Rebecca McMullen - What does she do?I study the fluid dynamics of short flux tubes such as those found in x-ray bright points, the building blocks of the solar corona. My work focuses on the coupling of the corona to the chromosphere and how the energy passes from system to system through a constricted magnetic field. I numerically simulate flux tubes of specific geometry, using a code developed at MSU.Some recent work for your edification: |
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R.A. McMullen, Unpublished Solar Journal Club Presentation of 02/21/02.
R.A. McMullen, D.W. Longcope, C.C. Kankelborg, In Press, Yohkoh10 Proceedings | PS (135 kb) | | PDF (101 kb) |
D.S. Brown, C.E. Parnell, E.E. DeLuca, L. Golub, R.A. McMullen, July 2001, Solar Physics, 201, 2, 305-321, | PDF(700 kb) |
S.K. Antiochos, E.E. DeLuca, L. Golub, R.A. McMullen, October 2000, ApJ Letters, 542,2, L151-L154, | PS (1143 kb) | | PDF (401 kb) |
G. Aulanier, S.K. Antiochos, E.E. De Luca, R.A. McMullen, L. Golub, September 10, 2000, The Astrophysical Journal, 540, 1126-1142, | PDF (6762 kb) | | PS (9449 kb) |
C. J. Schrijver, R. A. McMullen, March 10, 2000, Astrophysical Journal, 531, 1121-1128, | PS (391kb) | | PDF (164kb) |
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