Descripción
|
|
---|---|
Ice-doping processes are of great interest in fields such as atmospheric chemistry, astrophysics and geophysics. In recent years, various studies revealed the existence of subsurface salty oceans and the presence of high-pressure ice polymorphs in the interior of some planetary bodies such as Jupiters satellites or exoplanets such as Proxima b [1, 2]. These ices, stable over several gigapascals and hundreds of Kelvin, can contain a significant amount of small ions in their structure. The presence of doped ice suggests a plausible explanation for the behaviour and different physical properties observed in the interior of these icy bodies. | |
Internacional
|
No |
Nombre congreso
|
FISES 2018 |
Tipo de participación
|
970 |
Lugar del congreso
|
Madrid |
Revisores
|
Si |
ISBN o ISSN
|
|
DOI
|
|
Fecha inicio congreso
|
18/10/2018 |
Fecha fin congreso
|
20/10/2018 |
Desde la página
|
|
Hasta la página
|
|
Título de las actas
|