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Autor:
Cordier, D., Cornet, T., Barnes, J. W., MacKenzie, S. M., Bahers, T. Le, Nna-Mvondo, D., Rannou, P., Ferreira, A. G.
Numerous geological features that could be evaporitic in origin have been identified on the surface of Titan. Although they seem to be water-ice poor, their main properties -chemical composition, thickness, stratification- are essentially unknown. In
Externí odkaz:
http://arxiv.org/abs/1512.07294
Autor:
Bachellier, N.1, Ormaza, M.1, Faraggi, M.2, Verlhac, B.1, Vérot, M.3, Bahers, T. Le3, Bocquet, M.-L.2, Limot, L.1 limot@ipcms.unistra.fr
Publikováno v:
Physical Review B. May2016, Vol. 93 Issue 19, p1-1. 1p.