Sources


Rachael Roettenbacher

Faculty Advisor: Robert Harmon


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Theory

Method

Analysis

Conclusions

Sources 

The works used to put this project together:

  • Berdyugina, S., Ilyin, I., & Tuominen, I. 1998, in ASP Conf. Ser. 154, 1384; The Tenth Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, ed. R. A. Donahue J. A. Bookbinder (San Francisco: ASP) 
  • Carroll, B. W., & Ostlie, D. A. 2007, An Introduction to Modern Astrophysics (2nd ed.; New York: Pearson)
  • Foukal, P., 1990, Solar Astrophysics (New York: Wiley) 
  • Harmon, R. O. & Crews, L. J. 2000, AJ, 120, 3274
  • Harmon, R. O. & Roettenbacher, R. M. 2006, in AAS Meeting 209, 2906; Bulletin of the American Astronomical Society (Seattle: AAS) 
  • Lawrence, J. K., Cadavid, A.C., & Ruzmaikin, A. 2008, in ArXiv e-prints 803; 0803.3260
  • Marino, G., Rodono, M., Leto, G., & Cutispoto, G. 1999, AA, 352, 189 
  • Press, W. H., Tuekolsky,  S. A., Vetterling, W. T., & Flannery, B. P. 1992, Numerical Recipes in FORTRAN 2e (Cambridge: Cambridge Univ.) 
  • Zirin, H. 1989, Astrophysics of the Sun (New York: Cambridge Univ.)

I would like to extend my thanks to several (groups of) people:

Ohio Wesleyan University's Department of Physics and Astronomy for having senior research as a graduation requirement.  It was well worth all of the stress.

Gregory Henry of the Center of Excellence in Information Systems at Tennessee State University for providing us with a massive amount of data.

Finally, as this is the culmination of my undergraduate career, I thank everyone who had a hand in supporting me for the past four years. 

 For our final results, please see our article in the Astronomical Journal:  Roettenbacher et al. 2011.