bluuebunny/crossref_metadata_2025_split huggingface dataset:
Peningkatan Ketahanan Pangan Bagi Masyarakat Terdampak Covid-19
Authors: Andini Lidia , Prajogo Uke , Bunyamin Bunyamin , Munfaqiroh Siti , Muslichah Muslichah , Ratnasari Siwi dyah , Haji Son , Sunarto Sunarto , Syadeli M , Sugiono Djoko , Rahmania Benita 
Published: July 2022

Tujuan Kegiatan Pengabdian Kepada Masyarakat: 1) Meningkatkan ketersediaan pangan bagi masyarakat terdampak Covid-19, 2) Memberikan pengetahuan dan ketrampilan kepada pengelola Pondok Pesantren El-Jasmeen mengenai teknik budidaya sayur di dalam pot secara organik, 3) Memberikan pengetahuan dan ketrampilan mengenai teknik pascapanen pengolahan sayur menjadi produk olahan yang bernilai ekonomi tinggi. Hasilnya, pengetahuan dan keterampilan pengelola mengenai teknik budidaya sayur dalam pot dan pascapanennya mengalami peningkatan. Pengelola Pondok Pesantren El-Jasmeen dapat membudidayakan tanaman sayur secara baik dan mampu mengolahnya menjadi produk olahan es krim sayur yang enak dan bernilai ekonomi tinggi. Kegiatan pengabdian kepada masyarakat ini berdampak kepada ketahanan pangan dan peningkatan taraf ekonomi masyarakat di era pandemi Covid-19 karena dapat dikembangkan menjadi usaha skala rumah tangga.
Design of an ultra-sensitive and miniaturized diamond NV magnetometer based on a nanocavity structure
Authors: Katsumi Ryota , Sekino Masaki , Yatsui Takashi 
Published: July 2022

Abstract
The ensemble of nitrogen-vacancy (NV) centers in diamond allows for the potential realization of the sensitive magnetometers by leveraging their excellent spin properties. However, the NV-based magnetometers are limited by their experimental magnetic field sensitivity owing to its inefficient photon collection. Moreover, they are a disadvantage to the reduced spatial resolution and excessive excitation power. To overcome these issues, we propose a ultra-sensitive diamond magnetometer based on nanocavities. The device structure can attain a high collective efficiency and enhance the photon emission intensity of the NV ensemble. This device can allow the efficient photon collection even when considering the positional distribution of the NV centers. Our theoretical analysis indicates that the minimum expected sensitivity is 60 fT/

H
z

.

The proposed design can achieve a volume-normalized sensitivity of 0.92 aT/

H
z

c

m

−
3

along with the required power of 7 μW, both of which are superior to those of bulk diamond. The proposed approach offers a promising route towards highly sensitive and energy-efficient magnetometers.
Thermoelectric properties of composition-controlled Fe2TiSi-based full-Heusler thin films
Authors: Kurosaki Yosuke , Yabuuchi Shin , Nishide Akinori , Fukatani Naoto , Hayakawa Jun 
Published: July 2022

Abstract
Fe2TiSi full-Heusler thin films were synthesized with a homogeneous single-phase structure and the composition was controlled in a wide range by deposition techniques. By detailed tuning of the film composition, the Seebeck coefficient reached −184 μV K−1, which is almost the maximum for the full-Heusler alloys, with a power factor of 3.9 mW K−2 m−1. The thermal conductivity was 3.5 W K−1 m−1 and first-principles calculations clarified that this small value may be due to alloy scatterings. Consequently, ZT reached 0.36 at room temperature without any heavy element doping, indicating that Fe2TiSi is one of the promising thermoelectric materials.
Measuring Determinants of Time Deposit in The Commercial Banks in Nepal
Authors: Bista Raghu Bir , Basnet Priyanka 
Published: July 2022

Time deposit is one of major source of liquidity of the commercial bank to maintain money supply to the demand of business and household sector. In this context, an interesting query is the determinants of time deposit. This paper measures the determinants of time deposit in the commercial banks of Nepal based on 15 years’ time series data sets from 2000-01 to 2017-18 of the sample commercial banks published by the central bank of Nepal. Using descriptive statistics and multiple regression models as the analytical tools, the paper has found fluctuating trend of liquidity in the commercial banks but inclining trend of external and internal variables including GDP, Deposit, Capital, Size of Bank, remittance and public debt. In this trend, the liquidity of the commercial banks depends significantly on time deposit and remittance inflow. Besides, the positive trend of time deposit from 1994-95 to 2017-18 has caused the positive trend of total deposit from 1994-95 to 2017-18. Additionally, the paper has found that GDP per capita, US exchange rate, interest rate and the branch of the bank are positively and significantly determinants to the time deposit of the commercial bank but inflation rate is negatively and determinant with significance. The internal variables are more determinants than the external variables to the time deposits. It is clear that time deposit is a reliable and long-term source to main the bank liquidity of the commercial bank for their financial stability and performance depends on more the internal variables than the external variables. Therefore, the commercial bank should reform as mentioned in the monetary policy and money market dynamics to improve the competitiveness and smartness of bank policy including interest rate policy and branch of the commercial banks for effective mobilization of the scattered small resources all over the country for higher rate of capital formation, investment, and economic growth
ЗАБЕЗПЕЧЕННЯ ЯКОСТІ ПІДГОТОВКИ ДОКТОРІВ ФІЛОСОФІЇ ЗА СПЕЦІАЛЬНІСТЮ «011 ОСВІТНІ, ПЕДАГОГІЧНІ НАУКИ» В ІНСТИТУТІ ВИЩОЇ ОСВІТИ НАПН УКРАЇНИ
Authors: Kalashnikova Svitlana , Skyba Yurii , Slyusarenko Olena , Talanova Zhanneta 
Published: July 2022

У доповіді представлено інформацію про забезпечення якості підготовки докторів філософії за спеціальністю «011 Освітні, педагогічні науки» в Інституті вищої освіти Національної академії педагогічних наук України. Показано вплив системи внутрішнього забезпечення якості вищої освіти на якість підготовки докторів філософії в Інституті вищої освіти НАПН України. Наголошено, що якість підготовки забезпечується системою внутрішнього забезпечення якості вищої освіти, її моніторингом, актуальністю змісту навчальних дисциплін, високою кваліфікацією кадрів, спрямуванням істотних фінансових ресурсів в освітній процес, низкою необхідних організаційних заходів і процедур, зокрема міжнародних. Зазначено, що кожну освітньо-наукову програму Інституту Національне агентство із забезпечення якості вищої освіти у 2021 р. акредитувало з визначенням «зразкова».
New Photometric Calibration of the Wide Field Camera 3 Detectors
Authors: Calamida Annalisa , Bajaj Varun , Mack Jennifer , Marinelli Mariarosa , Medina Jennifer , Pidgeon Aidan , Kozhurina-Platais Vera , Shanahan Clare , Som Debopam 
Published: July 2022

Abstract
We present a new photometric calibration of the WFC3-UVIS and WFC3-IR detectors based on observations collected from 2009 to 2020 for four white dwarfs—namely, GRW +70 5824, GD 153 , GD 71 , G191B2B—and a G-type star, P330E. These calibrations include recent updates to the Hubble Space Telescope primary standard white dwarf models and a new reference flux for Vega. Time-dependent inverse sensitivities for the two WFC3-UVIS chips, UVIS1 and UVIS2, were calculated for all 42 full-frame filters after accounting for temporal changes in the observed count rates with respect to a reference epoch in 2009. We also derived new encircled energy values for a few filters and improved sensitivity ratios for the two WFC3-UVIS chips by correcting for sensitivity changes with time. Updated inverse sensitivity values for the 20 WFC3-UVIS quad filters and 15 WFC3-IR filters were derived by using the new models for the primary standards, the new Vega reference flux, and, in the case of the IR detector, new flat fields. However, these values do not account for any sensitivity changes with time. The new calibration provides a photometric internal precision better than 0.5% for the wide-, medium-, and narrowband WFC3-UVIS filters; 5% for the quad filters; and 1% for the WFC3-IR filters. As of 2020 October 15, an updated set of photometric keywords were populated in the WFC3 image headers.
Evaluating the Evidence for Water World Populations Using Mixture Models
Authors: Neil Andrew R. , Liston Jessica , Rogers Leslie A. 
Published: July 2022

Abstract
Water worlds have been hypothesized as an alternative to photoevaporation in order to explain the gap in the radius distribution of Kepler exoplanets. We explore water worlds within the framework of a joint mass–radius–period distribution of planets fit to a sample of transiting Kepler exoplanets, a subset of which have radial velocity mass measurements. We employ hierarchical Bayesian modeling to create a range of ten mixture models that include multiple compositional subpopulations of exoplanets. We model these subpopulations—including planets with gaseous envelopes, evaporated rocky cores, evaporated icy cores, intrinsically rocky planets, and intrinsically icy planets—in different combinations in order to assess which combinations are most favored by the data. Using cross-validation, we evaluate the support for models that include planets with icy compositions compared to the support for models that do not, finding broad support for both. We find significant population-level degeneracies between subpopulations of water worlds and planets with primordial envelopes. Among models that include one or more icy-core subpopulations, we find a wide range for the fraction of planets with icy compositions, with a rough upper limit of 50%. Improved data sets or alternative modeling approaches may be able to better distinguish between these subpopulations of planets.
Climate Outcomes of Earth-similar Worlds as a Function of Obliquity and Rotation Rate
Authors: He Feng , Merrelli Aronne , L’Ecuyer Tristan S. , Turnbull Margaret C. 
Published: July 2022

Abstract
A set of simulations with a 3D global climate model are performed to investigate the roles of obliquity and rotation period in the habitability of Earthlike exoplanets. The simulations cover the obliquity–rotation parameter space, from 0° to 90° in obliquity and 1–128 days in rotation period. The simulated global mean temperatures are warmest at 45° obliquity with fast rotations, due to the modification of the greenhouse effect from the spatial redistribution of clouds and water vapor. The slow-moving insolation–cloud mechanism, previously found in simulations with slow rotations and zero obliquity, also produces a cooling trend from intermediate obliquity to high obliquity, with the coldest climate occurring at 90° obliquity for all rotation periods. At low obliquities and fast rotation, persistent snow and sea ice can form, producing cooler temperatures. A Climate Habitability metric is defined, based on temperature and precipitation, which compares well with observations when applied to a simulation using Earth’s obliquity and rotation. Over a wider range of obliquity and rotation period, the Climate Habitability ranges from 10% to 70% of the terrestrial area. Overall, the simulated global mean surface temperature shows a much larger spread across the range of simulated rotation periods at 45° obliquity compared to 0° obliquity. Therefore, we conclude that 3D exoplanet simulations using intermediate obliquities (e.g., 45°) instead of 0° will reveal a wider range of possible climate conditions for specific orbital configurations. In addition, Earth’s climate habitability can increase by 25% if the obliquity increases from 23.°5 to 45°.
Inferring the Thermal History of the Intergalactic Medium from the Properties of the Hydrogen and Helium Lyα Forest
Authors: Villasenor Bruno , Robertson Brant , Madau Piero , Schneider Evan 
Published: July 2022

Abstract
The filamentary network of intergalactic medium (IGM) gas that gives origin to the Lyα forest in the spectra of distant quasars encodes information on the physics of structure formation and the early thermodynamics of diffuse baryonic material. Here we use a massive suite of more than 400 high-resolution cosmological hydrodynamical simulations run with the Graphics Processing Unit–accelerated code Cholla to study the IGM at high spatial resolution maintained over the entire computational volume. The simulations capture a wide range of possible IGM thermal histories by varying the photoheating and photoionizing background produced by star-forming galaxies and active galactic nuclei. A statistical comparison of synthetic spectra with the observed 1D flux power spectra of hydrogen at redshifts 2.2 ≤ z ≤ 5.0 and with the helium Lyα opacity at redshifts 2.4 < z < 2.9 tightly constrains the photoionization and photoheating history of the IGM. By leveraging the constraining power of the available Lyα forest data to break model degeneracies, we find that the IGM experienced two main reheating events over 1.2 Gyr of cosmic time. For our best-fit model, hydrogen reionization completes by z

R
≈ 6.0 with a first IGM temperature peak of T
0 ≃ 1.3 × 104 K and is followed by the reionization of He ii that completes by z
R ≈ 3.0 and yields a second temperature peak of T
0 ≃ 1.4 × 104 K. We discuss how our results can be used to obtain information on the timing and the sources of hydrogen and helium reionization.
MHD Turbulent Power Anisotropy in the Inner Heliosphere
Authors: Adhikari L. , Zank G. P. , Zhao L.-L. , Telloni D. 
Published: July 2022

Abstract
We study anisotropic magnetohydrodynamic (MHD) turbulence in the slow solar wind measured by Parker Solar Probe (PSP) and Solar Orbiter (SolO) during its first orbit from the perspective of variance anisotropy and correlation anisotropy. We use the Belcher & Davis approach (M1) and a new method (M2) that decomposes a fluctuating vector into parallel and perpendicular fluctuating vectors. M1 and M2 calculate the transverse and parallel turbulence components relative to the mean magnetic field direction. The parallel turbulence component is regarded as compressible turbulence, and the transverse turbulence component as incompressible turbulence, which can be either Alfvénic or 2D. The transverse turbulence energy is calculated from M1 and M2, and the transverse correlation length from M2. We obtain the 2D and slab turbulence energy and the corresponding correlation lengths from those transverse turbulence components that satisfy an angle between the mean solar wind flow speed and mean magnetic field θ
UB of either (i) 65° < θ
UB < 115° or (ii) 0° < θ
UB < 25° (155° < θ
UB < 180°), respectively. We find that the 2D turbulence component is not typically observed by PSP near perihelion, but the 2D component dominates turbulence in the inner heliosphere. We compare the detailed theoretical results of a nearly incompressible MHD turbulence transport model with the observed results of PSP and SolO measurements, finding good agreement between them.
Formation of Episodic Jets and Associated Flares from Black Hole Accretion Systems
Authors: Čemeljić Miljenko , Yang Hai , Yuan Feng , Shang Hsien 
Published: July 2022

Abstract
Episodic ejections of blobs (episodic jets) are widely observed in black hole sources and usually associated with flares. In this paper, by performing and analyzing three-dimensional general relativity magnetohydrodynamical numerical simulations of accretion flows, we investigate their physical mechanisms. We find that magnetic reconnection occurs in the accretion flow, likely due to the turbulent motion and differential rotation of the accretion flow, resulting in flares and formation of flux ropes. Flux ropes formed inside of 10–15 gravitational radii are found to mainly stay within the accretion flow, while flux ropes formed beyond this radius are ejected outward by magnetic forces and form the episodic jets. These results confirm the basic scenario proposed in Yuan et al. Moreover, our simulations find that the predicted velocity of the ejected blobs is in good consistency with observations of Sgr A*, M81, and M87. All of the processes were found to occur quasiperiodically, with the period being the orbital time at the radius where the flux rope is formed. The predicted period of the flares and ejections is consistent with those found from the light curves or image of Sgr A*, M87, and PKS 1510–089. The possible applications to protostellar accretion systems are discussed.
Nutritional Intake Education by Peers, Nutritionists, and Combinations to Changes in Nutritional Status in Adolescent Girl in School
Authors: Christiany Irine , Mu’afiro Adin , Waluyo Kiaonarni Ongko , Suparji Suparji 
Published: July 2022

Background: Adolescents pay such close attention to their physical shape and frequently construct their own body image. Low knowledge of nutrients will have an impact on attitudes and behavior related to nutritional status in adolescents. Nutrition education can also help youth gain adolescents' knowledge. Peers are believed to be very influential as educators, so, peer nutritional education in adolescents will be felt positively and have a very significant impact on nutritional status. Aims: This study aims to determine the effect of nutrition education conducted by peers, nutrition, and a combination on the nutritional status of adolescents. Methods and Material: This research used is a quasi-experimental design using a pretest-posttest control group design.The sample consisted of 120 students with an age range of 15–18 years, selected by random sampling. Nutrition education is provided by means of lectures and discussions by peers, nutritionists, or a combination of the two for 1 meeting a week. Statistical analysis used: This study will use the paired t test. Results: The findings revealed that nutrition education delivered by peers had a p value of 0.033 and nutrition education delivered by nutritionists had a p value of 0.003, but there was no significant effect on adolescent nutritional status when nutrition education was delivered in combination with a p value of 0.317. Nutrition education provided by peers is very useful for improving the nutritional status of adolescents. Conclusions: Nutritional education provided by peers is proven to be able to have a positive impact on adolescents because peers are the axis of youth association, so that what is shared and learned by peers will be more easily accepted.
Psycho-Religious Therapy improving the Quality of Life of the Elderly in Nursing Homes
Authors: Setiowati Dwi , Maudina Shova , Jamaludin Jamaludin , Rasdiyanah Rasdiyanah 
Published: July 2022

Abstract
BACKGROUND As people get older, body functions in the elderly will decrease so that it will affect their quality of life. One way to improve the quality of life of the elderly is to meet the basic needs of the elderly through a spiritual approach (Islamic psychotherapy).

AIM: This study aims to determine the effect of Zikr on the quality of life of the elderly in nursing homes.

METHODS: This study used a quasi-experimental nonequivalent control group design. The sampling technique used purposive sampling , a total of 10 respondents from the intervention group and 10 respondents from the control group. Quality of life score using the World Health Organization Quality of Life-BREF questionnaire (WHOQOL-BREF). The research analysis used paired t-test and Wilcoxon test for differences in quality-of-life scores of each group and for differences in quality of life between the intervention group and control group using unpaired t-test and Mann-Whitney test.

RESULTS: The effect of psycho-religious therapy (Zikr) on the quality of life of the elderly in the intervention group before and after doing Zikr (p = 0.000), there were differences in 3 domains of quality of life, namely the psychological domain ( p = 0.000), the domain of social relations (p = 0.027), and the environmental domain. p = 0.010).

CONCLUSION: Psycho-religious therapy (Zikr) affects the quality of life of the elderly in the nursing home and suggests Nursing homes to provide guidance with a religious approach, especially Zikr to improve the quality of life of the elderly.
Apprendre à faire genre
Authors: Beaubatie Emmanuel 
Published: July 2022

Dans les services publics, les consignes se multiplient pour assurer un accueil adapté aux usagers·ères trans. Mais qu’en est-il concrètement pour les personnes concernées ? Cet article présente une analyse statistique de leurs déclarations de discriminations administratives, ainsi qu’une étude qualitative de leurs vécus et de leurs stratégies face à de tels épisodes. Les jeunes sont particulièrement touché·e·s – quantitativement mais aussi et surtout subjectivement – par les discriminations. Après en avoir fait leurs premières expériences, ils et elles tendent à s’engager dans un apprentissage tactique visant à composer avec les catégories et normes de genre des services publics. Au fil de la vie, les individus sont ainsi amené·e·s, ne serait-ce que par stratégie, à apprendre à se montrer conformes et respectables.
Analisis Diversifikasi, Merger, dan Akuisis Perusahaan
Authors: Warti Risma , Dara Audina Dea , Azizi Adelia 
Published: July 2022

This research aims to analyze the diversification, mergers and acquisitions of manufacturing companies in Indonesia. The research method used is descriptive qualitative analysis with a literature study approach. The results show that the diversification analysis was developed with various objectives including increasing growth when the existing market/product has reached a maturity stage, maintaining stability by spreading the risk of profit fluctuations, increasing credibility in the capital market, to avoid dependence on a single item or product in circulation. in the market, fulfill the wishes of unsatisfied consumers, increase the attractiveness or interest of consumers, increase sales turnover, increase profits by using the same ingredients, and prevent consumer boredom.
Keywords: Diversification, Mergers, and Company Acquisitions.
O IMAGINÁRIO ORIENTALISTA NOS RELATOS DE VIAGEM DE PABLO NERUDA
Authors: Loureiro Isabela Roque , Azevedo Suzana de Carvalho Barroso , Dazzi Camila Carneiro 
Published: July 2022

Este artigo propõe-se a investigar os relatos de viagem do escritor chileno Pablo Neruda no início do século XX, quando vivencia sua carreira diplomática no exterior. Nosso objetivo é analisar esses textos buscando identificar as (des) continuidades de um Oriente místico, exótico e pitoresco, fruto de um imaginário construído no século XIX, sobretudo pela arte e pela literatura. Para tanto, valemo-nos de conceitos como imaginário, definido como um acervo coletivo de sentidos que motiva a ação, bem como do entendimento de relato de viagem como um gênero subjetivo, impressionista e de natureza, muitas vezes, política. As análises apontam para uma percepção híbrida e não idealizada de Neruda em relação ao Oriente, composta por construções orientalistas de singular beleza assim como por uma visão negativa, possivelmente derivada de sua experiência como um cidadão de um país que também teve a história marcada pelo processo de colonização. Dessa maneira, os relatos nerudianos transgridem a lógica hegemônica não só por terem sido escritos por um viajante de origem não europeia, mas também por subverterem um imaginário colonial sobre o Oriente, construído em um contexto de dominação violenta.