7 results match your criteria: "DSFTA University of Siena[Affiliation]"
Biodivers Data J
July 2024
Italian National Antarctic Museum (MNA, section of Genoa), Genoa, Italy Italian National Antarctic Museum (MNA, section of Genoa) Genoa Italy.
Background: The order Isopoda Latreille, 1816 consists of species occurring in terrestrial, marine and freshwater environments. In the Southern Ocean (SO), this group is amongst the most speciose and occur at all depths. Isopoda biogeography, despite being studied since the first Antarctic expeditions, is still poorly known from a geographical point of view and shows large occurrence gaps for some groups in specific sectors of the SO.
View Article and Find Full Text PDFBiodivers Data J
March 2024
Italian National Antarctic Museum (MNA, section of Genoa), Genoa, Italy Italian National Antarctic Museum (MNA, section of Genoa) Genoa Italy.
Background: Distributional data on planktonic, benthic and sympagic copepods collected in the framework of the XXXIV Expeditions of the Italian National Antarctic Programme (PNRA) to the Ross Sea sector from 2018-2019 are here provided. These occurrences correspond to specimens collected from the 25 μm filters used in the desalination plant of the Italian research station "Mario Zucchelli" (MZS), located in the Terra Nova Bay area (TNB; Ross Sea, Antarctica). This dataset is a contribution to the Antarctic Biodiversity Portal, the thematic Antarctic node for both the Ocean Biogeographic Information System (AntOBIS) and the Global Biodiversity Information Facility Antarctic Biodiversity Information Facility (ANTABIF).
View Article and Find Full Text PDFRev Sci Instrum
March 2022
DSFTA University of Siena, Via Roma 56, 53100 Siena, Italy.
We present a set of results obtained with an innovative eye-tracker based on magnetic dipole localization by means of an array of magnetoresistive sensors. The system tracks both head and eye movements with a high rate (100-200 Sa/s) and in real time. A simple setup is arranged to simulate head and eye motions and to test the tracker performance under realistic conditions.
View Article and Find Full Text PDFRev Sci Instrum
April 2020
Department of Information Engineering and Mathematics, DIISM University of Siena, Via Roma 56, 53100 Siena, Italy.
We present a system developed to premagnetize liquid samples in an ultra-low-field nuclear magnetic resonance experiment. Liquid samples of a few milliliters are exposed to a magnetic field of about 70 mT, which is abruptly switched off, to leave a transverse microtesla field, where nuclei start precessing. An accurate characterization of the transients and intermediate field level enables a reliable operation of the detection system, which is based on an optical magnetometer.
View Article and Find Full Text PDFRev Sci Instrum
April 2019
Department of Physical Sciences, Earth and Environment, DSFTA University of Siena, Via Roma 56, 53100 Siena, Italy.
Nuclear magnetic resonance detection in ultra-low-field regime enables the measurement of different components of a spurious remanence in the polymeric material constituting the sample container. A differential atomic magnetometer detects simultaneously the static field generated by the container and the time-dependent signal from the precessing nuclei. The nuclear precession responds with frequency shifts and decay rate variations to the container magnetization.
View Article and Find Full Text PDFRev Sci Instrum
March 2017
DSFTA University of Siena, Via Roma, 56, 53100 Siena, Italy.
A low cost, stable, programmable, unipolar current source is described. The circuit is designed in view of a modular arrangement, suitable for applications where several DC sources must be controlled at once. A hybrid switching/linear design helps in improving the stability and in reducing the power dissipation and cross-talking.
View Article and Find Full Text PDFMinor Planet Bull
January 2016
Carpione Observatory (K49), San Casciano in Val di Pesa (FI), ITALY.
The Hungaria asteroid 7958 Leakey is a known binary (Warner et al., 2012). It was observed in 2015 to confirm and refine the original periods for the primary rotation and satellite orbit.
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