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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 1.

O VI channel parameters referring to the period from 1996 April to 1997 December during the daily UVCS synoptic observation program: heliocentric distance of the UVCS instantaneous field of view (a), intensity of the 1031.92 Å (black) and 1037.61 Å (red) spectral lines (b), doublet intensity ratio ρ (c), and variance of the 1031.92 Å line, corrected for instrumental effects, σ2 (d).

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