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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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 GALFA-HI Survey: Analyzing The New Ultra-Compact Cloud Catalog.
Saul, D., Peek, J., Grcevich, J., Putman, M., Douglas, K., et al., 2012
Conference Proceedings in "American Astronomical Society, AAS Meeting #219, #349.18" Pages
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Interstellar Sonic and Alfvénic Mach Numbers and the Tsallis Distribution
Tofflemire, B., Burkhart, B., Lazarian, A., 2011
The Astrophysical Journal, Vol. 736, Pages 60
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Low-Mach-number turbulence in interstellar gas revealed by radio polarization gradients
Gaensler, B., Haverkorn, M., Burkhart, B., Newton-McGee, K., Ekers, R., et al., 2011
Nature, Vol. 478, Pages 214-217
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