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"NASA Technical Reports Server (NTRS) 19980017417: Numerical Modeling Of Solidification In Space With MEPHISTO-4. Part 2" and the language of the book is English.


“NASA Technical Reports Server (NTRS) 19980017417: Numerical Modeling Of Solidification In Space With MEPHISTO-4. Part 2” Metadata:

  • Title: ➤  NASA Technical Reports Server (NTRS) 19980017417: Numerical Modeling Of Solidification In Space With MEPHISTO-4. Part 2
  • Author: ➤  
  • Language: English

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  • Internet Archive ID: NASA_NTRS_Archive_19980017417

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"NASA Technical Reports Server (NTRS) 19980017417: Numerical Modeling Of Solidification In Space With MEPHISTO-4. Part 2" Description:

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A pre-flight analysis of the directional solidification of BiSn with MEPHISTO-4 is presented. Simplified Bridgman growth under microgravity conditions is simulated using a two dimensional finite element model. This numerical model is a single domain, pseudo-steady state model, and includes the effects of both thermal and solutal convection. The results show that for all orientations of the applied steady state gravity vector, of magnitude 1 micro-g, the directional solidification process remains diffusion controlled. The maximum convective velocity was found to be 4.424 x 10(exp -5) cm/s for the horizontal Bridgman growth configuration. This value is an order of magnitude lower than the growth velocity. The maximum and minimum values or solute concentration in the liquid at the crystal-melt interface were 13.867 at.% and 13.722 at.%, respectively. This gives a radial segregation value of xi = 1.046% at the interface. A secondary objective of this work was to compare the results obtained to those that consider thermal convection only (no solutal convection). It was found that the convective flow patterns in simulations which included solutal convection were significantly different from those which ignored solutal convection. The level of radial segregation predicted by the current simulations is an order of magnitude lower than that found in simulations which ignore solutal convection. The final aim was to investigate the effect of g-jitter on the crystal growth process. A simulation was performed to calculate the system response to a 1 second, 100 micro-g gravity impulse acting normal to the direction of growth. This pulse is consistent with that induced by Orbiter thruster firings. The results obtained indicate that such a gravity pulse causes an increase in the level of radial solute segregation at the interface from the steady state values. The maximum value of solute concentration in the liquid was found to be 13.888 at.%, the minimum value calculated was 13.706 at.%, yielding a radial segregation value of xi = 1.31% at the interface. These values occurred 126 seconds after the pulse terminated. Thus it is anticipated that the process will remain diffusion controlled even when subjected to such g-jitter.

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