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On the Fast Solar Wind Heating and Acceleration Processes: A Statistical Study Based on the UVCS Survey Data

  • Authors: Daniele Telloni, Silvio Giordano, and Ester Antonucci

2019 The Astrophysical Journal Letters 881 L36.

  • Provider: AAS Journals

Caption: Figure 2.

(a) ρσ2 scatter plot for UVCS O VI observations performed between 1.3 and 2.8 R (different colors refer to different distances as reported in the legend); the corresponding values of the Spearman's rank correlation factor r are also shown. (b) Radial profile of the correlation factor r fitted with a logarithmic function (red curve). (c) Intensity ratio ρ as a function of the UVCS observation distance (colors are the same as used for panel (a)); the corresponding mean values and error bars (inferred from the standard deviation) are also displayed; ρ = 0.5 is marked by the dashed line; the sonic point rc ≃ 1.9 R is indicated by the dotted line. (d) ρσ2 scatter plot in the subsonic (blue) and supersonic (red) regions, separated by the ρ = 0.5 dashed line. (e) Radial profile of the amplitude of the ρ (red) and σ2 (blue) fluctuations, normalized to the corresponding average values; the dashed line marks the sonic point rc, separating regions of subsonic and supersonic flow.

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