ABSTRAK Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
BAB 1 Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
BAB 2 Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
BAB 3 Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
BAB 4 Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
BAB 5 Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
COVER Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
DAFTAR Ghiffari Ahmadijaya
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
2024 TA PP GHIFFARI AHMADIJAYA 1 - LAMPIRAN.pdf
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
Terbatas  Irwan Sofiyan
» Gedung UPT Perpustakaan
The aerodynamics of an reentry capsule, Orion Crew Module, during its high altitude
reentry from the Earth’s orbit are studied using numerical simulations. The conditions are
similar to those that the Orion Crew Module would face when coming back from space
missions. The simulations are performed for non-reacting rarefied gas flows which cover
the range of hypersonic flow regimes from free molecular to slip flow (Knudsen numbers
from 111 to 0.0263). The simulations are done with Direct Simulation Monte Carlo code
from hyStrath, the open-source OpenFOAM solvers for hypersonic/rarefied gas dynamics
developed by Casseau, et al. The aerodynamics forces and moments are shown to depend
on the degree of incidence angle and rarefaction. The results agree well with DS3V code
results from Moss, et al. with relatively small errors.