352 research outputs found

    Collision detection and proximity warning systems for mobile mining equipment: A human factors exploration

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    The relatively high number of collisions between mining vehicles is the primary reason why collision detection and proximity warning systems are being increasingly introduced in this domain. This work presents a series of studies undertaken in underground mining where a prototype proximity warning system has recently been introduced. These studies encompassed a review of the system constraints (detection distances), an ergonomic audit of the system interface, Cognitive Tasks Analyses and other structured interview methods, a naturalistic field study, and a human factors risk assessment. All combined, the studies reviewed, from a user-centred perspective, the effectiveness of a system being trialled. Preliminarily results emerging to date and provisional recommendations for future system development or additional research are briefly outlined in this paper

    Knowledge elicitation solutions for improving performance and efficiency

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    Despite advances in mechanisation and automation processes, mining remains a people intensive industry, a large proportion of whom are responsible for operating and maintaining mining equipment under conditions that challenge even the most experienced people. Mining techniques, equipment designs and the work environment are constantly evolving and changing, imposing new demands on the technical competence of workers. With the trend towards global mining companies and ease of international travel, the workforce of the future may well encompass social and cultural changes that need to be addressed. The system of work rosters used by mine sites adds a further element of change to the situation, all of which contribute to the potential for unwanted events during normal operation

    Human factors methods to design safer mobile mining equipment

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    Placing meta-stable states of consciousness within the predictive coding hierarchy: The deceleration of the accelerated prediction error.

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    While many studies have linked prediction errors and event related potentials at a single processing level, few consider how these responses interact across levels. In response, we present a factorial analysis of a multi-level oddball task - the local-global task - and we explore it when participants are sedated versus recovered. We found that the local and global levels in fact interact. This is of considerable current interest, since it has recently been argued that the MEEG response evoked by the global effect corresponds to a distinct processing mode that moves beyond predictive coding. This interaction suggests that the two processing modes are not distinct. Additionally, we observed that sedation modulates this interaction, suggesting that conscious awareness may not be completely restricted to a single (global) processing level

    The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star-Black Hole Merger GW190814

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    We present optical follow-up imaging obtained with the Katzman Automatic Imaging Telescope, Las Cumbres Observatory Global Telescope Network, Nickel Telescope, Swope Telescope, and Thacher Telescope of the LIGO/Virgo gravitational wave (GW) signal from the neutron star-black hole (NSBH) merger GW190814. We searched the GW190814 localization region (19 deg2^{2} for the 90th percentile best localization), covering a total of 51 deg2^{2} and 94.6% of the two-dimensional localization region. Analyzing the properties of 189 transients that we consider as candidate counterparts to the NSBH merger, including their localizations, discovery times from merger, optical spectra, likely host-galaxy redshifts, and photometric evolution, we conclude that none of these objects are likely to be associated with GW190814. Based on this finding, we consider the likely optical properties of an electromagnetic counterpart to GW190814, including possible kilonovae and short gamma-ray burst afterglows. Using the joint limits from our follow-up imaging, we conclude that a counterpart with an rr-band decline rate of 0.68 mag day−1^{-1}, similar to the kilonova AT 2017gfo, could peak at an absolute magnitude of at most −17.8-17.8 mag (50% confidence). Our data are not constraining for ''red'' kilonovae and rule out ''blue'' kilonovae with M>0.5M⊙M>0.5 M_{\odot} (30% confidence). We strongly rule out all known types of short gamma-ray burst afterglows with viewing angles <<17∘^{\circ} assuming an initial jet opening angle of ∼\sim5.2∘5.2^{\circ} and explosion energies and circumburst densities similar to afterglows explored in the literature. Finally, we explore the possibility that GW190814 merged in the disk of an active galactic nucleus, of which we find four in the localization region, but we do not find any candidate counterparts among these sources.Comment: 86 pages, 9 figure
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