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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 4.

Left: normalized light curves (solid curves) for thetav = 29° and all values of . 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 .

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