OBSERVATION OF THE $3\nu_{2}\leftarrow 0$ OVERTONE BAND OF $H_{3}^{+}$

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1991

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Ohio State University

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We report the observation the second overtone band1 (3ν2(1=1)←0) of H3+ using a 1.45 μm InGaAsP near infrared diode laser with the short external cavity mode control technique developed at McMaster University.2 H3+ was generated using 1.5 Torr of H2 with or without 4∼5 Torr of He in a liquid-N2 cooled multiple-inlet-multiple-outlet discharge cell. The H3+ signal was detected with velocity modulation or ion concentration modulation in an AC glow discharge. Altogether four lines have been observed in the region of 6860--6925 cm−1. The positions of the lines were determined using a wavemeter calibrated with H2O reference lines. The assignment of the transitions is based on Miller and Tennyson’s first principles calculation3 and on observed temperature dependence of the relative intensities. Extended search of other transitions is being conducted. It is our hope that this observation may lead to detection of H3+ in higher vibrational states in Jupiter and other astronomical objects, and that it may also help in the assignment of the laboratory FTIR emission spectrum of hydrogen plasma.

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1S. S. Lee, B. F. Ventrudo, D. T. Cassidy, T. Oka, S. Miller, and J. Tennyson, J. Mol. Spec. 145, 222 (1991). 2D. T. Cassidy, Appl. Opt. 27, 610 (1988). 3S. Miller and J. Tennyson, private communication.""


Author Institution: Department of Chemistry and Department of Astronomy and Astrophysics, The University of Chicago; Department of Engineering Physics, McMaster University; Department of Physics and Astronomy, University College London

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