Here we present timing analysis of a set of eight Rossi X-Ray Timing Explorer (RXTE) observations of the black hole candidate GX 339-4 that were taken during its hard/low state. On long timescales, the RXTE All Sky Monitor data reveal evidence of a 240 day periodicity, comparable to timescales expected from warped, precessing accretion disks. On short timescales all observations save one show evidence of a persistent fQPO≈0.3 Hz quasi-periodic oscillation. The broadband (10-3 to 102 Hz) power appears to be dominated by two independent processes that can be modeled as very broad Lorentzian fits with Q1. The coherence function between soft and hard photon variability shows that if these are truly independent processes, then they are individually coherent, but they are incoherent with one another. This is evidenced by the fact that the coherence function between the hard and soft variability is near unity between 5 × 10?3 to 10 Hz but shows evidence of a dip at f≈1 Hz. This is the region of overlap between the broad Lorentzian fits to the power spectral density. As in Cyg X-1, the coherence also drops dramatically at frequencies 10 Hz. Also as in Cyg X-1, the hard photon variability is seen to lag the soft photon variability with the lag time increasing with decreasing Fourier frequency. The magnitude of this time lag appears to be positively correlated with the flux of GX 339-4. We discuss all of these observations in light of current theoretical models of both black hole spectra and temporal variability.
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