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Two-temperature Models for Polar Plumes: Cooling by Means of Strong Base Heating

  • Authors: R. Grappin, Y.-M. Wang, and F. Pantellini

Grappin, Wang, & Pantellini 2011 The Astrophysical Journal 727 30.

  • Provider: AAS Journals

Caption: Figure 1.

Effect of depositing energy in the ions but not the electrons, by taking F i g0 = 5 × 10 5 erg cm −2 s −1, H g = 1  R , F e g0 = F e b0 = 0. Dotted curves: solution without base heating, F i b0 = 0. Solid curves: solution with strong base heating, F i b0 = 4 × 10 5 erg cm −2 s −1 and H b = 0.01  R . Top panel: profiles of bulk flow speed u (in units of 100 km s −1), electron temperature T e (in MK), and ion temperature T i (in MK) as a function of heliocentric distance r. Bottom panel: logarithmic profiles of number density n = n e = n i (cm −3) and number flux density nu (in units of 10 5 cm −2 s −1) as a function of r.

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