%0 Journal Article %1 xianming1998electronimpact %A Liu, Xianming %A Shemansky, D. E. %A Ahmed, Syed M. %A James, G. K. %A Ajello, J. M. %D 1998 %I AGU %J J. Geophys. Res. %K electron emission excitation impact %N A11 %P 26739--26758 %T Electron-impact excitation and emission cross sections of the H2 Lyman and Werner Systems %U http://dx.doi.org/10.1029/98JA02721 %V 103 %X Excitation functions of the H2 Lyman (Ly) ( B 1∑u+-X 1∑g+ ) and Werner (W) ( C 1∏u-X 1∑g+ ) band systems have been reanalyzed using a combination of measurements and theoretical considerations. These systems are prominent emitters in outer planet atmospheric dayglow and auroral activity and can be used to infer energy deposition and heating rates. Earlier measurements of the cross sections reported by Shemansky et al. 1985a have been found to be inaccurate in the threshold energy region. A combination of high-resolution spectral and shape function measurements obtained at the Jet Propulsion Laboratory (JPL) in low- and medium-energy regions have been used to obtain relative excitation shape functions of the two systems. At energies above 250 eV, we have used the measurements obtained earlier by De Heer and Carri�re 1971 in order to define the first two terms of the Born electric dipole collision strength. The complete set of collision strength terms is obtained by combining the JPL and De Heer and Carri�re 1971 data. We have found that, contrary to results of Shemansky et al. 1985a, the shape functions of the H2 Ly and W systems, expressed in units of threshold energy, are the same within experimental error. Absolute cross sections of the H2 Ly and W systems are established using the theoretical oscillator strengths of Abgrall et al. 1987, 1993a, b, c and Abgrall and Roueff 1989. The atomic hydrogen H Ly α emission cross section resulting from dissociative excitation of H2 at 100 eV obtained from relative intensities of H2 W emission lines is also derived and compared with other experimental measurements. At a gas temperature of 300 K and electron energy of 100 eV, the cross sections for the H Ly α, H2 Ly, and W emissions are (0.716 � 0.095) � 10−17, (2.62 � 0.34) � 10−17, and (2.41 � 0.31) � 10−17 cm2, respectively. The accuracy of the absolute values and shape functions is limited primarily by electron gun performance, as was the case for Shemansky et al. The rotational dependence of the transition dipole matrix elements and perturbations between the B 1∑u+ and C 1∏u+ states have a significant effect on the cross sections.

@article{xianming1998electronimpact, abstract = {Excitation functions of the H2 Lyman (Ly) ( B&#8201;1&#8721;u+-X&#8201;1&#8721;g+ ) and Werner (W) ( C&#8201;1&#8719;u-X&#8201;1&#8721;g+ ) band systems have been reanalyzed using a combination of measurements and theoretical considerations. These systems are prominent emitters in outer planet atmospheric dayglow and auroral activity and can be used to infer energy deposition and heating rates. Earlier measurements of the cross sections reported by Shemansky et al. [1985a] have been found to be inaccurate in the threshold energy region. A combination of high-resolution spectral and shape function measurements obtained at the Jet Propulsion Laboratory (JPL) in low- and medium-energy regions have been used to obtain relative excitation shape functions of the two systems. At energies above 250 eV, we have used the measurements obtained earlier by De Heer and Carri�re [1971] in order to define the first two terms of the Born electric dipole collision strength. The complete set of collision strength terms is obtained by combining the JPL and De Heer and Carri�re [1971] data. We have found that, contrary to results of Shemansky et al. [1985a], the shape functions of the H2 Ly and W systems, expressed in units of threshold energy, are the same within experimental error. Absolute cross sections of the H2 Ly and W systems are established using the theoretical oscillator strengths of Abgrall et al. [1987, 1993a, b, c] and Abgrall and Roueff [1989]. The atomic hydrogen H Ly &#945; emission cross section resulting from dissociative excitation of H2 at 100 eV obtained from relative intensities of H2 W emission lines is also derived and compared with other experimental measurements. At a gas temperature of 300 K and electron energy of 100 eV, the cross sections for the H Ly &#945;, H2 Ly, and W emissions are (0.716 � 0.095) � 10&#8722;17, (2.62 � 0.34) � 10&#8722;17, and (2.41 � 0.31) � 10&#8722;17 cm2, respectively. The accuracy of the absolute values and shape functions is limited primarily by electron gun performance, as was the case for Shemansky et al. The rotational dependence of the transition dipole matrix elements and perturbations between the B&#8201;1&#8721;u+ and C&#8201;1&#8719;u+ states have a significant effect on the cross sections.}, added-at = {2010-05-16T15:34:06.000+0200}, author = {Liu, Xianming and Shemansky, D. E. and Ahmed, Syed M. and James, G. K. and Ajello, J. M.}, biburl = {https://www.bibsonomy.org/bibtex/2227c13ceebefbda4b1aa2712aca60d17/gensemer}, description = {Electron-impact excitation and emission cross sections of the H<sub xmlns="">2</sub> Lyman and Werner Systems}, interhash = {cf5c664b4a2d4afd91b447c43fd4911f}, intrahash = {227c13ceebefbda4b1aa2712aca60d17}, issn = {01480227}, journal = {J. Geophys. Res.}, keywords = {electron emission excitation impact}, number = {A11}, pages = {26739--26758}, publisher = {AGU}, timestamp = {2010-05-16T15:34:06.000+0200}, title = {Electron-impact excitation and emission cross sections of the H2 Lyman and Werner Systems}, url = {http://dx.doi.org/10.1029/98JA02721}, volume = 103, year = 1998 }