The electron-ion recombination coefficients for H3(+) and H5(+) ions were determined by means of a microwave afterglow/mass spectrometer apparatus. Measurements of electron density decays in helium-hydrogen mixtures are correlated with the decay of mass-identified ion currents to the wall of the microwave cavity. At low partial pressures of hydrogen in the mixture, the ion H3(+) dominates the ion composition and the ion wall current tracks the electron density decay curves. From recombination controlled electron density decay curves, the values alpha (H3(+)) = (2.9 + or - 0.3), (2.3 + or - 0.3), and (2.0 + or - 0.2) x 0.0000001 cu cm per sec, are obtained at 205, 300 and 450 K, respectively. At higher partial pressures of hydrogen and low t...
"August 3, 1949."Bibliography: p. 6.Army Signal Corps Contract No. W36-039-sc-32037 Project No. 102B...
We have investigated dissociative recombination (DR) of NH+ with electrons using a merged beams conf...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
A microwave afterglow mass spectrometer apparatus is used to determine the dependence on electron te...
$^{a}$J. M. Butler, L. M. Babcock, and N. G. Adams, Mol. Physics. 16, 81-90 (1997).Author Institutio...
We study binary and the recently discovered process of ternary He-assisted recombination of H-3+ ion...
During the current reporting period we have continued our studies of the dissociative recombination ...
We have been studying the dissociative recombination (DR) of HeH(+) with an electron with the goal o...
Flowing-afterglow measurements in decaying H3(+) or D3(+) plasmas suggest that de-ionization does no...
An important participant in interstellar chemistry is the H+3 molecular ion. Its concentration depen...
Measurements of recombination rate coefficients of binary and ternary recombination of H3+ and D3+ i...
An important participant in interstellar chemistry is the H+3 molecular ion. Its concentration depen...
The stationary afterglow with cavity ring down spectrometer (SA-CRDS) was used to study the recombin...
Measurements of recombination rate coefficients of binary and ternary recombination of H3+ and D3+ i...
A quantitative theory of ionization in diffuse clouds is developed which includes H(+) charge exchan...
"August 3, 1949."Bibliography: p. 6.Army Signal Corps Contract No. W36-039-sc-32037 Project No. 102B...
We have investigated dissociative recombination (DR) of NH+ with electrons using a merged beams conf...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...
A microwave afterglow mass spectrometer apparatus is used to determine the dependence on electron te...
$^{a}$J. M. Butler, L. M. Babcock, and N. G. Adams, Mol. Physics. 16, 81-90 (1997).Author Institutio...
We study binary and the recently discovered process of ternary He-assisted recombination of H-3+ ion...
During the current reporting period we have continued our studies of the dissociative recombination ...
We have been studying the dissociative recombination (DR) of HeH(+) with an electron with the goal o...
Flowing-afterglow measurements in decaying H3(+) or D3(+) plasmas suggest that de-ionization does no...
An important participant in interstellar chemistry is the H+3 molecular ion. Its concentration depen...
Measurements of recombination rate coefficients of binary and ternary recombination of H3+ and D3+ i...
An important participant in interstellar chemistry is the H+3 molecular ion. Its concentration depen...
The stationary afterglow with cavity ring down spectrometer (SA-CRDS) was used to study the recombin...
Measurements of recombination rate coefficients of binary and ternary recombination of H3+ and D3+ i...
A quantitative theory of ionization in diffuse clouds is developed which includes H(+) charge exchan...
"August 3, 1949."Bibliography: p. 6.Army Signal Corps Contract No. W36-039-sc-32037 Project No. 102B...
We have investigated dissociative recombination (DR) of NH+ with electrons using a merged beams conf...
Relevant data is available at: http://www.astronomy.ohio-state.edu/~nahar/nahar_radiativeatomicdata/...