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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 3.

Left: normalized light curves (solid curves) for and all values of thetav. The light curves and their mean values (dashed curves) have been shifted vertically by incremental factors of two for clarity. Right: normalized power spectra of these light curves compared to their best power-law fits (dashed curves). The power spectra are separated by incremental factors of 100. In both plots, the curves are ordered bottom to top in increasing order of thetav.

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