Collegiate Sport Participation and Student-Athlete Development through the Lens of Emotional Intelligence

A continued debate persists over the place of sport within institutions of higher education. Proponents of sport champion its ability to contribute to a holistic notion of education and develop an array of competencies touted in institutional missions. There is however a dearth of empirical data examining the educational impact of athletic participation at the college level. This paper assessed the educational ability of collegiate sport participation in a unique manner, through the lens of Emotional Intelligence (EI). Student-athletes and students at five NCAA Division III institutions completed online assessments prior to and after the completion of the winter sports seasons. Evidence was produced that participation in a single season of collegiate sport does not develop interpersonal, intrapersonal, and leadership capacities significantly differently from the collegiate experience of students not participating in athletics. Institutions are advised to explore EI interventions as way to maximize the educative potential of sport

The Acute Physiological Responses of Eccentric Cycling During the Recovery Periods of a High Intensity Concentric Cycling Interval Session

Eccentric and concentric exercise is associated with disparate acute and chronic responses. We uniquely interspersed workload equivalent eccentric cycling during each recovery period of a high intensity interval training (HIIT) cycling trial to determine acute cardiopulmonary, thermal and psycho-physiological responses. Twelve males [age 28 years (SD 6), peak oxygen consumption 48 mL ⋅ kg-1 ⋅ min-1 (SD 6)] completed two high intensity interval cycling trials [4 x 5 min, 60% peak power output (PPO)] separated by 7-10 days. The CONR trial required participants to cycle concentrically during each recovery period (5 min, 30% PPO). The ECCR trial modified the recovery to be eccentric cycling (5 min, 60% PPO). High intensity workload (CONR: 187 ± 17; ECCR: 187 ± 21 W), oxygen consumption (CONR: 2.55 ± 0.17; ECCR: 2.68 ± 0.20 L ⋅ min-1), heart rate (CONR: 165 ± 7; ECCR: 171 ± 10 beats ⋅ min-1) and RPE legs (CONR: 15 ± 3; ECCR: 15 ± 3) were equivalent between trials. Eccentric cycling recovery significantly increased external workload (CONR: 93 ± 18; ECCR: 196 ± 24 W, P \u3c 0.01) yet lowered oxygen consumption (CONR: 1.51 ± 0.18; ECCR: 1.20 ± 0.20 L ⋅ min-1, P \u3c 0.05) while heart rate (CONR: 132 ± 13; ECCR: 137 ± 12 beats ⋅ min-1) and RPE of the legs (CONR: 11 ± 7; ECCR: 12 ± 7) remained equivalent. There was no significant difference in the aural temperature between the trials (ECCR: 37.3 ± 0.1°C; CONR: 37.4 ± 0.1°C, P \u3e 0.05), yet during recovery periods mean skin temperature was significantly elevated in the ECCR (ECCR: 33.9 ± 0.2°C; CONR: 33.3 ± 0.2°C, P \u3c 0.05). Participants preferred ECCR (10/12) and rated the ECCR as more achievable (82.8 ± 11.4 mm) than CONR (79.4 ± 15.9 mm, P \u3c 0.01). In conclusion, eccentric cycling during the recovery period of a HIIT training session, offers a novel approach to concurrent training methodology. The unique cardiopulmonary and skeletal muscle responses facilitate the achievement of both training stimuli within a single exercise bout

Offsetting of CO₂ emissions by air capture in mine tailings at the Mount Keith Nickel Mine, Western Australia: Rates, controls and prospects for carbon neutral mining

The hydrated Mg-carbonate mineral, hydromagnesite [Mg₅(CO₃)₄(OH)₂•4H₂O], precipitates within mine tailings at the Mount Keith Nickel Mine, Western Australia as a direct result of mining operations. We have used quantitative mineralogical data and δ¹³C, δ¹⁸O and F¹⁴C isotopic data to quantify the amount of CO₂fixation and identify carbon sources. Our radiocarbon results indicate that at least 80% of carbon stored in hydromagnesite has been captured from the modern atmosphere. Stable isotopic results indicate that dissolution of atmospheric CO₂ into mine tailings water is kinetically limited, which suggests that the current rate of carbon mineralization could be accelerated. Reactive transport modeling is used to describe the observed variation in tailings mineralogy and to estimate rates of CO₂ fixation. Based on our assessment, approximately 39,800 t/yr of atmospheric CO₂ are being trapped and stored in tailings at Mount Keith. This represents an offsetting of approximately 11% of the mine's annual greenhouse gas emissions. Thus, passive sequestration via enhanced weathering of mineral waste can capture and store a significant amount of CO₂. Recommendations are made for changes to tailings management and ore processing practices that have potential to accelerate carbonation of tailings and further reduce or completely offset the net greenhouse gas emissions at Mount Keith and many other mines

Swift/XRT monitoring of five orbital cycles of LSI +61 303

LSI +61 303 is one of the most interesting high-mass X-ray binaries owing to its spatially resolved radio emission and its TeV emission, generally attributed to non-thermal particles in an accretion-powered relativistic jet or in the termination shock of the relativistic wind of a young pulsar. Also, the nature of the compact object is still debated. Only LS 5039 and PSR B1259-63 (which hosts a non-accreting millisecond pulsar) have similar characteristics. We study the X-ray emission from LSI +61 303 covering both short-term and orbital variability. We also investigate the source spectral properties in the soft X-ray (0.3-10 keV) energy range. 25 snapshot observations of LSI +61 303 have been collected in 2006 with the XRT instrument on-board the Swift satellite over a period of four months, corresponding to about five orbital cycles. Since individual data sets have too few counts for a meaningful spectral analysis, we extracted a cumulative spectrum. The count rate folded at the orbital phase shows a clear modulation pattern at the 26.5 days period and suggests that the X-ray peak occurs around phase 0.65. Moreover, the X-ray emission appears to be variable on a timescale of ~1 ks. The cumulative spectrum is well described by an absorbed power-law model, with hydrogen column density Nh=(5.7+/-0.3)E+21 cm^-2 and photon index 1.78+/-0.05. No accretion disk signatures, such as an iron line, are found in the spectrum.Comment: Revised to match the A&A versio

Primary accumulation in the Soviet transition

The Soviet background to the idea of primary socialist accumulation is presented. The mobilisation of labour power and of products into public sector investment from outside are shown to have been the two original forms of the concept. In Soviet primary accumulation the mobilisation of labour power was apparently more decisive than the mobilisation of products. The primary accumulation process had both intended and unintended results. Intended results included bringing most of the economy into the public sector, and industrialisation of the economy as a whole. Unintended results included substantial economic losses, and the proliferation of coercive institutions damaging to attainment of the ultimate goal - the building of a communist society

Long Term X-ray Monitoring Of The TeV Binary LS I +61 303 with RXTE

We report on the results of a long term X-ray monitoring campaign of the galactic binary LS I +61 303 performed by the Rossi X-ray Timing Explorer. This dataset consists of 1 ks pointings taken every other day between 2007 August 28 until 2008 February 2. The observations covered six full cycles of the 26.496 day binary period and constitute the largest continuous X-ray monitoring dataset on LS I +61 303 to date with this sensitivity. There is no statistically strong detection of modulation of flux or photon index with orbital phase; however, we do find a strong correlation between flux and photon index, with the spectrum becoming harder at higher fluxes. The dataset contains three large flaring episodes, the largest of these reaching a flux level of 7.2 (+0.1,-0.2)*10^-11 erg cm^-2 s^-1 in the 3-10 keV band, which is a factor of three times larger than flux levels typically seen in the system. Analysis of these flares shows the X-ray emission from LS I +61 303 changing by up to a factor of six over timescales of several hundred seconds as well as doubling times as fast as 2 seconds. This is the fastest variability ever observed from LS I +61 303 at this wavelength and places constraints on the size of the X-ray emitting region.Comment: 24 pages, 7 figures, 2 tables. Accepted for publication in Ap

Understanding the contribution of metabolism to Mycobacterium tuberculosis drug tolerance

Treatment o