The impact of balance training on balance, confidence, and functionality in assisted living adults.

Assisted living adults are at a great risk for falls, which can negatively impact their life. Confidence may be related to balance, as older adults may discontinue physical activity due to a fear of falling. Balance training may mitigate the prevalence of falls and increase confidence. The purpose of this study was to determine the effects of a balance training program on balance, confidence, and functionality in assisted living older adults. Recruiting was done at two different retirement communities. The control group (n=4) was conducted at one facility. Participants completed stretches for each muscle group on an ergonomic disk 45 minutes a day, twice a week for eight weeks. The intervention group (n=5) completed a warm-up, strength training for the upper and lower body, balance training and a cool down for 45 minutes. The Berg Balance Scale (BBS) and 8-foot-up-and-go (UPGO) were used to measure balance. The KATZ ADL and chair stand (CS) were utilized to measure functionality. The Modified Falls Efficacy Scale (MFES) and Balance Efficacy Scale (BES) examined confidence. A repeated measures ANOVA was conducted to analyze results. The intervention group experienced a significant improvement in balance on the BBS (p=.006) from 40??3.39 points to 47.6??2.88 points. No other significant improvements were seen. However, large effect sizes were seen in the control group on the BES (d=1.026), UPGO (d=1.301), and MFES(d=.088). The intervention group possessed large effect sizes on the BBS (d=2.24) and moderate effect sizes on the MFES (d=0.51) and CS (d=0.46). Researchers concluded that confidence may be improved by any increase in physical activity, but a balance training program may be most effective in improving balance. Future research should focus on a comparison of groups participating in no physical activity and those doing a comprehensive program to include walking, strength training, and balance

Effect of school-based interventions on attention and academic performance of primary schoolchildren from lower socioeconomic communities in Port Elizabeth

Health benefits associated with regular physical activity (PA) have been widely established. Regular PA is not only associated with improved physical and psychological well-being, but also with improved brain function and cognition, thereby enhancing academic performance (AP). Despite these benefits, decreasing levels of PA and increasing levels of overweight and obesity exist world-wide, making childhood physical inactivity a global concern. Research suggests children who meet the recommended PA guidelines of 60-minutes of moderate-to-vigorous intensity attain substantially higher academic grades. Schools provide ideal settings for PA promotion due to the substantial amount of time children spend at school. However, in many countries, including South Africa (SA), Physical Education (PE) programmes have been reduced and replaced with other subjects to increase AP. Furthermore, a scarcity of water, limited accessibility to improved sanitation and lack of personal hygiene at home and in school substantially contributes to the burden of preventable childhood diseases. These hygiene-related illnesses augment the cycle of poverty and disease through its detrimental effect on children’s school attendance, academic performance and productivity. Studies also show that obesity, poor nutrition and food insufficiency affect children’s school achievement. Hence, the school environment plays an essential role in improving children’s health, since many teaching opportunities about important health and nutrition practices are provided. The primary aim of this study was to determine the effect of various combinations of school-based interventions on the attention and AP of primary schoolchildren from disadvantaged communities in Port Elizabeth. Overall, 857 schoolchildren (n = 434 boys and n = 423 girls, aged 8 – 13 years) participated in the study. A 10-week cluster randomised controlled trial using four experimental and four control schools was conducted. Setting-specific interventions incorporated PA, health and hygiene education and nutrition components. The d2 Test of Attention measured selective visual attention and concentration with outcome measures of the percentage of errors, total performance and concentration performance. End of year school results were used to assess AP. Post-intervention and pre- to post-intervention differences between the inter-school comparisons revealed mixed results for the attention and AP measurements, therefore, no conclusions could be drawn regarding the assessed variables. Intervention group comparisons at post-intervention indicated that the PA intervention group achieved a statistically significant improvement (p 0.8) for AP, when compared with the non-PA intervention group. No significant differences were found for AP in relation to intervention group comparisons for the health and hygiene education and nutrition intervention groups. Similarly, the intervention group comparisons revealed no significant differences regarding attention for post-intervention and pre- to post-intervention differences. Findings suggest that a school-based PA intervention can positively affect children’s AP. The current study emphasises the necessity of PA and reinforces the importance of PE in the school curriculum. Therefore, it is strongly recommended that PE regains its rightful place and be actively taught within the school curriculum

Search for L5 Earth Trojans with DECam

Most of the major planets in the Solar system support populations of co-orbiting bodies, known as Trojans, at their L4 and L5 Lagrange points. In contrast, Earth has only one known co-orbiting companion. This paper presents the results from a search for Earth Trojans (ETs) using the DECam instrument on the Blanco Telescope at CTIO. This search found no additional Trojans in spite of greater coverage compared to previous surveys of the L5 point. Therefore, the main result of this work is to place the most stringent constraints to date on the population of ETs. These constraints depend on assumptions regarding the underlying population properties, especially the slope of the magnitude distribution (which in turn depends on the size and albedo distributions of the objects). For standard assumptions, we calculate upper limits to a 90 per cent confidence limit on the L5 population of N_(ET) < 1 for magnitude H < 15.5, N_(ET) = 60–85 for H < 19.7, and N_(ET) = 97 for H = 20.4. This latter magnitude limit corresponds to Trojans ∼300 m in size for albedo 0.15. At H = 19.7, these upper limits are consistent with previous L4 ET constraints and significantly improve L5 constraints

Detection of Diatomic Carbon in 2I/Borisov

2I/Borisov is the first-ever observed interstellar comet (and the second detected interstellar object (ISO)). It was discovered on 2019 August 30 and has a heliocentric orbital eccentricity of ~3.35, corresponding to a hyperbolic orbit that is unbound to the Sun. Given that it is an ISO, it is of interest to compare its properties—such as composition and activity—with the comets in our solar system. This study reports low-resolution optical spectra of 2I/Borisov. The spectra were obtained by the MDM Observatory Hiltner 2.4 m telescope/Ohio State Multi-Object Spectrograph (on 2019 October 31.5 and November 4.5, UT). The wavelength coverage spanned from 3700 to 9200 Å. The dust continuum reflectance spectra of 2I/Borisov show that the spectral slope is steeper in the blue end of the spectrum (compared to the red). The spectra of 2I/Borisov clearly show CN emission at 3880 Å, as well as C2 emission at both 4750 and 5150 Å. Using a Haser model to covert the observed fluxes into estimates for the molecular production rates, we find Q(CN) = 2.4 ± 0.2 × 10²⁴ s⁻¹, and Q(C₂) = (5.5 ± 0.4) × 10²³ s⁻¹ at the heliocentric distance of 2.145 au. Our Q(CN) estimate is consistent with contemporaneous observations, and the Q(C₂) estimate is generally below the upper limits of previous studies. We derived the ratio Q(C₂)/Q(CN) = 0.2 ± 0.1, which indicates that 2I/Borisov is depleted in carbon-chain species, but is not empty. This feature is not rare for the comets in our solar system, especially in the class of Jupiter-family comets

Photometric Survey of Neptune's Trojan Asteroids I: The Color Distribution

In 2018, Jewitt identified the "The Trojan Color Conundrum", namely that Neptune's Trojan asteroids (NTs) had no ultra-red members, unlike the the nearby Kuiper Belt. Since then, numerous ultra-red NTs have been discovered, seemingly resolving this conundrum (Lin et al. 2019; Bolin et al.12 2023). However, it is still unclear whether or not the Kuiper Belt has a color distribution consistent with the NT population, as would be expected if it were the source population. In this work, we present a new photometric survey of 15 out of 31 NTs. We utilized the Sloan g'r'i'z' filters on the IMACS f/4 instrument which is mounted on the 6.5m Baade telescope. In this survey, we identify four NTs as being ultra-red using a Principal Component Analysis (PCA). This result brings the ratio of red to ultra-red NTs to 7.75:1, more consistent with the corresponding Trans-Neptunian Object (TNO) ratio of 4-11:1. We also identify three targets as being blue (nearly Solar) in color. Such objects may be C-type surfaces, but we see more of these blue NTs than has been observed in the Kuiper Belt (Seccull et al. 2018). Finally, we show that there are hints of a color-absolute magnitude (H) correlation, with larger H (smaller sized, lower albedo) tending to be more red, but more data is needed to confirm this result. The origin of such a correlation remains an open question which will be addressed by future observations of the surface composition of these targets and their rotational properties.Comment: 15 pages, 8 figures, accepted to PS

Environmental Policy Update 2012: Development Strategies and Environmental Policy in East Africa

The seven chapters that comprise this report explore ways to integrate sustainability goals and objectives into Ethiopia's current development strategies

O ATO PERFORMÁTICO COMO ESTRATÉGIA DE LUTA DAS MULHERES

Este trabalho apresenta algumas reflexões sobre o feminismo contemporâneo a partir da análise de um ato performático realizado por estudantes brasileiras, em junho de 2016, com o objetivo de contestar e repudiar a violência sexual sofrida por uma jovem que foi estuprada por um grupo de homens no Rio de Janeiro. A violência, amplamente divulgada pela mídia brasileira, provocou manifestações de ordens variadas em diferentes segmentos sociais. A performance apresentada neste estudo estabelece uma estreita relação com o corpo feminino que se torna uma ferramenta de luta e reivindicação.Palavras-chave: Performance. Mulheres. Violência. Luta.-----------------------------------------------------------THE PERFORMATING ACT AS A WOMEN'S STRATEGY FOR FIGHTINGThis paper presents some reflections on contemporary feminism from the analysis of a performative act performed by Brazilian students, in June 2016, in order to contest and repudiate the sexual violence suffered by a teenager in Rio de Janeiro, who was raped by a group of men. The violence widely reported by the Brazilian media caused manifestations of different orders in different social segments. The performance presented in this study establishes a close relation with the female body, which becomes a tool of struggle and social claim.Keywords: Performance. Women. Violence. Fight

Search for L5 Earth Trojans with DECam

Most of the major planets in the Solar system support populations of co-orbiting bodies, known as Trojans, at their L4 and L5 Lagrange points. In contrast, Earth has only one known co-orbiting companion. This paper presents the results from a search for Earth Trojans (ETs) using the DECam instrument on the Blanco Telescope at CTIO. This search found no additional Trojans in spite of greater coverage compared to previous surveys of the L5 point. Therefore, the main result of this work is to place the most stringent constraints to date on the population of ETs. These constraints depend on assumptions regarding the underlying population properties, especially the slope of the magnitude distribution (which in turn depends on the size and albedo distributions of the objects). For standard assumptions, we calculate upper limits to a 90 per cent confidence limit on the L5 population of N_(ET) < 1 for magnitude H < 15.5, N_(ET) = 60–85 for H < 19.7, and N_(ET) = 97 for H = 20.4. This latter magnitude limit corresponds to Trojans ∼300 m in size for albedo 0.15. At H = 19.7, these upper limits are consistent with previous L4 ET constraints and significantly improve L5 constraints

Search for L5 Earth Trojans with DECam

Most of the major planets in the Solar System support populations of co-orbiting bodies, known as Trojans, at their L4 and L5 Lagrange points. In contrast, Earth has only one known co-orbiting companion. This paper presents the results from a search for Earth Trojans using the DECam instrument on the Blanco Telescope at CTIO. This search found no additional Trojans in spite of greater coverage compared to previous surveys of the L5 point. Therefore, the main result of this work is to place the most stringent constraints to date on the population of Earth Trojans. These constraints depend on assumptions regarding the underlying population properties, especially the slope of the magnitude distribution (which in turn depends on the size and albedo distributions of the objects). For standard assumptions, we calculate upper limits to a 90% confidence limit on the L5 population of $N_{ET}<1$ for magnitude $H<15.5$, $N_{ET}=60-85$ for $H<19.7$, and $N_{ET}\$= 97 for $H=20.4$. This latter magnitude limit corresponds to Trojans $\sim$300 m in size for albedo $0.15$. At H=19.7, these upper limits are consistent with previous L4 Earth Trojan constraints and significantly improve L5 constraints.Comment: 17 pages, 12 figures, Accepted to MNRA