𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The analysis of water in the Martian regolith

✍ Scribed by D. M. Anderson; A. R. Tice

Publisher
Springer
Year
1979
Tongue
English
Weight
357 KB
Volume
14
Category
Article
ISSN
0022-2844

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Modeling diffusion advection in the mass
Modeling diffusion advection in the mass transfer of water vapor through martian regolith
✍ Richard Ulrich πŸ“‚ Article πŸ“… 2009 πŸ› Elsevier Science 🌐 English βš– 312 KB

Diffusion advection is an effect in diffusive multicomponent mass transfer that occurs when the flux vectors of the individual components do not add up to zero. This can be a significant effect for the mass transfer of water vapor from subsurface ice or liquid reservoirs through porous regolith at m

Neutron Capture Isotopes in the Martian
Neutron Capture Isotopes in the Martian Regolith and Implications for Martian Atmospheric Noble Gases
✍ M.N. Rao; D.D. Bogard; L.E. Nyquist; D.S. McKay; J. Masarik πŸ“‚ Article πŸ“… 2002 πŸ› Elsevier Science 🌐 English βš– 258 KB

Impact-produced glasses in some martian meteorites have trapped significant amounts of the recent martian atmosphere. From literature data, we estimate that ∼9% of the trapped 80 Kr in these meteorites was produced from neutron capture on 79 Br. Estimates of neutron fluences made from 80 Kr and 149

Modelling of the dose-rate variations wi
Modelling of the dose-rate variations with depth in the Martian regolith using GEANT4
✍ P. Morthekai; M. Jain; L. Dartnell; A.S. Murray; L. BΓΈtter-Jensen; L. Desorgher πŸ“‚ Article πŸ“… 2007 πŸ› Elsevier Science 🌐 English βš– 159 KB

The environmental radiation field at the Martian surface consists mainly of Galactic Cosmic Rays (GCR) and charged particles ejected during the Solar Particle Events (SPE). Interactions between these radiation fluxes and the regolith result in a complex radiation field that varies both as a function