Martha Evonuk, Ph.D.
Affiliations: | 2006 | University of California, Santa Cruz, Santa Cruz, CA, United States |
Area:
Astronomy and Astrophysics, GeophysicsGoogle:
"Martha Evonuk"Mean distance: (not calculated yet)
Parents
Sign in to add mentor| Gary A. Glatzmaier | grad student | 2006 | UC Santa Cruz | |
| (Numerical modeling of convection in the interiors of giant planets.) | ||||
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Publications
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| Evonuk M. (2015) Convection in deformed bodies: The effect of equatorial ellipticity on convective behavior Earth and Planetary Science Letters. 430: 249-259 |
| Evonuk M, Samuel H. (2012) Simulating rotating fluid bodies: When is vorticity generation via density-stratification important? Earth and Planetary Science Letters. 317: 1-7 |
| Glatzmaier GA, Evonuk M, Rogers TM. (2009) Differential rotation in giant planets maintained by density-stratified turbulent convection Geophysical and Astrophysical Fluid Dynamics. 103: 31-51 |
| Evonuk M. (2008) The role of density stratification in generating zonal flow structures in a rotating fluid Astrophysical Journal. 673: 1154-1159 |
| Evonuk M, Glatzmaier GA. (2007) The effects of rotation rate on deep convection in giant planets with small solid cores Planetary and Space Science. 55: 407-412 |
| Evonuk M, Glatzmaier GA. (2006) Heat transport in 3D anelastic simulations of the internal dynamics of giant planets without cores Proceedings of the International Astronomical Union. 2: 221-223 |
| Evonuk M, Glatzmaier GA. (2006) Modeling convection and zonal winds in giant planets Proceedings of the International Astronomical Union. 2: 177-187 |
| Evonuk M, Glatzmaier GA. (2006) A 2D study of the effects of the size of a solid core on the equatorial flow in giant planets Icarus. 181: 458-464 |
| Evonuk M, Glatzmaier GA. (2004) 2D studies of various approximations used for modeling convection in giant planets Geophysical and Astrophysical Fluid Dynamics. 98: 241-255 |