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Figure C11Taurano (Villa Lauro); baulk showing a thick sequence of the Pollena syn-eruptive lahar units filling the Roman villa. The fallout sequence is not exposed in the villa, likely due to the presence of a roof. The deposit below the damaged walls is composed of bot for trading multiple lahar units represented by the Gms lithofacies (see Table 2). Finally, routine magnetic measurements were done on the lahar matrix to determine the characteristic remanent magnetization (ChRM) by thermal and alternating field demagnetizations. The direction of the Earth’s magnetic field during the Pollena eruption is well-known (Zanella et al., 2008).

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The presence of the erosional features (Fig. 16a), and the fact that the deposits are mostly composed of massive and relatively thick units (Fig. 16b), suggests that high sediment transport and deposition both occurred in the same area (Doronzo and Dellino, 2013; Roche, 2015). Such occurrences of erosion and accumulation of multiple units were useful to inform the lahar modeling of de’ Michieli Vitturi et al. (2024). The methodology used in this work is geological (see Sect. 3.2), and the syn-eruptive definition of lahars is necessary to avoid underestimations of the volcanic hazard from sub-Plinian eruptions at Vesuvius. This study focuses on the analysis of pyroclastic fall and flow deposits and of the syn- and post-eruptive lahar deposits related to two sub-Plinian eruptions of Vesuvius in 472 CE (Pollena) and 1631.

In particular, the sampling was mostly made on the syn-eruptive lahar deposits, but also on the post-eruptive and, in a few cases, on the primary pyroclastic deposits. All lab analyses were performed in the laboratories of sedimentology and optical microscopy at the Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Napoli Osservatorio Vesuviano (INGV–OV). The material samples were pre-heated at a temperature of 60–70 °C to eliminate any fraction of humidity and then quartered and sieved. To avoid any breaking of fragile clasts like pumices, the dry-sieving of the grain-size classes between −4 (a coarse limit variable depending on the sample) and 0 phi was made manually, while for the classes between 0.5 and 5 phi a mechanical sieving apparatus was used. The platform offers a multichannel support system, including phone, email, and live chat, ensuring that users can reach out through their preferred mode of communication.

The magnetic fabric in this type of deposit records the main flow direction (local or regional) followed during the emplacement processes. The second aspect was (ii) estimating the deposition temperature (Tdep) of the deposits to understand whether the lahar was triggered soon after the eruption or at later times. The hypothesis is that the temperature is higher in the case of syn-eruptive lahars deriving from hot (pyroclastic current) deposits and lower in all other cases. The third aspect was (iii) testing the relative sequence (contemporaneity) of the lahar emplacement with respect to the Pollena eruption.

The presence of slightly humified surfaces below the lahar deposits or traces of human artifacts, such as excavations and plowing, are considered to be evidence of a long period without deposition; also in this case, the lahars are considered to be post-eruptive. In other words, the similar componentry of the lahar and pyroclastic deposits and the evidence of short-term exposure between these two are strong indicators of the syn-eruptive occurrence of the lahar events. Instead, the absence of such features is more indicative of a post-eruptive origin, i.e., lahar events more spaced in time from the corresponding eruption. We used a set of geological, stratigraphical, sedimentological, archeological, and pedological information for the reconstruction of the type of events, their emplacement mechanisms, timing, and impact on pre-existing structures and environment.

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A massive deposit follows upward; it is progressively humified and contains abundant reworked and rounded pumice clasts from the Avellino eruption. The top humified surface is almost always eroded by anthropogenic activity and is generally plowed (p1 in Fig. C2). It is few centimeters thick and is composed of a basal layer of dark coarse ash (small pumice fragments), overlain by a massive ash bed, containing abundant accretionary lapilli.