Time Adaptation for 3-D Unsteady Flow around Moving Bodies

Mapping Intimacies ◽

10.2514/6.2022-2023 ◽

2022 ◽

Author(s):

Taeyoon Kung ◽

Jae Sang Rhee ◽

Junseok Oh ◽

Jinyoung Huh ◽

Kyu Hong Kim

Keyword(s):

Unsteady Flow ◽

Moving Bodies

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THE NUMERICAL SIMULATION OF STRONGLY UNSTEADY FLOW WITH HUNDREDS OF MOVING BODIES

Computational Fluid Dynamics Review 1998 ◽

10.1142/9789812812957_0056 ◽

1998 ◽

pp. 1027-1033

Author(s):

Rainald LÖHNER ◽

Joseph D. BAUM ◽

Chi YANG ◽

Hong LUO

Keyword(s):

Numerical Simulation ◽

Unsteady Flow ◽

Moving Bodies

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The numerical simulation of strongly unsteady flow with hundreds of moving bodies

International Journal for Numerical Methods in Fluids ◽

10.1002/(sici)1097-0363(19990915)31:1<113::aid-fld958>3.0.co;2-q ◽

1999 ◽

Vol 31 (1) ◽

pp. 113-120 ◽

Cited By ~ 28

Author(s):

Rainald Löhner ◽

Chi Yang ◽

Joseph D. Baum ◽

Hong Luo ◽

Daniele Pelessone ◽

...

Keyword(s):

Numerical Simulation ◽

Unsteady Flow ◽

Moving Bodies

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Dynamics of comets in the collapsing protosolar nebula

International Astronomical Union Colloquium ◽

10.1017/s0252921100031225 ◽

1999 ◽

Vol 173 ◽

pp. 45-50

Author(s):

L. Neslušan

Keyword(s):

Solar System ◽

Velocity Distribution ◽

Oort Cloud ◽

Interstellar Clouds ◽

Protosolar Nebula ◽

Moving Bodies

AbstractComets are created in the cool, dense regions of interstellar clouds. These macroscopic bodies take place in the collapse of protostar cloud as mechanically moving bodies in contrast to the gas and miscroscopic dust holding the laws of hydrodynamics. In the presented contribution, there is given an evidence concerning the Solar system comets: if the velocity distribution of comets before the collapse was similar to that in the Oort cloud at the present, then the comets remained at large cloud-centric distances. Hence, the comets in the solar Oort cloud represent a relict of the nebular stage of the Solar system.

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