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ALEGRA: Finite element modeling for shock hydrodynamics and multiphysics

International Journal of Impact Engineering

Niederhaus, John H.; Bova, S.W.; Carleton, James B.; Carpenter, John H.; Cochrane, Kyle C.; Crockatt, Michael M.; Dong, Wen D.; Fuller, Timothy J.; Granzow, Brian N.; Ibanez-Granados, Daniel A.; Kennon, Stephen; Luchini, Christopher B.; Moral, Ramon; O'Brien, Christopher J.; Powell, Michael P.; Robinson, Allen C.; Rodriguez, Angel E.; Sanchez, Jason J.; Scott, Walter A.; Siefert, Christopher S.; Stagg, Alan K.; Kalashnikova, Irina; Voth, Thomas E.; Wilkes, John

ALEGRA is a multiphysics finite-element shock hydrodynamics code, under development at Sandia National Laboratories since 1990. Fully coupled multiphysics capabilities include transient magnetics, magnetohydrodynamics, electromechanics, and radiation transport. Importantly, ALEGRA is used to study hypervelocity impact, pulsed power devices, and radiation effects. The breadth of physics represented in ALEGRA is outlined here, along with simulated results for a selected hypervelocity impact experiment.

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Modeling a ring magnet in ALEGRA

Niederhaus, John H.; Pacheco, Jose L.; Wilkes, John; Hooper, Russell H.; Siefert, Christopher S.; Goeke, Ronald S.

We show here that Sandia's ALEGRA software can be used to model a permanent magnet in 2D and 3D, with accuracy matching that of the open-source commercial software FEMM. This is done by conducting simulations and experimental measurements for a commercial-grade N42 neodymium alloy ring magnet with a measured magnetic field strength of approximately 0.4 T in its immediate vicinity. Transient simulations using ALEGRA and static simulations using FEMM are conducted. Comparisons are made between simulations and measurements, and amongst the simulations, for sample locations in the steady-state magnetic field. The comparisons show that all models capture the data to within 7%. The FEMM and ALEGRA results agree to within approximately 2%. The most accurate solutions in ALEGRA are obtained using quadrilateral or hexahedral elements. In the case where iron shielding disks are included in the magnetized space, ALEGRA simulations are considerably more expensive because of the increased magnetic diffusion time, but FEMM and ALEGRA results are still in agreement. The magnetic field data are portable to other software interfaces using the Exodus file format.

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Nuclear Risk Assessment 2019 Update for the Mars 2020 Mission Environmental Impact Statement

Clayton, Daniel J.; Wilkes, John; Starr, Michael J.; Ehrhart, Brian D.; Mendoza, Hector M.; Ricks, Allen J.; Villa, Daniel V.; Potter, Donald L.; Dinzl, Derek J.; Fulton, John F.; Laros, James H.; Cochran, Lainy D.; Brooks, Dusty M.

In the summer of 2020, the National Aeronautics and Space Administration (NASA) plans to launch a spacecraft as part of the Mars 2020 mission. The rover on the proposed spacecraft will use a Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) to provide continuous electrical and thermal power for the mission. The MMRTG uses radioactive plutonium dioxide. NASA is preparing a Supplemental Environmental Impact Statement (SEIS) for the mission in accordance with the National Environmental Policy Act. This Nuclear Risk Assessment addresses the responses of the MMRTG option to potential accident and abort conditions during the launch opportunity for the Mars 2020 mission and the associated consequences. This information provides the technical basis for the radiological risks discussed in the SEIS.

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5 Results
5 Results