Blakesley Burkhart
Graduate Student
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Office: 4558 Sterling Hall
Research Interests:
Magnetohydrodynamic Turbulence is an essential physical process in our Galaxy and beyond. How can we better understand it by connecting observations, numerical simulations, and theory?
Biography:
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My Publications
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Gauging the Turbulent Mach Numbers in Optically Thick Clouds
Burkhart, B., Lazarian, A., Ossenkopf, V., Stutzki, J., 2012
Conference Proceedings in "Numerical Modeling of Space Plasma Slows (ASTRONUM 2011)" Pages 9
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Properties of Interstellar Turbulence from Gradients of Linear Polarization Maps
Burkhart, B., Lazarian, A., Gaensler, B., 2012
The Astrophysical Journal, Vol. 749, Pages 145
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Snakes in the Plane: Direct Imaging of Magnetized Turbulence in the Interstellar Medium
Gaensler, B., Haverkorn, M., Burkhart, B., Newton-McGee, K., Ekers, R., et al., 2012
Conference Proceedings in "American Astronomical Society, AAS Meeting #219, #349.04" Pages
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The Column Density Variance-{\cal M}_s Relationship
Burkhart, B., Lazarian, A., 2012
The Astrophysical Journal Letters, Vol. 755, Pages L19
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The GALFA-H I Compact Cloud Catalog
Saul, D., Peek, J., Grcevich, J., Putman, M., Douglas, K., et al., 2012
The Astrophysical Journal, Vol. 758, Pages 44
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