Titlebook: Laser Interaction and Related Plasma Phenomena; Proceedings of the F Helmut J. Schwarz (Professor of Physics),Heinrich Conference proceedi

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書目名稱Laser Interaction and Related Plasma Phenomena影響因子(影響力)




書目名稱Laser Interaction and Related Plasma Phenomena影響因子(影響力)學科排名




書目名稱Laser Interaction and Related Plasma Phenomena網絡公開度




書目名稱Laser Interaction and Related Plasma Phenomena網絡公開度學科排名




書目名稱Laser Interaction and Related Plasma Phenomena被引頻次




書目名稱Laser Interaction and Related Plasma Phenomena被引頻次學科排名




書目名稱Laser Interaction and Related Plasma Phenomena年度引用




書目名稱Laser Interaction and Related Plasma Phenomena年度引用學科排名




書目名稱Laser Interaction and Related Plasma Phenomena讀者反饋




書目名稱Laser Interaction and Related Plasma Phenomena讀者反饋學科排名

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Nutrient

employor

Scattering of Laser Radiationssible studies of non-linear scattering effects which could not have been undertaken readily, if at all, with conventional sources. In the present paper, an attempt will be made to survey some recent scattering experiments and theory. No attempt at completeness is made.

Spartan

Shock Wave Process and Numerical Calculationsoncluded that a non-transparent layer is formed on the surface of the solid in the very early stages of the irradiation process. Most of the laser energy is absorbed in this layer, and a hot plasma is formed and expands with high velocities. The reaction forces produce a shock wave in the solid.

異端邪說下

效果

Numerical Calculations of Plasma Heating by Means of Subnanosecond Laser Pulsesion of state. The calculation technique is applied to various experimental situations, including the recent lithium deuteride thick target neutron detection experiments, and the results are presented.

BROTH

騷動

Thin Films of Metals and Inorganic Compounds Vacuum Deposited by High Energy Laser kinetic energy equivalent to at least the condensation heat; it is of the order of 5–10 eV or more. By changing the deposition rate with conventional thermal evaporation sources the velocity is not affected so much, since it is only a function of the square root of the temperature, whereas a much g

MITE