Excitation of hydrogen molecules by electron impact. II - Excitation to D/3ppi 1piu/ state
Excitation of hydrogen molecules by electron impact
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Excitation of hydrogen molecules by electron impact
Exchange excitation of hydrogen molecule by electron impact from ground to triplet electronic state
Fluid behavior in cylindrical tank under relatively low frequency random longitudinal excitation
Fluid behavior in unbaffled circular cylindrical tank under relatively low frequency random lateral excitation
Excitation and luminescence of solids subjected to surface-catalyzed atom recombination and photoexcitation
Parabolic coordinate evaluation of atomic form factor of hydrogen atom for excitation cross section induced by electron collision
Subexcitation molecular collisions resonances demonstrated by numerical solution of integral equations for rotational excitation, exhibiting adiabatic approximation limitations
Hydrogen and inert gas atoms collisional excitation cross sections calculated by multistate impact parameter approximation
Vibrationally excited ground state hydroxyl in fast flow system, considering mean radiative lifetime and reaction rate with ozone
Symmetric excited state electron capture cross sections in ion-atom inelastic scattering, using two state approximation formulas
Excitation of neutral atoms by inelastic scattering of incident electrons in gaseous nebulae were investigated using Slater Wave functions to describe the initial and final states of the atom. Total cross sections using the Born Approximation are calculated for: Li(2s yields 2p), Na(3s yields 4p), k(4s yields 4p). The intensity of emitted radiation from gaseous nebulae is also calculated, and Maxwell distribution is employed to average the kinetic energy of electrons.
Time dependent matrix elements for multistate impact-parameter calculations for atom-atom inelastic cross sections
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A new local oscillator housing was built which seems to have improved laser life. Laser cooling was changed from internal water cooling to the more convenient thermal contact cooling. At the present time, a conclusion can not be made if the 20 percent reduction in power output is the result of poorer cooling or poorer grating alignment. The coupling-starting network was improved from 55 to about 90 percent. It can be adjusted by varying trimmers C sub 1 and C sub 2 to match RF power levels between 10 and 30 W. If the laser admittance changes greatly with laser life rematching will have to be achieved by remote control for space applications. The same holds true if the RF power level has to be changed with a maximum efficiency constraint.