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ChunLin Tian
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  Dr. Chunlin TIAN
  Vistiting Research Scientist
(2013.9-2014.9)
  Address: School of Space Science and Physics, Shandong University, Weihai, Shandong, China, 264209
  Email: chunlin.tian2012@gmail.com






Research Interests

Practical High Performance Computation: the practical ways to parallelize MHD code with OpenMP, MPI and CUDA

Computational Fluid Dynamics: gas-kinetic BGK scheme, MHD schemes

Stellar and Solar Physics: turbulent magnetoconveciton related problems, such as overshooting, differential rotation, Sunspot,dynamo; CME related problems.

 

Education

Ph.D. Astrophysics, Graduate University of Chinese Academy of Sciences, 7/2008

M.Phil. Applied Mathematics, Hong Kong University of Science and Technology, 7/2005

B.S. Physics, Lanzhou University, 6/2002

 

Employment History

Postdoc: Magneto-convection inside the Sun, ELTE, Budapest, 12/2008-11/2010

Visitor: Coronal Mass Ejection, Huairou Solar Observing Station, NAOC, Beijing, 12/2010-7/2011

Postdoc: Active Sun, Department of Physics, University of Helsinki, Helsinki, 8/2011-7/2013

Visitor: MHD numerical simulation of Coronal Physics, Shandong University at Weihai, Weihai, 9/2013-

 

Teaching Experience

Co-Lecturer, Magetohydrodynamics, Department of Physics, UH, 2012

Co-Lecturer, Practical Methods In Numerical MHD, Department of Physics, UH, 2011

Teaching Assistant, Ordinary Differential Equation, Department of Mathematics, HKUST, 2005

Teaching Assistant, Partial Differential Equation, Department of Mathematics, HKUST, 2004

Teaching Assistant, Numerical Analysis, Department of Mathematics, HKUST, 2004

 

Publications

1. A three-dimensional multidimensional gas-kinetic scheme for the Navier-Stokes equations under gravitational felds. C.L. Tian, K. Xu,

    K. L. Chan and L. Deng, J. Comput. Phys., 226 (2007), pp. 2003-2027. [ADS]

 

2. Efficient turbulent compressible convection in the deep stellar atmosphere.  Chun-Lin Tian, Li-Cai Deng, Kwing-Lam Chan and Da-Run Xiong,

    RAA, 9 (2009), pp. 102-114.

 

3. Numerical simulations of downward overshooting in the Giants. Chun-Lin Tian, Li-Cai Deng and Kwing-Lam Chan,  MNRAS, 398 (2009), pp. 1011-1022.

 

4. An extension of gas-kinetic BGK Navier-Stokes scheme to multidimensional astrophysical magnetohydrodynamicsChunlin Tian, arXiv:1010.3594, 2010.

 

5. Structures in compressible magnetoconvection and the nature of umbral dots. Chunlin Tian and Kristóf Petrovay, AA, 551(2013), A92

 

6. Rotating convection in f-boxes: morphology of flow and topology of magnetic field. Chunlin Tian,Petri J. K¨apyl¨a, and Maarit J. Mantere (in preparation)

 


 
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