rydberg (27.2 eV) for incident electrons and much greater than hundredths of an eV for incident ions. For ions, atoms, or molecules this criterion is satisfied for the full energy range of interes
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Two-Phase Flow Analysis of Sediment Velocitylness of classical or semi-classical methods can be established: collision energies much greater than a Rydberg (27.2 eV) for incident electrons and much greater than hundredths of an eV for incident ions. For ions, atoms, or molecules this criterion is satisfied for the full energy range of interes
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F. Watchorn,G. J. Nichols,D. W. J. Bosence treated as gases of a given density when discussing incident particle penetration and energy deposition. The material properties are introduced latter when describing the fate of the energy deposited.
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