Constraining the CME Core Heating and Energy Budget with SOHO/UVCS

@article{Wilson2022ConstrainingTC,
  title={Constraining the CME Core Heating and Energy Budget with SOHO/UVCS},
  author={Maurice L. Wilson and John C. Raymond and Susan T. Lepri and Roberto Lionello and Nicholas A. Murphy and Katharine K. Reeves and Chengcai Shen},
  journal={The Astrophysical Journal},
  year={2022},
  volume={927}
}
We describe the energy budget of a coronal mass ejection (CME) observed on 1999 May 17 with the Ultraviolet Coronagraph Spectrometer (UVCS). We constrain the physical properties of the CME’s core material as a function of height along the corona by using the spectra taken by the single-slit coronagraph spectrometer at heliocentric distances of 2.6 and 3.1 solar radii. We use plasma diagnostics from intensity ratios, such as the O vi doublet lines, to determine the velocity, density, temperature… 
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