  We report on the RXTE/PCA observation of the X-ray burster 1E1724-3045
located in the globular cluster Terzan 2. The persistent X-ray emission shows a
high level of noise variability, the so-called High Frequency Noise (HFN) with
a fractional Root Mean Squared (RMS) of about 25% in the 2E-3 - 40 Hz range.
The strong HFN together with the hardness of its X-ray spectrum suggest that
1E1724-3045 is an ``Atoll'' source which was in its ``Island'' state during the
observation. The Fourier Power Density Spectra (PDS) can be modeled in terms of
the sum of two ``shot noise'' components for which the shots have a single-side
exponential shape. The characteristic shot decay timescales inferred from the
best fitting of the PDS are ~680 and 16 msec respectively. The two components
contribute similarly to the total RMS (about 15%). The PDS contains also a
third component: a broad and asymmetric peaked noise feature centered at 0.8
Hz. This Quasi Periodic Oscillation-like (QPO) feature contributes at the level
of ~ 10% to the total RMS. The integrated RMS of all three components shows a
positive correlation with energy up to at least 40 keV. We also show that
1E1724-3045 has striking timing similarities with the black hole candidate GRO
J0422+32 (Nova Persei 1992). Our observation demonstrates that a low frequency
QPO simultaneously with a high level of RMS is not a timing signature unique to
black holes. This extends the growing list of similarities between Atoll
sources and black hole systems.
