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Long D.G. & Drinkwater M.R. (1999). Cryosphere applications of NSCAT data : Special issue on ADEOS. IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 37(3), 1671–1684.
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Frezzotti M. & Flora O. (2002). Ice dynamics and climatic surface parameters in East Antarctica from Terra Nova Bay to Talos Dome and Dome C: ITASE Italian Traverses. Terra antarctica, 9(1), 47–54.
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. (2002).1, 15–27.
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Petit J.R., Blot M. & Bulat S. (2003). Bachelor's thesis, , .
Abstract: Presses Universitaires de Bordeaux
Programme: 355
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Vernon P. & Vannier G. (2002). Evolution of freezing susceptibility and freezing tolerance in terrestrial arthropods. Comptes rendus de biologies, 325, 1185–1190.
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. (2001). Comments on New insight into the structure of the Nuussuaq Basin. Central West Greenland, MPG, 1999.
Abstract: from Chalmers et al.
Programme: 290
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. (2002). Artificial ion tracks in volcanic dark mica simulating natural radiation damage: a scanning force microscopy study. Nuclear Instruments and Methods in Physics Research Section B, 191(1-4), 346–351.
Abstract: A new dating technique uses alpha-recoil tracks (ART), formed by the natural /?-decay of U, Th and their daughter products, to determine the formation age of Quaternary volcanic rocks (/<106 a). Visualization of etched ART by scanning force microscopy (SFM) enables to access track densities beyond 108cm-2 and thus extend the new ART-dating technique to an age range />106 a. In order to simulate natural radiation damage, samples of phlogopite, originating from Quaternary and Tertiary volcanic rocks of the Eifel (Germany) and Kerguelen Islands (Indian Ocean) were irradiated with U, Ni (11.4 MeV/u), Xe, Cr, Ne (1.4 MeV/u) and Bi (200 keV) ions. After irradiation and etching with HF at various etching times, phlogopite surfaces were visualized by SFM. Hexagonal etch pits are typical of U, Xe and Cr ion tracks, but the etch pits of Ni, Ne and Bi ion tracks are triangular. Surfaces irradiated with U, Xe, Cr and Ni ions do not show any significant difference between etch pit density and irradiation fluence, whereas the Ne-irradiated surface show /~14 times less etch pit density. The etching rate vH (parallel to cleavage) depends on the chemical composition of the phlogopite. The etching rate vT' (along the track) increases with energy loss.
Programme: 251
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Giret A., Tourpin S., Marc S., Verdier O. & Cottin J.Y. (2002).334, 481–488.
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Rochette P., Sagnotti L., Consolmagno G., Folco L., Maras A., Panzarino F., Pesonen L., Serra R. & Terho M. (2001). A database of magnetic susceptibility of stony meteorites. Quaderni di Geofisica – Quaderni Geofisc, , 30.
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. (2001).27, 83–100.
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