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  • figure 7

Figure 7: Photodepletion kinetics of dicyanoacetylene ice.

From Photochemical activity of Titan’s low-altitude condensed haze

  • Murthy S. Gudipati1, 2,
  • Ronen Jacovi1, 7,
  • Isabelle Couturier-Tamburelli3,
  • Antti Lignell1, 7,
  • Mark Allen1, 4,
Journal name:
Nature Communications
Volume:
4,
Article number:
1648
DOI:
doi:10.1038/ncomms2649
Photodepletion kinetics of dicyanoacetylene ice.

Time variation of change in absorption at 2,244 cm−1 when C4N2 film at 100 K is photolysed at 355 nm (inset) and 266 nm. As expected for a forbidden and weak singlet-triplet absorption-induced photochemistry, the depletion of C4N2 is linearly proportion to the irradiation time when exposed at 355 nm, representing initial stages of an exponential process. Only 14% of C4N2 was depleted after ~1,400 min irradiation at ~50 mW cm−2. The last three points on the lower curve (filled squares) were obtained using higher laser power (160 mW cm−2 or 8 mJ per pulse), whereas the rest of the data were derived using a 50 mW cm−2 (2.5 mJ per pulse) laser power. Linearity of this curve when fluence is converted to time clearly indicates that the 355 nm photochemistry is a one-photon process. We also plotted these three points with 160 mW cm−2 laser power separately (filled circles). As discussed in the text, the slopes of these two curves scale linearly with the laser fluencies—confirming that the 355 nm photochemistry is indeed a one-photon process. The 266 nm photolysis through singlet-singlet excitation follows a monoexponential curve with over 35% depletion within the first 800 min of irradiation at 120 mW cm−2. Extrapolation towards the longer durations of the 266 nm photolysis may not be accurate due to simultaneous increase in extinction of the film at this wavelength from the formation of new products.

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Affiliations

  1. Jet Propulsion Laboratory, Science Division, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA

    • Murthy S. Gudipati,
    • Ronen Jacovi,
    • Antti Lignell &
    • Mark Allen
  2. IPST, University of Maryland, College Park, Maryland 20742, USA

    • Murthy S. Gudipati
  3. Laboratoire Physique des interactions ioniques et moléculaires, UMR CNRS 7345, Aix-Marseille Université, 13397 Marseille cedex 20, France

    • Isabelle Couturier-Tamburelli
  4. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA

    • Mark Allen
  5. Present addresses: Flight Control Group, Urban Aeronautics LTD, Nahal-Snir 10, Yavne 81224, Israel (R.J.); Arthur Amos Noyes Laboratory of Chemical Physics, California Institute of Technology, MC 127-72 1200 East California Boulevard, Pasadena, California 91125, USA (I.C.-T.)

    • Ronen Jacovi &
    • Antti Lignell

Contributions

M.S.G. and M.A. conceived the research ideas and wrote a significant part of the publication. M.S.G. coordinated the research activity, put the team together, involved in conducting the experiments, data analysis and data interpretation. R.J. and A.L. contributed to build infrastructure of the laboratory needed to synthesize the materials, conducted synthesis under the guidance of I.C. and majority of experiments described in this publication under the guidance of M.G. I.C. conducted the research in Marseille, France, as well as guided the synthesis and a part of photochemical investigations at JPL. R.J. performed the work as a NASA Post Doctoral Fellow at the Jet Propulsion Laboratory. A.L. performed a part of this work at the Jet Propulsion Laboratory during Academy of Finland fellowship.

Competing financial interests

The authors declare no competing financial interests.

Corresponding author

Correspondence to:

  • Murthy S. Gudipati

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  • Murthy S. Gudipati

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