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I am always on the look-out for an ambitious new graduate student.
• Check out my Research slide below for my research interests. • Here are a few ideas for thesis topics and the whereabouts of my former students. • Interested? You can apply to our graduate programme here.
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Density greyscale of an axisymmetric simulation (top half only shown) of a propagating jet (M=10, η=0.1) from left to right with: (top) passive magnetic field; (middle) strong toroidal field (β=0.2); and (bottom) strong poloidal field (β=0.2) all after the same propagation time. In 2-D, a toroidal field enhances propagation speed, a poloidal field impedes it.
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The maiden AZEuS simulation showing the Alfvénic Mach number (colours) and magnetic field lines of a protostellar jet with eight levels of refinement. This is the first simulation to follow a magnetocentrifugally launched jet (at resolution 0.00625 AU) to observational scales (2,000 AU) where the jet takes on its familiar bow-shock led morphology. See Ramsey & Clarke for details.
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Line-of-sight integration of the pseudo-synchrotron emission of two ZEUS-3D simulations of supersonic (M=10), light (η=0.1) jets with: (top) a trace magnetic field; and (bottom) a strong (β=0.2) toroidal magnetic field. Jet propagation is from left to right.
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Line-of-sight integration of ∇ · v in a jet launched magnetocentrifugally from the left face (red ring with orange centre). The jet propagates from left to right and follows a helical path as it succumbs to higher-order modes of the Kelvin-Helmholtz instability. Details in Ouyed, Clarke, & Pudritz.
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Line-of-sight integration of the magnetic energy density in a supersonic (M=10), super-Alfvénic turbulent medium using the Consistent Method of Characteristics (CMoC) in dzeus36 on a 2563 grid.
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I believe one gets what one works for, and those who work hard in my class will learn a lot. Read more about what you can expect from me as a professor here.
Download an 8.5" × 11" or a 3' × 4' version of my poster.
Below are listed most of the courses I have taught at SMU since 1993; only those I am currently teaching are "live". Selected resources from "dormant" courses (e.g., my primers for PHYS 3210) are available from my "document bar".
| ASTR 5700 | Magnetohydrodynamics |
PHYS 2301 | Analytical Mechanics |
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| PHYS 1100 | University Physics I |
PHYS 3200 | Mathematical Methods in Physics I |
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| PHYS 1101 | University Physics II |
PHYS 3210 | Computational Methods in Physics |
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| PHYS 2200* | Introduction to Mathematical Physics |
PHYS 3500 | Quantum Mechanics I |
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| PHYS 2300 | Vibrations, Waves, and Optics |
PHYS 4380 | Fluid Dynamics |
*Course no longer part of the curriculum.
In 2007, the department curriculum was revised and fully documented. Expectations and outcomes for each course were defined, described, and placed on the web for faculty and student reference. I encourage students to review the course curriculum of each course they take, and to hold their professors accountable to its content.
I am the developer and curator of the widely used magnetohydrodynamics (MHD) computer code, ZEUS-3D. With it, I and my students perform multi-dimensional simulations of fluid phenomena such as astrophysical jets.
You can read more about my research interests here, consider graduate student projects here, and see a partial list of my publications here.
ZEUS-3D website for gallery, description, user/installation guides, and downloading the code (version 3.5). |
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AZEuS (AMR+ZEUS-3D) website for gallery and description. The code is not yet ready for distribution. |
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EDITOR is my source-code manager for ZEUS-3D and AZEuS. Version 2.2 and user manual available for download. |
I am pleased to say that every student who finished their degree with me moved on successfully to the next logical stage of their academic career.
Early in my career, I dabbled in radio astronomy using the VLA to observe radio galaxies such as 3C 219 (above left; image courtesy Alan Bridle, NRAO). You might imagine my surprise when, about ten years later, I happened upon our data immortalised in tile on the Hayden Planetarium floor (insert; image courtesy of Jodi)!
Links to the programmes (PDF files) for the department's annual summer student mini-symposium, which I've organised since 2009.
| 2009 | 2010 | 2011 | 2012 |
Science Curriculum Cmte., department rep. | A&P Curriculum Cmte., chair |
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Science Space Cmte., department rep. | University Copyright Cmte., faculty rep. (2011-) |
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Academic Appeals Board, faculty rep. (2006-) | University Budget Cmte., faculty rep. (2002-05) |
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Sexual Harassment Cmte., faculty rep. (1997-2000) | Graduate Awards Cmte., department rep. (1997-98) |
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Academic Standing Cmte., faculty rep. (1995-98) | Academic Computer User's Cmte., faculty rep. (1993-94) |
ACEnet SMU Local user's group, chair (2008-09) | ACEnet Research Directorate, founding member |
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CASCA Theory and Computation Cmte. (1998-2004) | (2002-06) |
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CFI RDF Selection Cmte. (1998-2000) | CITA Council (1998-2000) |
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NRAO review panel (1993-95) |
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Links to the PDFs of primers and manuals I have written or contributed to are given below. For documents authored solely by me, permission is granted to use and distribute freely for non-profit and academic purposes only, provided the original authorship and affiliation are retained. Those wanting any of the LATEX files should contact me directly.
Did someone say bar?
| A primer on Tensor Calculus | Something I prepared for my own edification. |
| FORTRAN77 primer | A quick start-up guide for first-time programmers in FORTRAN. |
| Unix primer | Exceedingly basic introduction to unix for first-time users. |
| DBX primer | Beginner's guide to debugging with Sun's DBX. |
| LATEX primer | An augmented version of David Wilkins' excellent primer. |
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| dzeus34 user manual | User manual for ZEUS-3D, version 3.4. |
| dzeus35 user manual | User manual for ZEUS-3D, version 3.5. |
| dzeus36 user manual | User manual for ZEUS-3D, version 3.6. |
| edit21 user manual | User manual for EDITOR, version 2.1. |
| edit22 user manual | User manual for EDITOR, version 2.2. |
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Lab manual and answer guide for a two-semester first year calculus-based physics course (e.g., HRW), no longer in use at SMU for reasons too tedious to explain. If anyone else can use them, I can provide the LATEX files and figures. |
Coming at some point, a table of possibly useful coding snippets...
Despite my background in algorithm development and supercomputer simulations, I remain a bit of a ludite. I'm not a blogger, I don't do Facebook, and I most certainly don't tweet. I don't even own a cell phone! This web-page, such as it is, represents my first and likely only foray into "social media".
Born in Charlottetown, Prince Edward Island to Sheila (née Davison; Charlottetown) and Alan Clarke (Halifax) in 1958, I was raised in Ontario and did my B.Sc. at Queen's University at Kingston (Honours Physics, 1981). My M.Sc. (Thesis: "Two-Dimensional Collapse of a Rotating Interstellar Cloud", 1984) was also from Queen's under Dick Henriksen. My Ph.D. (Dissertation: "A Search for the Effects of Active Magnetic Fields in Extragalactic Radio Sources", 1988) was from the University of New Mexico under Jack Burns and Mike Norman (LANL, NCSA).
I was a post-doctoral fellow at the NCSA (U. Illinois) from 1988–1992 under Mike Norman, and a post-doctoral research associate at the Harvard-Smithsonian CfA from 1992–1993 under Ramesh Narayan.
In 1993, I was appointed an assistant professor at Saint Mary's University, promoted to associate professor in 1995, gained tenure in 1996, and promoted again to full professor in 2003. During my 2000–2001 sabbatical leave, I was appointed astronome invité at l'observatoire de Grenoble. You can view my CV here.
I went to the U.S. in 1984 single, came home in 1993 with a family. My wife now of 25 years, Jodi Asbell-Clarke, hails from North Haven, CT and is currently a senior science curriculum developer at a non-profit in Cambridge MA. My son, Dane, born in Albuquerque NM in 1989, is a graphic artist (check out his webpage!) in a small but growing firm in Halifax. My daughter, Alison, born in Urbana IL in 1992, is an undergraduate in political science at the University of Guelph.
I have one brother (Peter) who works and lives in Toronto. My mother lives in Halifax and my father and his wife Adaline live in Victoria.
I offer here a few snippets of "pre-historic" comedy, all from well before most of our students were born! They're timeless, they're clean, and they're fun; enjoy!
Many from my generation remember the Carol Burnett Show as a one-of-a-kind. In the few years SNL has been great, it has occasionally come close. A few of my favourite sketches include... |
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And speaking of SNL, here are a few of my favourite characters. The only one from the "modern era" (Wiig's Gifford) doesn't seem to be on You-Tube yet. |
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One of my Dad's all-time favourites was Victor Borge. His "phonetic punctuation" sketch is a classic. |
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All the world's daft, save thee and me. And lately I've been wondering about thee.
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My grandmother's paraphrasing of Robert Owen's utterance in 1828 on severing business relations with his partner William Allen: All the world is queer save thee and me, and even thou art a little queer. |
If, in the last few years, you haven't discarded a major opinion or acquired a new one, check your pulse. You may be dead.
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American poet Gelett Burgess (1866-1951) |
You don't really understand something until you can compute it.
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Computational astrophysicist Michael L. Norman, on numerous occasions. |
Numquam ponenda est pluralitas sine necessitate; Plurality must never be posited without necessity.
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William of Ockham (1287-1347), though versions of "Occam's Razor" can be traced to Ptolomy (90-168 AD): We consider it a good principle to explain the phenomenon by the simplest hypothesis possible. Modern versions include: The simplest explanation is usually the best. |
The most incomprehensible thing about the Universe is that it is comprehensible.
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Albert Einstein, 1879-1955. |
Prediction is very difficult, especially about the future.
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Niels Bohr (1885-1962), often (but inaccurately) attributed to Yogi Berra (1925-). |
I cannot seriously believe in quantum theory because it cannot be reconciled with the idea that physics should represent a reality in time and space, free from spooky actions at a distance.
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Albert Einstein, 1948, on his favourite critique of quantum mechanics where, so the theory requires, a measurement at location B can instantaneously have an influence at location A. On this he had stated the year before: My instinct for physics bristles at this, and in 1935 he wrote: No reasonable definition of reality could be expected to permit this. |
I have stated previously that the arrow of time should follow the arrow of universal expansion, and if the universe should start to collapse, we'd all start getting younger. I was wrong.
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Stephen Hawking in an address to the XIII Texas Symposium on Relativistic Astrophysics, Chicago, 1986 |
Nothing tastes as good as skinny feels.
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model Kate Moss, 2009, who received a backlash from the anti-anorexia crusaders after saying it. Still, this is the best advice this non-anorexic (but always waging the battle of the bulge) has heard on how to resist eating a cake. |
And I find it kinda funny, I find it kinda sad; the dreams in which I'm dying are the best I've ever had; I find it hard to tell you, 'cause I find it hard to take; when people run in circles, it's a very very mad world, mad world.
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from Mad World by Roland Orzabal and Curt Smith, Tears for Fears (1982); covered in 2001 by Michael Andrews and Gary Jules for the soundtrack of Donnie Darko. |
Space to place documents temporarily for uploading.
Looking for my course web pages? Go to my Teaching slide. ZEUS-3D or AZEuS? Go to my Research slide. Primers and manuals? Go to my Document bar. |
Last updated by DAC, March 31, 2013 |
Background: ZEUS-3D simulation showing the magnetic energy density in a super-Alfvénic turbulent medium. |