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A list of all the posts and pages found on the site. For you robots out there is an XML version available for digesting as well.
Pages
About me
About me
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Posts
Future Blog Post
Published:
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Blog Post number 4
Published:
This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.
Blog Post number 3
Published:
This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.
Blog Post number 2
Published:
This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.
Blog Post number 1
Published:
This is a sample blog post. Lorem ipsum I can’t remember the rest of lorem ipsum and don’t have an internet connection right now. Testing testing testing this blog post. Blog posts are cool.
portfolio
Zoom-in Simulations
The movie is shown in this section.
Morphology of the magnetic fields in the simulated galaxy
The magnetic fields is decomposed into radial, tangential and vertical components.
publications
A sub-grid turbulent dynamo for cosmic magnetism
Published in , 2020
This paper will be available on arXiv by the end of the year.
talks
MHD simulation of galaxy formation with subgrid dynamo
Published:
The magnetic field in galaxies is one of the frontiers of galaxy formation and evolution. We perform a cosmological magnetohydrodynamic (MHD) simulation of galaxy formation with adaptive mesh refinement (AMR) techniques using RAMSES code. In this project, we manage to amplify an initially very weak seed magnetic field to a final value close to equipartition via a simple sub-grid dynamo model. The amplification process features a rapid growth in the magnetic energy, which reaches saturation at the early times of the galaxy evolution. Then the magnetic field follows the fluid distribution. We analyze the magnetic field at redshift z=0 and estimate the magnetic field strength to be a few microG within the galaxy, where turbulent motion dominates. The circumgalactic medium (CGM) is also magnetized by galactic winds driven by supernova explosions and the field strength is estimated there to be a few nG in the CGM.
A Subgrid Turbulent Dynamo for Cosmic Magnetism
Published:
I present a sub-grid turbulent dynamo model in this talk.
A Subgrid Turbulent Dynamo for Cosmic Magnetism (Upcoming)
Published:
I present a sub-grid turbulent dynamo model in this talk.
Building Galxies in Supercomputers (Upcoming)
Published:
This talk aims to give the general pubic an introduction about simulating galaxy formation using advanced supercomputers. This talk will cover basic concepts about galaxy formation, numerical mehods for PDEs and high performance computing tools.
teaching
Teaching experience 1
Undergraduate course, University 1, Department, 2014
This is a description of a teaching experience. You can use markdown like any other post.
Teaching experience 2
Workshop, University 1, Department, 2015
This is a description of a teaching experience. You can use markdown like any other post.