TY - GEN
T1 - Damage of 5A06 whipple shield caused by hypervelocity impact of AL 2017 sphere
AU - Lin, Musen
AU - Pang, Baojun
AU - Zhang, Wei
PY - 2009
Y1 - 2009
N2 - All long duration spacecraft in low-earth-orbit are subject to high speed impacts by meteoroids and space debris. Especially the menace by those particles which can not be observed should be put more importance. In order to get the damage mode and resist character of spacecraft shield structure by the high-velocity impact of space debris, numerical simulations of Al 2017 sphere projectiles impacting on 5A06 aluminum alloy Whipple shield at normal angle were carried out using the smoothed particle hydrodynamics (SPH) technique of AUTODYN hydro-codes. Compared with the high-velocity impact experiment in impact velocity (2 ∼5.2 km/s), projectile diameter (4 mm, 6.35 mm) and bumper thickness (0.5 mm, 1.5 mm, 2 mm and 3 mm), the laws of penetration hole of bumper and damage of bulkhead were obtained. By analyzing the shapes and velocities characteristics of debris clouds in contrast with X photographs, the explanations for damage of bulkhead from the view of debris clouds were purposed. It is shown that the results of numerical simulations are in agreement with those of experiment. Furthermore, the high-velocity impact numerical simulations that velocities are up to 10 km/s were investigated.
AB - All long duration spacecraft in low-earth-orbit are subject to high speed impacts by meteoroids and space debris. Especially the menace by those particles which can not be observed should be put more importance. In order to get the damage mode and resist character of spacecraft shield structure by the high-velocity impact of space debris, numerical simulations of Al 2017 sphere projectiles impacting on 5A06 aluminum alloy Whipple shield at normal angle were carried out using the smoothed particle hydrodynamics (SPH) technique of AUTODYN hydro-codes. Compared with the high-velocity impact experiment in impact velocity (2 ∼5.2 km/s), projectile diameter (4 mm, 6.35 mm) and bumper thickness (0.5 mm, 1.5 mm, 2 mm and 3 mm), the laws of penetration hole of bumper and damage of bulkhead were obtained. By analyzing the shapes and velocities characteristics of debris clouds in contrast with X photographs, the explanations for damage of bulkhead from the view of debris clouds were purposed. It is shown that the results of numerical simulations are in agreement with those of experiment. Furthermore, the high-velocity impact numerical simulations that velocities are up to 10 km/s were investigated.
KW - Damage mode
KW - High-velocity impact
KW - Numerical simulation
KW - Space debris
KW - Whipple shield
UR - https://www.scopus.com/pages/publications/77953523677
M3 - 会议稿件
AN - SCOPUS:77953523677
SN - 9781615679089
T3 - 60th International Astronautical Congress 2009, IAC 2009
SP - 1880
EP - 1888
BT - 60th International Astronautical Congress 2009, IAC 2009
T2 - 60th International Astronautical Congress 2009, IAC 2009
Y2 - 12 October 2009 through 16 October 2009
ER -