NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Experiences with explicit finite-difference schemes for complex fluid dynamics problems on STAR-100 and CYBER-203 computersSeveral two- and three-dimensional external and internal flow problems solved on the STAR-100 and CYBER-203 vector processing computers are described. The flow field was described by the full Navier-Stokes equations which were then solved by explicit finite-difference algorithms. Problem results and computer system requirements are presented. Program organization and data base structure for three-dimensional computer codes which will eliminate or improve on page faulting, are discussed. Storage requirements for three-dimensional codes are reduced by calculating transformation metric data in each step. As a result, in-core grid points were increased in number by 50% to 150,000, with a 10% execution time increase. An assessment of current and future machine requirements shows that even on the CYBER-205 computer only a few problems can be solved realistically. Estimates reveal that the present situation is more storage limited than compute rate limited, but advancements in both storage and speed are essential to realistically calculate three-dimensional flow.
Document ID
19820059716
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kumar, A.
(NASA Langley Research Center Hampton, VA, United States)
Rudy, D. H.
(NASA Langley Research Center Hampton, VA, United States)
Drummond, J. P.
(NASA Langley Research Center Hampton, VA, United States)
Harris, J. E.
(NASA Langley Research Center Hampton, VA, United States)
Date Acquired
August 10, 2013
Publication Date
August 1, 1982
Subject Category
Fluid Mechanics And Heat Transfer
Accession Number
82A43251
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available