Kinetic energies of fragment ions produced by dissociative photoionization of NO |
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| Affiliation: | 1. Dpto. de Física de la Tierra y Astrofísica, Universidad Complutense de Madrid (UCM), Avd. Complutense s/n, 28040-Madrid, Spain;2. Instituto de Geociencias IGEO (UCM, CSIC), Calle Severo Ochoa 7, Edificio Entrepabellones 7 y 8, 28040-Madrid, Spain;1. Science Policy Research Unit (SPRU), Room 325, Jubilee Building, University of Sussex, Brighton, UK;2. Science Policy Research Unit (SPRU), Room 368, Jubilee Building, University of Sussex, Brighton, UK;3. Finnish Environment Institute, 140 00251, Helsinki, Finland;1. Henan University of Urban Construction, Pingdingshan 467041, China;2. School of Surveying and Land Information Engineering, Henan Polytechnic University, Jiaozuo 454000, China;3. Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;4. The First Monitoring and Application Center, China Earthquake Administration, Tianjin 300180, China;1. Space and Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, NM, USA;2. Institut de Mécanique des Fluides de Toulouse, Université de Toulouse III Paul Sabatier, INP, CNRS, Toulouse, France;3. Department of Physics, University of Louisiana at Lafayette, Lafayette, LA, USA;4. Space Exploration Sector, Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA;5. Institut de Recherches en Astrophysique et Planétologie (IRAP), Toulouse, France;6. Institute of Optical Sensor Systems, German Aerospace Center (DLR), Berlin, Germany;7. Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN, USA;8. Institut Supérieur de l''Aéronautique et de l''Espace (ISAE-SUPAERO), Université de Toulouse, Toulouse, France;9. LESIA, Observatoire de Paris, Université PSL, Sorbonne Université, Université de Paris, CNRS, Meudon, France;10. Institute of Sound and Vibration Research, University of Southampton, Southampton, United Kingdom;11. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA;12. Física Aplicada, Escuela de Ingeniería de Bilbao, UPV/EHU, Bilbao, Spain;13. Lunar and Planetary Institute, Universities Space Research Association, Houston, TX, USA;14. Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA;15. Aeolis Research, Chandler, AZ, USA;p. Centro de Astrobiología (INTA-CSIC), Madrid, Spain;q. Finnish Meteorological Institute, Helsinki, Finland;1. Research Center for Eco-Environmental Sciences, Chinese Academy of Sciences, Beijing 100085, China;2. University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing 100049, China |
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| Abstract: | The kinetic energies of ions produced by dissociative photoionization of NO have been measured at the discrete resonance lines of He (584 Å) and Ne (736 Å), and with undispersed synchrotron radiation. O+ ions were identified with energies from 0 to approximately 0.5 eV and two groups of N+ ions one with energy of 0.36 eV and another with energies between 0.9 and 1.5 eV, apparently produced by predissociation of the c3Π and B′1Σ states, respectively. |
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