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Quasi-Periodic Oscillations in Lasco Coronal Mass Ejection Speeds

  • Authors: A. Shanmugaraju, Y.-J. Moon, K.-S. Cho, S. C. Bong, N. Gopalswamy, S. Akiyama, S. Yashiro, S. Umapathy, and B. Vrsnak

SHANMUGARAJU et al. 2010 The Astrophysical Journal 708 450.

  • Provider: AAS Journals

Caption: Figure 9.

Lorentz acceleration (wavy solid gray line) estimated by assuming the solar wind model with an asymptotic speed of 400 km s −1 and using an empirical relation for drag coefficient. The accelerations due to gravitation ( g: monotonously decreasing dash-dotted red line), drag ( a d : wavy dotted blue line), and net acceleration from Figure  8 ( a n : wavy dashed line) are also shown.

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