Large coseismic slip was thought to be unlikely to occur on the shallow portions of plate-boundary thrusts, but the 11 March 2011 Tohoku-Oki earthquake [moment magnitude (Mw) = 9.0] produced huge displacements of ~50 meters near the Japan Trench with a resultant devastating tsunami. To investigate the mechanisms of the very large fault movements, we conducted high-velocity (1.3 meters per second) friction experiments on samples retrieved from the plate-boundary thrust associated with the earthquake. The results show a small stress drop with very low peak and steady-state shear stress. The very low shear stress can be attributed to the abundance of weak clay (smectite) and thermal pressurization effects, which can facilitate fault slip. This behavior provides an explanation for the huge shallow slip that occurred during the earthquake.

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[1] Very-low-frequency earthquakes (VLFE) occur within accretionary prisms and near subduction plate boundaries at slip rates of 0.05-2 mm/s. However, the geological and frictional aspects of VLFE remain poorly understood. The thrusts in the Shimanto accretionary complex exhumed from source depths of VLFE are composed of quartz-rich fault rocks with or without clay foliations. We examined the frictional velocity dependence of thrust materials. At slip rates of 0.0028-0.28 mm/s, the powder sample from non-foliated fault rock shows velocity-weakening behavior, while that from foliated fault rock exhibits velocity-strengthening behavior. Both samples show velocity-strengthening behavior at slip rates of 0.28-2.8 mm/s. Microstructural analysis reveals that the velocity-weakening sample shows a shear localization, while the velocity-strengthening sample is marked by clay foliations oblique and parallel to shear zone boundaries. Our results imply that frictional instability generates along quartz-rich fault rock but slip becomes stable at higher slip rates, regardless of mineral composition. This is favorable for the occurrence of VLFE in subduction zones.Citation: Saito, T., K. Ujiie, A. Tsutsumi, J. Kameda, and B. Shibazaki (2013), Geological and frictional aspects of very-lowfrequency earthquakes in an accretionary prism, Geophys. Res. Lett., 40,[703][704][705][706][707][708]

The present study evaluated the histopathological features, biological nature, anatomical location, sex, age and breeds of dogs affected by spontaneous gastrointestinal epithelial tumor. Biopsy samples of gastrointestinal tumors, from 95 dogs were examined and classified according to the WHO histological classification. A total of 131 samples, including 38 gastric, 13 small intestinal, and 80 large intestinal tumors were examined. The study observed that Jack Russell Terriers and Miniature Dachshunds were the breeds with the highest predisposition for gastrointestinal tumors. Gastric tumors included 5 adenomas, 30 adenocarcinomas (12 tubular, 2papillary, 4 tubulopapillary and 12 signet-ring cell carcinomas) and 3 undifferentiated carcinomas. Intestinal tumors included 35 adenomas, 57 adenocarcinomas (43 acinar, 4 papillary, 7 mucinous and 3 signet-ring cell carcinomas), and 1 undifferentiated carcinoma. The study did not detect any difference among the incidence rates of invasion/metastasis in the tubular (44%), papillary (33%) and tubulopapillary (25%) adenocarcinomas. Additionally, the tubular (acinar), papillary and tubulopapillary adenocarcinomas were further divided into 48 polypoid and 17 non-polypoid types, based on their growth patterns. Invasion/metastasis was detected in 21% of the polypoid type and 100% of the non-polypoid type of adenocarcinomas. A correlation was detected between the occurrence of invasion/metastasis and the type of histopathological growth pattern in adenocarcinomas. The study demonstrated that Jack Russell terriers and Miniature Dachshunds are the most common breeds affected by gastrointestinal tumors and the entire group of the canine adenocarcinomas with non-polypoid growth pattern has greater malignant potentials, compared to the adenocarcinomas with polypoid growth patterns.

Among spontaneous neoplasms of the rat central nervous system, the discrimination between astrocytoma and malignant reticulosis (MR) is sometimes difficult because of their similar cell morphology and infiltration patterns. In the present study, we carried out histological and immunohistochemical analyses on a total of sixty-four cases in Sprague-Dawley and F344 rats. These cases were diagnosed as benign/malignant astrocytoma containing no neoplastic oligodendroglial elements or MR according to the diagnostic criteria of the World Health Organization International Classification of Rodent Tumors (Mohr et al. 1994). Astrocytomas were divided into three types and MR into two types based on the number of lesions, cellularity and infiltration patterns, and so on. Although the neoplastic cells from all types showed various immunoreactivities for RM-4 (anti-rat macrophages and dendritic cells), ED-1, and/or vimentin, there were no distinctive differences among these types, and most cells that were positive for RM-4 were also positive for ED-1. None of the tumor types showed any reactivity for GFAP or S-100 protein. From the results of morphological and immunohistochemical examinations, it was indicated that there are no distinctive differences between spontaneous astrocytomas and MR in rats, and they are probably derived from the same cell lineage, that is, microglia, macrophage, or radial glia.