PRODUCTION OF N+-STAR FROM N-2+HV - EFFECTIVE EUV EMISSION YIELDS FROM LABORATORY AND DAYGLOW DATA

Photodissociative ionization of N2 into the unbound N2+ H 2-SIGMA-g+ state is identified as the parentage of a number of N+ and N excited states that contribute to the u.v. dayglow. Yields have been obtained for the production of extreme ultraviolet emission lines of N+ (and N) from a laboratory experiment using a broad-band synchrotron radiation source with fluorescence spectroscopy. The yields are termed "effective", in that they are constant percentages of the H state cross section. These are compared with effective yields needed to reproduce NII 1085 and 916 angstrom lines from four dayglow observations using a model of solar energy deposition and photoelectron production and loss in the Earth's thermosphere. The 1085 angstrom effective yield measured in the laboratory (18%) agrees with that from the dayglow data (average of 17%) to well within experimental uncertainties. Thus, we conclude that photodissociative ionization of N2 is the primary source of the NII 1085 angstrom dayglow. However, there is an order of magnitude discrepancy among the various dayglow observations of the 1085/916 intensity ratio, only one of which is consistent with the laboratory observation of 4.4. Neither contamination by other dayglow features nor atmospheric extinction can account for the disparities. Laboratory measurements of N2 and O2 absorption cross sections at these wavelengths are also reported.