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GRMHD Prediction of Coronal Variability in Accreting Black Holes

  • Authors: Scott C. Noble and Julian H. Krolik

NOBLE & KROLIK 2009 The Astrophysical Journal 703 964.

  • Provider: AAS Journals

Caption: Figure 9.

Left: phase ψ(ν, r) of dF/ dr fluctuations when seen face-on ( thetav = 5°) for . Note that we deviate from prior figure layouts and use a linear frequency scale here in order to resolve small-scale features. In addition, we show only the lower half of our frequency range. The dashed curve is the local inflow rate ν inflow. Right: the linear, periodic color map used to generate this figure.

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