( en | de | ru )

 

Disambiguation of "Yee, H. C."

Author of the publication

copydeleteadd this publication to your clipboard
Entropy Splitting for High Order Numerical Simulation of Vortex Sound at Low Mach Numbers.

, and . J. Sci. Comput., 17 (1-4): 181-190 (2002)

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

C H Johl

Prashanth H C

H C Thejaswini

Charles Woei-Jye Yee

Sun Yee

 

Other publications of authors with the same name

Divergence Free High Order Filter Methods for the Compressible MHD Equations., and . HPSC, page 559-575. Springer, (2003)Construction of low dissipative high-order well-balanced filter schemes for non-equilibrium flows., , , , and . J. Comput. Phys., 230 (11): 4316-4335 (2011)High-order well-balanced schemes and applications to non-equilibrium flow., , , and . J. Comput. Phys., 228 (18): 6682-6702 (2009)Assessment of high-resolution methods for numerical simulations of compressible turbulence with shock waves., , , , , , , , , and 2 other author(s). J. Comput. Phys., 229 (4): 1213-1237 (2010)Efficient Low Dissipative High Order Schemes for Multiscale MHD Flows, II: Minimization of Delta*B Numerical Error., and . J. Sci. Comput., 29 (1): 115-164 (2006)High order finite difference methods with subcell resolution for advection equations with stiff source terms., , , and . J. Comput. Phys., 231 (1): 190-214 (2012)Entropy Splitting for High Order Numerical Simulation of Vortex Sound at Low Mach Numbers., and . J. Sci. Comput., 17 (1-4): 181-190 (2002)Red but not dead : Unveiling the Star-forming Far-infrared Spectral Energy Distribution of SpARCS Brightest Cluster Galaxies at 0 < z < 1.8, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1704.02721Comment: 26 pages, 7 tables, 7 figures.The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z=1, , , , , , , , , and 15 other author(s). (2013)cite arxiv:1305.0882Comment: 15 pages, 6 figures, accepted for publication in MNRAS. Reduced data will be made available through the ESO archive.Computer tools to teach channel models for optical links., , and . CONIELECOMP, page 68-72. IEEE, (2010)