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Title: Professor Degrees:
Research Interests:
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Middle atmosphere dynamics with gravity wave interactions in the numerical spectral model: Tides and planetary waves (Mayr et al. 2011, J. Atmos. Sol.-Terr. Phys., 73: 711-730).
Middle atmosphere dynamics with gravity wave interactions in the numerical spectral model: Zonal-mean variations (Mayr et al. 2010, J. Atmos. Sol.-Terr. Phys., 72: 807-828).
Lunar regolith thermal behavior revealed by Chang'E-1 microwave brightness temperature data (Chan et al. 2010, Earth & Planet. Sci. Lett. 295: 287-291)
Numerical simulations of downward convective overshooting in giants (Tian et al. 2009, MNRAS, 39: 1011-1022).
Mapping the moon with Chang'E-1 microwave brightness temperature data (Tsang et al. 2009, in 『绕月探测工程探测数据应用研究进展论文集』，「中国科学院探月工程总体部」汇编，240-244).
Efficient turbulent compressible convection in the deep stellar atmosphere (Tian et al. 2009, Research in Astron. Astrophys., 9: 102-114)
A shallow convective model for Jupiters alternating wind bands (Chan & Mayr 2008, JGR-Planets, Vol. 113, E10002, doi:10.1029/2008JE003124)
Proxies for overshooting above a convection zone (Chan & Singh 2008, in Proceedings IAU Symposium 252: The Art of Modeling Stars in the 21st Century, eds L. Deng and K.L. Chan)
Rotating convection in f-boxes: Faster rotation (Chan 2007, Astron. Nach., 10: 1059-1061)
A three-dimensional multidimensional gas-kinetic scheme for the Navier-Stokes equations under gravitational fields (Tian et al. 2007, Journal of Computational Physics, 226: 2003-2027)
Turbulent compressible convection with rotation-penetration below a convection zone (Pal et al. 2007, Astrophysics and Space Science, 307: 399-407)
Modeling of transport of metals with rate-limited EDTA-promoted extraction and dissolution during EDTA-flushing of copper-contaminated soils (Tsang et al. 2007, Environ. Sci. Tech., 41: 3660-3666)
A finite-difference convective model for Jupiter's equatorial jet (Chan 2006, in Convection in Astrophysics, IAU Symposium No. 239, p.230-232)
An anisotropic nonlocal convection theory (Deng et al. 2006, ApJ, 643:426-437)
Mesospheric non-migrating tides generated with planetary waves. I. Characteristics (Mayr et al. 2005, J. Atmos. Sol.-Terr. Phys., 67: 959-980)
Mesospheric non-migrating tides generated with planetary waves. II. Influence of gravity waves (Mayr et al. 2005, J. Atmos. Sol.-Terr. Phys., 67: 981-991)
Flow patterns and transitions in rotating convection (Chan 2005, in Proceedings of Workshop on Interdisciplinary Aspects of Turbulence, Tegernsee, Germany, p. 159-160)
Properties of internal planetary-scale inertial gravity waves in the mesosphere (Mayr et al. 2004, Annales Geophysicae, 22: 1-15)
Modeling studies with QBO: II. Solar cycle effect (Mayr et al. 2003, J. Atmos. Sol.-Terr. Phys., 65: 901)
Turbulence in rotating convection (Chan 2003, in Proceedings of NATO Advanced Research Workshop: Turbulence, Waves and Instabilities in the Solar Plasma, Publ. Aston. Dept. of Eotvos U., 13: 49)
Numercial study of rotating convection (Chan 2003, in Proceedings of the 3D Stellar Evolution Conference, Livermore, ASP Conf. Series, 293: 168) original file (better figures)
The 'stratified' approximation for computing geophysical flows (Chan 1996, Southeast Asia Bull. Math., 20: 65)
Rotating convection and solar differential rotation (Chan 1994, Solar Phys., 152: 238)
A spectral approach for studying middle and upper atmospheric phenomena (Chan et al. 1994, J. Atmos. Terr. Phys., 56: 1399)
A 'stratified' spectral model for stable and convective atmospheres (Chan et al. 1994, J. Comput. Phys., 113: 165)
Recent development in solar convection theory (Chan et al. 1991, in Solar Interior and Atmosphere, eds. A.N. Cox, W.C. Livingston, M.S. Matthews, U. Arizona Press, Tucson, p.223-274)
