The Optimization of Microbus-Based Public Transportation Facilities in Jayapura City

Public transport services will work well if there is a balance between supply and demand. The research aimed to analyze the performance and the needs for the number of public transportation facilities based on the microbuses in Jayapura City. The types of the public transports, which would be discussed, were the microbuses which operated in 12 routes of the total routes of 26 in Jayapura city; those were B1, B2, B3, B4, J1, J2, K, I1, E, G, IA and I. The analyses of the performance and the demand for number of public transports were analyzed based on the load factor and the break event in accordance with the value of the vehicles operating costs (BOK) in setting tariffs. The research results indicated that the standard performance value of the public transport route code of K, I1, G, IA were categorized as less, while the routes of B1, B2, B3, B4, J1, J2, E and IB were categorized as medium. The microbuses demand was only 50% of the total microbuses now operating in Jayapura city

Adrenocortical status in infants and children with sepsis and septic shock

AbstractBackgroundThe benefit from corticosteroids remains controversial in sepsis and septic shock and the presence of adrenal insufficiency (AI) has been proposed to justify steroid use.AimTo determine adrenal state and its relation with outcome in critical children admitted with sepsis to PICU of Cairo University, Children Hospital.MethodsThirty cases with sepsis and septic shock were studied. Cortisol levels (CL) were estimated at baseline and after high-dose short ACTH stimulation in those patients and in 30 matched controls. Absolute AI was defined as basal CL<7μg/dl and peak CL<18μg/dl. Relative AI was diagnosed if cortisol increment after stimulation is <9μg/dl.ResultsOverall mortality of cases was 50%. The mean CL at baseline in cases was higher than that of controls (51.39μg/dl vs. 12.83μg/dl, p=0.000). The mean CL 60min after ACTH stimulation was higher than that of controls (73.38μg/dl vs. 32.80μg/dl, p=0.000). The median of %rise in cases was lower than that of controls (45.3% vs. 151.7%). There was a positive correlation between basal and post-stimulation cortisol with number of system failure, inotropic support duration, mechanical ventilation days, and CO2 level in blood. There was a negative correlation between basal and post stimulation cortisol with blood pH and HCO3.ConclusionRAI is common with severe sepsis/septic shock. It is associated with more inotropic support and has higher mortality. Studies are warranted to determine whether corticosteroid therapy has a survival benefit in children with RAI and catecholamine resistant septic shock

A Relationship Model between Accident Factors and the Traffic Accident Severity Using Logistic Regression Model

The present paper purposes to develop the relationship model between the factors of accidents and severity level of traffic accidents by using multinomial logistic regression model approach, for a case study the traffic accident in Makassar City, Indonesia. In further, the study evaluates the traffic accident factors which significantly influence the traffic accident severity level. In this regard, the outcome variable is the severity level of the traffic accident which has three attributes, i.e., death, serious injury, and minor injury. The explanatory variables involve victim characteristics and traffic accident characteristics. The present study used the traffic accident database during 2012 – 2015 which recorded by the traffic police agency in the city. The model calibration results show that the relationship model has a good accuracy level. The victim position and the collision types significantly influence the severity accident level. The results provide basic information for efforts in reducing traffic accidents.

Locus of Control as Budget Slack Moderator: The Role of Ethical Leadership and Budget Participation

The current study investigates the impact of Budget Participation and Ethical Leadership on Budget Slack. Further, the study investigates how Locus of Control serves as a moderator. The study sample includes bankers working in the Egyptian banking sector. The study deployed an electronic survey. Of the 384 total distributed questionnaires 275 were retrieved, with a response rate of 71.6%. The final sample for the statistical analysis was 251 questionnaires after all exclusions. For testing hypothesis about the relationship between the study variables simple and multiple regression models were adapted. The study results revealed a negative and significant impact of Ethical Leadership on Budget Slack, while Budget Participation was found to affect Budget Slack behaviour positively and significantly. Furthermore, our study revealed that Locus of Control partially and negatively moderating the correlation between Ethical Leadership and Budget slack. These findings contribute to the organizational behavior and management accounting literature, representing one of the first studies to examine this interdisciplinary relationship and confirm the moderating roles identified in African and Middle Eastern contexts

Magnetically Torqued Thin Accretion Disks

We compute the properties of a geometrically thin, steady accretion disk surrounding a central rotating, magnetized star. The magnetosphere is assumed to entrain the disk over a wide range of radii. The model is simplified in that we adopt two (alternate) ad hoc, but plausible, expressions for the azimuthal component of the magnetic field as a function of radial distance. We find a solution for the angular velocity profile tending to corotation close to the central star, and smoothly matching a Keplerian curve at a radius where the viscous stress vanishes. The value of this ''transition'' radius is nearly the same for both of our adopted B-field models. We then solve analytically for the torques on the central star and for the disk luminosity due to gravity and magnetic torques. When expressed in a dimensionless form, the resulting quantities depend on one parameter alone, the ratio of the transition radius to the corotation radius. For rapid rotators, the accretion disk may be powered mostly by spin-down of the central star. These results are independent of the viscosity prescription in the disk. We also solve for the disk structure for the special case of an optically thick alpha disk. Our results are applicable to a range of astrophysical systems including accreting neutron stars, intermediate polar cataclysmic variables, and T Tauri systems.Comment: 9 sharper figs, updated reference

New Polymer Syntheses Part: 55#. Novel Conducting Arylidene Polymers and Copolymers Based on Methyl-Cyclohexanone Moiety

A new interesting class of conducting polymers based on methyl-cyclohexanone in the polymer main chain has been synthesized by solution polycondensation of terephthalaldehyde with methyl-cyclohexanone. Copolymers containing different cycloalkanone moieties were also synthesized using solution polycondensation technique. The model compound I was synthesized by the interaction of methyl-cyclohexanone monomer with benzaldehyde, and its structure was confirmed by elemental and spectral analyses. The resulting new polymers and copolymers were characterized by elemental and spectral analyses, beside solubility and viscometry measurements. The thermal properties of those polymer and copolymers were evaluated by TGA, DrTGA and DTA measurements and correlated to their structural units. PDT as well as T10 was in the range from 205 to 370 ºC. In addition, T10 thermal stability for all the polymers was in theorder: VI&gt; II &gt; III &gt; IV &gt; V. X–ray analysis showed that it has some degree of crystallinity in the region 2q = 5–60 degree.The UV– visible spectra of some selected polymers were measured in DMSO solution and showed absorption bands in the range 265-397 nm, due to n – π* and π – π* transition. The morphological properties of copolymer IV as selected examples were tested by SEM. The electrical conductivities of the synthesized polymers and copolymers enhanced to become in the range of 10-9-10-8 S cm-1 by doping with iodine

New Mixed Ligand Complexes of Ditertiary Phosphanes with Ni(II) Alkylxanthates

Mixed Iigand complexes of Ni(II) with alkylxanthates and ditertiary phosphanes of the composition Ni(ROCSSb(diphoshhave been prepared, where R = methyl, ethyl, propyl, butyl, and cyclohexyl and diphos = bis(diphenylphosphino)ethane (dpe) and bis- (diphenylphosphino)butane (dpb). The newly prepared compounds were characterized on the basis of chemical analyses, infrared and electronic spectra, lH-NMR, molar conductance, and thermal analysis. A square planar structure was proposed for the complexes

"Propeller" Regime of Disk Accretion to Rapidly Rotating Stars

We present results of axisymmetic magnetohydrodynamic simulations of the interaction of a rapidly-rotating, magnetized star with an accretion disk. The disk is considered to have a finite viscosity and magnetic diffusivity. The main parameters of the system are the star's angular velocity and magnetic moment, and the disk's viscosity, diffusivity. We focus on the "propeller" regime where the inner radius of the disk is larger than the corotation radius. Two types of magnetohydrodynamic flows have been found as a result of simulations: "weak" and "strong" propellers. The strong propeller is characterized by a powerful disk wind and a collimated magnetically dominated outflow or jet from the star. The weak propeller have only weak outflows. We investigated the time-averaged characteristics of the interaction between the main elements of the system, the star, the disk, the wind from the disk, and the jet. Rates of exchange of mass and angular momentum between the elements of the system are derived as a function of the main parameters. The propeller mechanism may be responsible for the fast spinning-down of the classical T Tauri stars in the initial stages of their evolution, and for the spinning-down of accreting millisecond pulsars.Comment: 18 pages, 16 figures, ApJ (accepted), added references, corrected typos; see animation at http://astrosun2.astro.cornell.edu/us-rus/disk_prop.ht

Warping of Accretion Disks with Magnetically Driven Outflows: A Possible Origin for Jet Precession

Current theoretical models for the outflows/jets from AGN, X-ray binaries and young stellar objects involve large-scale magnetic fields threading an underlying accretion disk. We suggest that such a disk is subjected to warping instability and retrograde precession driven by magnetic torques associated with the outflow. The growth timescale for the disk warp and the precession period are of order the radial infall time of the disk. These effects may be relevant to jet precession and other variabilities observed in many systems.Comment: 4 pages with 2 figures. ApJL in pres