Surface blistering of metals due to low energy hydrogen bombardment.
Surface blistering of metals due to low energy hydrogen ion bombardment, determining solar absorptance change in gold-plated specimens
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Surface blistering of metals due to low energy hydrogen ion bombardment, determining solar absorptance change in gold-plated specimens
Surface blistering of metals due to low energy hydrogen ion bombardment, determining solar absorptance change in gold-plated specimens
The State-of-the-Art (SOA) air revitalization architecture onboard the International Space Station (ISS) recovered approximately 50% of the oxygen (O 2 ) from metabolic carbon dioxide (CO 2 ) via the Sabatier process from 2011 to 2017. O 2 recovery is currently constrained by the limited availability of reactant hydrogen (H 2 ) preventing complete conversion of CO 2 to H 2 O. Increasing O 2 recovery within Closed-Loop ECLSS is essential to reducing resupply mass for long-duration manned missions; specifically focusing on water (H 2 O) which supplies H 2 for Sabatier via water electrolysis. Past ground test endeavors at Marshall Space Flight Center (MSFC) have attempted to recover H 2 from Sabatier-produced CH 4 using technologies such as carbon vapor deposition (CVD) and plasma pyrolysis. The byproducts of these technologies can act as a catalyst poison or reactor deadload to the Sabatier reactor. Hydrogen separation techniques must be utilized to maintain the Sabatier catalyst during gas recycling and must be scalable, non-energy intensive, and safe to operate in a habitation setting. Research indicated that metal-organic frameworks (MOFs) could meet these criteria and were tested for their capability to capture the various carbon-based gaseous products of CVD and plasma pyrolysis such as acetylene (C 2 H 2 ), ethylene (C 2 H 4 ), ethane (C 2 H 6 ), and carbon monoxide (CO) which would purify the hydrogen gas stream passing through the MOF. A sub-scale adsorption column was developed by Marshall Space Flight Center to test three MOF candidates against a synthetic gas mixture comprised of process-relevant carbonous gases and hydrogen to evaluate the separation capability of the MOFs. The results of the hydrogen separation capability, isothermal desorption capability, and demonstrated cyclic reuse of the MOF are presented in this paper.
Deuterons and tritons determined for top of earth atmosphere, using grain density vs residual range in nuclear emulsion stack
Energy required for proton and molecular hydrogen ion production by electron impact in tenuous hydrogen plasma using Maxwellian electron gas model
Energy requirements for proton production by electron impact of hydrogen plasma
Potential energy curves for the X(sup 1)sigma+ and V(sup 1)sigma+ states of HF and DF have been calculated by the Rydberg-Klein-Rees method. The results calculated from the different sets of data for HF and DF are found to be in very good agreement. The theoretical results of Karo are compared to the experimental results obtained here.
Energy transfer from hydrogen air flames - measurement of heat flux near reaction zone using conductivity type heat flow meter
Hyperfine splitting of spin interaction energy of two hydrogen atoms, determining eigenfunctions for effective Hamiltonian
Energy loss, contraction and collapse of molecular hydrogen protostars tracing evolutionary processes
Positron s-wave elastic scattering by atomic hydrogen below inelastic threshold analyzed, using Dalgarno-Lynn second order adiabatic potential
Addition of electromagnetic wave energy to atomic hydrogen plasma at off-resonant conditions
Energy of interaction between two hydrogen atoms in their ground states described by Gauss-type functions
Steady state composition of low density nonequilibrium hydrogen plasma
Interaction of two H atoms in ground states using Hirschfelder-Linnet wave function and Gaussian type function
Electromagnetic radiation due to cosmic ray energy dissipation in interstellar hydrogen
Differential energy flux neutron spectra in liquid hydrogen obtained by time-of-flight techniques
Interaction energy levels and transport coefficients of lithium-hydrogen and oxygen- hydrogen gas mixtures at high temperatures