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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 1.

(a–d) Snapshots at, respectively, phiv = {π, π/2, 3π/2, 0}. Each image was taken at thetav = 53° and t = 9000 M with . The axes mark the image's vertical and horizontal extent in the image plane in units of M. Far right: logarithmic color map used to make the images. The intensity is normalized to the maximum intensity of the composite image shown in Figure 2.

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