Monitoring by Raman Spectroscopy of CO2 Clathrate Formation from Electrolyte Solutions. The Performance to Icy Satellites

Details Monitoring by Raman Spectroscopy of CO2 Clathrate Formation from Electrolyte Solutions. The Performance to Icy Satellites Monitoring by Raman Spectroscopy of CO2 Clathrate Formation from Electrolyte Solutions. The Performance to Icy Satellites

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..914m&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.914

Computer Science

Scientific paper

In the present work, we crystallize and dissociate CO2 clathrates from
an aqueous solution of MgSO4 and CO2. We assume that the aqueous magmas
from the Europa interior are salt-rich. This assumption is based on the
NIR Galileo observations of dark terrains, wich seems to be endogenous
and composed by salt hydrates[1].

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