Sources of ancient volcanic rocks are often unknown if they are either eroded and/or covered by younger deposits. This problem, as well as the provenance of reworked volcaniclastic, fluvial and mass-flow deposits, can be partially solved by the application of anisotropy of the magnetic susceptibility (AMS). For massive and poorly sorted volcaniclastic rocks in particular this may be the only way of finding reliable transport directions and therefore allowing for paleogeographic reconstructions. Here, we present a data set of 428 AMS measurements and 249 measurements of sedimentary paleocurrent indicators from the Miocene Tepoztlán Formation at the southern edge of the Transmexican Volcanic Belt (Central Mexico). The highest degree of reliability of AMS measurements is gained for data from lava samples and the lowest from mass flows. Sedimentary structures in sandstones and conglomerates such as trough cross-stratification, asymmetric ripple marks, and the shape of scours and channels could be used to calibrate the results from AMS data and to prove their reliability. AMS data on fluvial deposits point to a drainage system with a W-E flow direction, indicating an outflow of the river system into the ancient Gulf of Mexico.Keywords: Anisotropy of magnetic susceptibility; paleocurrent direction; volcaniclastic; Transmexican Volcanic Belt; Miocene; Mexico 3 In ancient volcanic settings, one challenge in the investigation of volcanic and volcaniclastic deposits is the determination of source vent locations, since former volcanic centers may be either eroded and/or covered by younger deposits. Furthermore, the determination of the provenance of fluvial and mass-flow deposits, arising from the volcanic ring plain itself (Manville et al., 2009, and references therein) or rivers in distal reaches, can also be problematic. In lava flows, both vesicle and crystal preferred orientations have been used extensively for this purpose (e.g., Waters, 1960;Smith and Rhodes, 1972;Walker, 1989;Cashman and Kauahikaua, 1997;Manga, 1998;Iezzi and Ventura, 2002). However, petrological structures such as foliation and lineation due to the movement of a lava flow are often difficult to observe and measure (Bascou et al., 2005). Massive pyroclastic rocks such as ignimbrites and block-and-ash flow deposits rarely show any measurable alignment or structure that can help determine flow direction. However, the magnetic fabric can be used to determine their paleocurrent direction, and the speed, precision, cheapness and range of applicability make it unique in this regard (Tarling and Hrouda, 1993).All materials, even if they do not acquire remanent magnetization, have a magnetic susceptibility (Liu et al., 2001), which is not always isotropic in the rock (Ising, 1942). This spatial susceptibility variation is defined as the anisotropy of magnetic susceptibility (AMS) and reflects the preferred orientation of magnetic minerals in the rock or sediments, i.e. its magnetic fabric (Hrouda, 1982;Tarling and Hrouda, 1993), which yields thr...