000001902 001__ 1902
000001902 005__ 20160701171655.0
000001902 037__ $$aASTROimport-59
000001902 100__ $$aGeller, M.
000001902 245__ $$aFirst identification of pure rotation lines of NH in the infrared solar spectrum
000001902 260__ $$c1991
000001902 520__ $$aPure rotation lines of NH of the v = 0 level and v = 1 level are detected in high-resolution solar spectra obtained from the Atmospheric Trace Molecule Spectroscopy (ATMOS) experimental observations. It is pointed out that the identification of the lines is favored by the typical appearance of the triplet lines of nearly equal intensities. The observed equivalent widths of these triplet lines are compared with predicted intensities, and it is observed that these widths are systematically larger than the predicted values. It is noted that because these very faint lines are observed in a region where the signal is very low, a systematic error in the measurements of the equivalent widths cannot be ruled out; therefore, the disagreement between the observed and predicted intensities is not considered to be real. 
000001902 700__ $$a Farmer, C. B.
000001902 700__ $$a Norton, R. H.
000001902 700__ $$a Sauval, A. J.
000001902 700__ $$a Grevesse, N.
000001902 773__ $$c550-552$$pAstronomy and Astrophysics$$v249$$y1991
000001902 85642 $$ahttp://esoads.eso.org/abs/1991A%26A...249..550G
000001902 905__ $$apublished in
000001902 980__ $$aREFERD