Published November 26, 2014 | Version v1

Empirical Testing of Solar Coronal and Solar Wind Models

Authors/Creators

  • 1. University of Maryland

Contributors

Supervisor:

  • 1. Harvard Smithsonian Center for Astrophysics

Description

Final presentations of the Center for Astrophysics HEA/SSP Solar Summer Intern Program.

Files

Woolsey_presentation.pdf

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Additional details

References

  • Akinari, N. (2007). Broadening of resonantly scattered ultraviolet emission lines by coronal hole outflows. ApJ, 660: 1660-1673.
  • Cranmer et al. (1999). An empirical model of a polar coronal hole at solar minimum. ApJ, 511: 481.
  • Jacques, S.A. (1977). Momentum and energy transport by waves in the solar atmosphere and solar wind. ApJ, 215: 942-951.
  • Kohl et al. (1995). The Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory. Solar Physics, 162(1-2): 313-356.
  • Landi, E. and Cranmer, S.R. (2009). Ion temperatures in the low solar corona: Polar coronal holes at solar minimum. ApJ, 691: 794-805.
  • Lionello, R., J.A. Linker, and Z. Mikić (2009). Multispectral emission of the Sun during the first whole Sun month: Magnetohydrodynamics simulations. ApJ, 690: 902-912.
  • Ong et al. (1997). Self-consistent and time-dependent solar wind models. ApJ, 474: L143-L145.
  • Withbroe, G.L., J.L. Kohl, and H. Weiser (1982). Probing the solar wind acceleration region using spectroscopic techniques. Space Science Reviews, 33: 17-52.