Structural Aspects of Traditional Cretan Masonry

Glowacki, K.T., J. M. Nichols, and N. L. Holland. “Structural Aspects of Traditional Cretan Masonry.” In Proceedings of the 15th International Brick and Block Masonry Conference, Florianópolis, Brazil, June 3–6, 2012, edited by Humberto Ramos Roman and Guilherme Aris Parsekian, CD-ROM, Paper No. 1C4. Florianopolis, Brazil: 15 IBMAC. ISBN: 9788563273109. (DOI: 10.13140/RG.2.1.1304.2728).The island of Crete has a long tradition of stone masonry construction, beginning over 8000 years before present. As noted by architectural historians, the vernacular architecture of modern (pre-World War II) villages on Crete has many close parallels with house remains uncovered in the archaeological record of the Minoan Bronze Age (ca. 3000-1050 BCE). Archaeologists have used modern ethnographic comparisons effectively to shed light upon issues ranging from the interpretation of ancient house plans to a better understanding of construction techniques, the use of local resources, and the effects of abandonment processes on the built environment. A full-scale replica of a typical Cretan house from the 12th-11th century BCE (Late Minoan IIIC period) is planned for construction in College Station. The first stage of the building will comprise a single room, ca. 6.20 m by 5.20 m, constructed of stacked limestone with minimal earth mortar, timber ceiling beams and laths, a layer of brush, and topped with a flat clay overlay. The purpose of this paper is to outline the design and structural analysis of the building, and to discuss issues related to construction processes, climate, and ventilation that may apply to both archaeological/historical and modern contexts. Modern interest in this traditional type of building technique stems from the use of limestone blocks in construction, and the potential it has to be a key element of the greening of building construction practices. This study forms one element of a major study of limestone and its uses

Spectroscopy of 54^{54}Ti and the systematic behavior of low energy octupole states in Ca and Ti isotopes

Excited states of the $N=32$ nucleus $^{54}$Ti have been studied, via both inverse-kinematics proton scattering and one-neutron knockout from $^{55}$Ti by a liquid hydrogen target, using the GRETINA $\gamma$-ray tracking array. Inelastic proton-scattering cross sections and deformation lengths have been determined. A low-lying octupole state has been tentatively identified in $^{54}$Ti for the first time. A comparison of $(p,p')$ results on low-energy octupole states in the neutron-rich Ca and Ti isotopes with the results of Random Phase Approximation calculations demonstrates that the observed systematic behavior of these states is unexpected.Comment: 7 pages, 8 figure

Spectroscopy of 54^{54}Ti and the systematic behavior of low energy octupole states in Ca and Ti isotopes

Excited states of the $N=32$ nucleus $^{54}$Ti have been studied, via both inverse-kinematics proton scattering and one-neutron knockout from $^{55}$Ti by a liquid hydrogen target, using the GRETINA $\gamma$-ray tracking array. Inelastic proton-scattering cross sections and deformation lengths have been determined. A low-lying octupole state has been tentatively identified in $^{54}$Ti for the first time. A comparison of $(p,p')$ results on low-energy octupole states in the neutron-rich Ca and Ti isotopes with the results of Random Phase Approximation calculations demonstrates that the observed systematic behavior of these states is unexpected.Comment: 7 pages, 8 figure

Universal interpretations of vocal music

Despite the variability of music across cultures, some types of human songs share acoustic characteristics. For example, dance songs tend to be loud and rhythmic, and lullabies tend to be quiet and melodious. Human perceptual sensitivity to the behavioral contexts of songs, based on these musical features, suggests that basic properties of music are mutually intelligible, independent of linguistic or cultural content. Whether these effects reflect universal interpretations of vocal music, however, is unclear because prior studies focus almost exclusively on English-speaking participants, a group that is not representative of humans. Here, we report shared intuitions concerning the behavioral contexts of unfamiliar songs produced in unfamiliar languages, in participants living in Internet-connected industrialized societies (n = 5,516 native speakers of 28 languages) or smaller-scale societies with limited access to global media (n = 116 native speakers of three non-English languages). Participants listened to songs randomly selected from a representative sample of human vocal music, originally used in four behavioral contexts, and rated the degree to which they believed the song was used for each context. Listeners in both industrialized and smaller-scale societies inferred the contexts of dance songs, lullabies, and healing songs, but not love songs. Within and across cohorts, inferences were mutually consistent. Further, increased linguistic or geographical proximity between listeners and singers only minimally increased the accuracy of the inferences. These results demonstrate that the behavioral contexts of three common forms of music are mutually intelligible cross-culturally and imply that musical diversity, shaped by cultural evolution, is nonetheless grounded in some universal perceptual phenomena

Design of and initial results from a highly instrumented reactor for atmospheric chemistry (HIRAC)

International audienceThe design of a Highly Instrumented Reactor for Atmospheric Chemistry (HIRAC) is described and initial results obtained from HIRAC are presented. The ability of HIRAC to perform in-situ laser-induced fluorescence detection of OH and HO2 radicals with the Fluorescence Assay by Gas Expansion (FAGE) technique establishes it as internationally unique for a chamber of its size and pressure/temperature variable capabilities. In addition to the FAGE technique, HIRAC features a suite of analytical instrumentation, including: a multipass FTIR system; a conventional gas chromatography (GC) instrument and a GC instrument for formaldehyde detection; and NO/NO2, CO, O3, and H2O vapour analysers. Ray tracing simulations and measurements of the blacklamp flux have been utilized to develop a detailed model of the radiation field within HIRAC. Comparisons between the analysers and the FTIR coupled to HIRAC have been performed, and HIRAC has also been used to investigate pressure dependent kinetics of the chlorine atom reaction with ethene and the reaction of O3 and t-2-butene. The results obtained are in good agreement with literature recommendations and Master Chemical Mechanism predictions. HIRAC thereby offers a highly instrumented platform with the potential for: (1) high precision kinetics investigations over a range of atmospheric conditions; (2) detailed mechanism development, significantly enhanced according to its capability for measuring radicals; and (3) field instrument intercomparison, calibration, development, and investigations of instrument response under a range of atmospheric conditions

Two-Screen Scattering in CRAFT FRBs

Temporal broadening is a commonly observed property of fast radio bursts (FRBs), associated with turbulent media which cause radiowave scattering. Similarly to dispersion, scattering is an important probe of the media along the line of sight to an FRB source, such as the circum-burst or circum-galactic mediums (CGM). Measurements of characteristic scattering times alone are insufficient to constrain the position of the dominant scattering media along the line of sight. However, where more than one scattering screen exists, Galactic scintillation can be leveraged to form strong constraints. We quantify the scattering and scintillation in 10 FRBs with 1) known host galaxies and redshifts and 2) captured voltage data enabling high time resolution analysis, obtained from the Commensal Real-time ASKAP (Australian Square Kilometre Array Pathfinder) Fast Transient survey science project (CRAFT). We find strong evidence for two screens in three cases. For FRBs 20190608B and 20210320C, we find evidence for scattering screens less than approximately 16.7 and 3000 kpc respectively, from their sources. For FRB 20201124A we find evidence for a scattering screen at $\approx$26 kpc. Each of these measures is consistent with the scattering occurring in the host ISM (inter-stellar medium) or CGM. If pulse broadening is assumed to be contributed by the host galaxy ISM or circum-burst environment, the definitive lack of observed scintillation in four FRBs in our sample suggests that existing models may be over-estimating scattering times associated with the Milky Way's ISM, similar to the anomalously low scattering observed for FRB 20201124A.Comment: 13 pages, 9 figures, 1 table. Submitted to MNRA