Air radiation tables - Spectral distribution functions for molecular band systems
Air radiation tables - spectral distribution functions for diatomic molecular band systems
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Air radiation tables - spectral distribution functions for diatomic molecular band systems
Oscillator strength of CN violet system from shock layer by time-of-flight scanning spectrometer
Helium afterglow discussing stability of collisional-radiative recombination of ions with electrons and neutral particles
Perturbation effects in differential elastic ion- atom scattering generated by crossing of molecular states from even potentials
Approximation of expectation values for nonenergy properties via perturbation theory, obtaining values for molecular polarizability
Numerical values describing molecular rainbow scattering in Airy approximation for 12-6 potential
Electron spin resonance of gamma irradiated single crystal of barbituric acid dihydrate, noting formation and Hamiltonian parameters of free radicals
Color centers in alkali metal azides, noting change of ion from linear to bent configuration
Microwave spectroscopy used to identify unambiguously contaminant trace gases in mixture and indicate amount of each
Collisions in inner region of cometary head, structure of emission bands and formation of free radicals
Beam foil excitation technique application in measuring mean lives of 2p and 3p levels of hydrogen
Microwave spectroscopy used in identification of atmospheric trace contaminants
Shock layer radiation predictions from molecular band systems in Martian and Venusian atmospheres
Chemical activity and comet phenomena - photochemical models of astrophysical reactions, electron bombardment of low pressure gases, and singlet carbide studies
Collision induced dissociation of deuterium by argon and nitrogen examined with angular ion scattering apparatus, determining kinetic energy and angular distribution
1/s line intensity distribution function for molecular spectra representation using growth curves calculated for Lorentz lines
Expression for electron contribution to Stark broadening, using impact approximation with Lewis or Debye cut-offs
CH molecule solar spectral observations interpreted using several upper photosphere models and assuming local thermodynamic equilibrium approximation