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Naji, M. |
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Motta, Antonella |
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Aletan, Dirar |
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Mohamed, Tarek |
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Ertürk, Emre |
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Taccardi, Nicola |
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Kononenko, Denys |
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Petrov, R. H. | Madrid |
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Alshaaer, Mazen | Brussels |
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Bih, L. |
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Casati, R. |
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Muller, Hermance |
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Kočí, Jan | Prague |
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Šuljagić, Marija |
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Kalteremidou, Kalliopi-Artemi | Brussels |
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Azam, Siraj |
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Ospanova, Alyiya |
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Blanpain, Bart |
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Ali, M. A. |
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Popa, V. |
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Rančić, M. |
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Ollier, Nadège |
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Azevedo, Nuno Monteiro |
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Landes, Michael |
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Rignanese, Gian-Marco |
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Baratta, Giuseppe
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Topics
Publications (10/10 displayed)
- 2016Wild 2 grains characterized combining MIR/FIR/Raman micro-spectroscopy and FE-SEM/EDS analyses
- 2011Formation of CO_2 and OCS after cosmic ion irradiation of icy grain mantles
- 2007Combined Micro-Infrared (IR) and Micro-Raman Measurements on Stratospheric Interplanetery Dust Particles
- 2004Raman spectroscopy of ion irradiated diamondcitations
- 2004Infrared and Raman spectroscopies of refractory residues left over after ion irradiation of nitrogen-bearing icy mixturescitations
- 2004A Raman study of ion irradiated icy mixturescitations
- 2004Raman and photoluminescence study of ion beam irradiated porous silicon: a case for the astrophysical extended red emission?citations
- 2003A Raman study of ion irradiated icy mixtures
- 2002Infrared and Raman spectroscopy of refractory residues left over after ion irradiation of nitrogen bearing icy mixtures
- 2000Laboratory and astronomical IR spectra: an experimental clue for their comparison
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article
A Raman study of ion irradiated icy mixtures
Abstract
In this paper we present a Raman study of pure CH<SUB>4</SUB>, H<SUB>2</SUB>O:CH<SUB>4</SUB>:N<SUB>2</SUB> and CH<SUB>3</SUB>OH:N<SUB>2</SUB> frozen films before and after ion irradiation at 12 K, 100 K and 300 K. By means of Raman spectroscopy, we monitor the structural evolution of each film, whose chemical and physical properties are deeply modified by the interaction with the ion beam. For the two methane containing samples, Raman spectra show that the initial ice is partially converted into a refractory residue, which under further irradiation evolves towards an amorphous carbon (AC) with a band near 1560 cm<SUP>-1</SUP> (G line) and a shoulder at about 1360 cm<SUP>-1</SUP> (D line). No evidence of the AC Raman band is seen in the spectra of the methanol-containing mixture. By means of Lorentzian fits, we have determined the specific parameters of the AC band (G and D line peak positions, widths and relative intensities) in our spectra after ion irradiation and we have compared them with the corresponding parameters of the band as observed in the spectra of 11 IDPs (Interplanetary Dust Particles). Here we present the experimental results and discuss their contribution to our knowledge of the origin and evolution of IDPs....