bluuebunny/crossref_metadata_2025_split huggingface dataset:
Masalah Emosi dan Perilaku pada Penderita TB Anak
Authors: Widakdo Giri , Rita Erni , Saputri Indah Noviana , Permatasari Tria Astika Endah , Kurniaty Ika 
Published: September 2020

Masalah emosi dan perilaku terhadap anak merupakan masalah yang cukup serius, salah satunya berdampak terhadap kesehatan jiwa, terlebih bagi anak yang menderita penyakit kronis, diantaranya penyakit TB (Tuberculosis) hingga dapat menyebabkan terganggunya produktivitas serta kualitas hidup termasuk pendidikan anak. Penelitian ini bertujuan untuk mengetahui masalah emosi dan perilaku pada penderita TB anak di Wilayah Puskesmas Jakarta Pusat dan Puskesmas Jakarta Timur.
Desain penelitian ini adalah potong lintang pada 91 penderita TB anak di tahun 2019 yang diukur dengan menggunakan Strength and Dfficulties Questionary (SDQ).
Hasil penelitian menunjukkan bahwa Sebanyak 44% dari seluruh subjek penelitian adalah usia sekolah dengan jenis kelamin laki-laki lebih banyak daripada perempuan. Skor SDQ untuk masalah dan perilaku penderita TB pada anak dengan 3 kelompok usia, yaitu : tingkah laku dengan proporsi abnormal sebesar 75 anak (yang tertinggi pada kelompok usia pra sekolah: 41,5%) dan teman sebaya didapatkan proporsi yang abnormal sebesar 75 anak ( dengan kelompok usia tertinggi pada kelompok usia sekolah: 44%), serta skor kesulitan, proporsi terbesar adalah pada kondisi abnormal, yaitu pada 39 anak (usia sekolah yang terbesar; yakni 40%) . Skor SDQ berdasarkan hubungan masalah dan perilaku penderita TB pada anak dengan jenis kelamin, yaitu : lelaki lebih banyak mengalami masalah hubungan dengan kesulitan (51,2%) , sedangkan anak perempuan lebih banyak mengalami masalah yang berhubungan dengan tingkah laku (57,6%), teman sebaya (53,3%) dan masalah kekuatan/prososial (54,5%). Analisis distribusi skor masalah dan perilaku penderita TB pada anak dengan kovariat ( Status Gizi, Riwayat kontak dan Status TB), yaitu : untuk masalah tingkah laku didapatkan proporsi abnormal terbesar baik terhadap status gizi normal (89,4%), riwayat kontak serumah (57,6%) dan status TB negatif (80,3%) dan untuk masalah hubungan dengan teman sebaya didapatkan proporsi yang abnormal terbesar baik terhadap status gizi normal (92%), riwayat kontak serumah (60%) dan status TB negatif (84%) serta masalah dan perilaku yang berhubungan dengan kesulitan didapatkan proporsi terbesar adalah pada kondisi abnormal baik terhadap status gizi normal (89,9%), riwayat kontak serumah (60%) dan status TB negatif (80%)
Kesimpulan:Penderita TB anak terbanyak adalah laki-laki namun berdasarkan skor SDQ yang abnormal terbesar adalah responden berjenis kelamin perempuan dengan proporsi abnormal terjadi kelompok usia pra sekolah – sekolah, yaitu untuk masalah tingkah laku, hubungan teman sebaya. dan prososial sedangkan laki-laki hanya pada masalah terkait dengan kesulitan dalam bersosialisasi saja. Proporsi terbesar abnormal pada analisis distribusi skor masalah dan perilaku penderita TB pada anak dengan kovariat ( Status Gizi, Riwayat kontak dan Status TB), yaitu : untuk masalah tingkah laku teman sebaya dan skor kesulitan
PENGARUH PERSEPSI KEMANFAATAN DAN PERSEPSI KEMUDAHAN TERHADAP MINAT MASYARAKAT DALAM PENGGUNAAN APLIKASI SISTEM INFORMASI PENGADUAN MASYARAKAT ONLINE (SIKESAL) KOTA JAMBI
Authors: Amalia Indahnur 
Published: September 2020

Abstract
This study aims to determine how the influence of benefits perception and easiness perception of community’s interest in using Application of Online Public Complaint Information System (SIKESAL) in Jambi City. The analytical method used in this study is SEM-PLS with Smart-PLS version 3. The results of this study that community's interest in using the online public complaint information system (SiKESAL) application can be explained by the perception of benefits and easiness perception of 64.6% and the remaining 35.4% was explained by variables outside this study. Then, benefits and easiness perception had effect on the community's interest.
Keywords: SiKESAL application, industrial revolution 4.0, benefits perception, easiness perception, technology.

Abstrak
Penelitian ini bertujuan untuk mengetahui bagaimana pengaruh persepsi kemanfaatan dan persepsi kemudahan terhadap minat masyarakat dalam penggunaan aplikasi system informasi keluhan masyarakat online (SiKESAL) di Kota Jambi. Metode analisis yang digunakan dalam penelitian ini adalah SEM-PLS dengan Smart-PLS versi 3. Hasil penelitian ini menunjukkan bahwa minat masyarakat dalam penggunaan aplikasi system informasi keluhan masyarakat online (SiKESAL) dapat dijelaskan oleh persepsi kemanfaatan dan persepsi kemudahan 64,6% dan sisanya 35,4% dijelaskan oleh variabel di luar penelitian ini. Selanjutnya, persepsi kemanfaatan dan kemudahan memiliki pengaruh terhadap minat masyarakat.
Kata Kunci : Aplikasi SiKESAL, revolusi industri 4.0, persepsi kemanfaatan, persepsi kemudahan, teknologi.
DEVELOPMENT OF STUDENTS WRITING SKILLS AS A STAGE OF PRACTICE-ORIENTED LEARNING AT LAW UNIVERSITY
Authors: Морохова Ольга Александровна 
Published: September 2020

В статье анализируются особенности письменного дискурса в эпоху электронных коммуникаций и задачи развития письменных умений обучающихся в юридическом вузе. Автор статьи показывает, что обучение работе с документами является важным этапом формирования общекультурных и профессиональных компетенций обучающихся.
The article analyzes the features of written discourse in the era of electronic communications and the tasks of developing the written skills of students in a law school. The author of the article shows that learning to work with documents is an important stage in the formation of general cultural and professional competencies of students.
ON THE NEED TO CREATE SCHOOL MEDIATION (RECONCILIATION) SERVICES FOR THE PREVENTION OF CONFLICTS AMONG ADOLESCENTS
Authors: Шарифзянова Кадрия Шяукатовна 
Published: September 2020

В данной статье анализируется проблема возникновения и урегулирования конфликтов среди несовершеннолетних, в том числе и детей находящихся в конфликте с законом. Описано создание школьных служб медиации (примирения), которая ориентирована на конструктивное разрешение конфликтной ситуации.
This article analyzes the problem of the emergence and settlement of conflicts among minors, including children in conflict with the law. The creation of school mediation (reconciliation) services is described, which is focused on constructive resolution of a conflict situation.
ECONOMIC ASPECTS OF WATER TRANSPORT SAFETY
Authors: Марков Владимир Петрович 
Published: September 2020

В связи с нововведениями обостряются существующие проблемы безопасности водного транспорта. Обращается внимание на тот факт, что существующая система безопасности водного транспорта не учитывает географический, технологический и отраслевой факторы. Реализация концепции транспортной безопасности на водном транспорте взывает немало вопросов, определяющих существование отрасли.
In connection with the innovations, the existing problems of the safety of water transport are aggravated. Attention is drawn to the fact that the existing water transport safety system does not take into account geographical, technological and sectoral factors. The implementation of the concept of transport security in water transport raises many questions that determine the existence of the industry.
RESILIENCE OF PHYSICAL EDUCATION TEACHERS AS AN ASPECT OF SOCIAL SECURITY
Authors: Осипова Ирина Сергеевна , Постникова Наталья Ивановна 
Published: September 2020

Цель статьи - на основе анализа научной литературы раскрыть актуальность формирования резильентности у будущих педагогов физической культуры. Резильентность педагога физической культуры рассматривается как опора формирования социальной безопасности.
The purpose of the article is to reveal the relevance of the formation of resilience in future teachers of physical culture. The resilience of a physical culture teacher is considered as a support for the formation of social security.
MEDICINAL PLANTS WITH ANTITUSSIVE AND EXPECTORANT EFFECT GROWING IN THE GARDEN OF MEDICINAL PLANTS OF BURDENKO STATE MEDICAL UNIVERSITY
Authors: Абаполова Ирина Ивановна , Пашков Александр Николаевич , Карташова Наталия Михайловна , Чепрасова Анна Александровна , Парфенова Наталья Владимировна 
Published: September 2020

В данной статье описаны виды коллекции участка лекарственных растений ВГМУ им. Н.Н. Бурденко, обладающие противокашлевым и отхаркивающим эффектом. Приведены сведения об их местообитании и условиях произрастания, а также указаны лечебные свойства.
This article describes the types of medicinal plants collection of VSMU named after N. N. Burdenko, which have antitussive and expectorant effect. Information about their habitat and growing conditions, as well as their medicinal properties has been represented.
OPTIMIZATION OF THE COMPOSITION OF THE AIRPLACE PARK FOR THE UTILIZATION OF THE CITY ROUTE
Authors: Балдин Александр Викторович , Ерошок Иван Дмитриевич 
Published: September 2020

Одной из актуальных задач является определение состава парка автобусов для обслуживания каждого маршрута. При этом необходимо иметь возможность варьировать типом и количеством автобусов, которые имеют различные технические характеристики. Предложены эвристические алгоритмы, которые направлены на выбор состава парка с учетом пассажировместимости потенциально приобретаемых автобусов.
One of the most important tasks is to determine the composition of the bus fleet to serve each route. It is necessary to be able to vary the type and number of buses that have different technical characteristics. Heuristic algorithms are proposed that are aimed at selecting the composition of the fleet, taking into account the passenger capacity of potentially purchased buses.
ANNOUNCEMENT OF THE BOOK MUSLOV S.A., SHELYAKOV A.V., ANDREEV V.A. “ALLOYS WITH SHAPE MEMORY: PROPERTIES, OBTAINING AND APPLICATION IN TECHNIQUE AND MEDICINE”
Authors: Муслов Сергей Александрович , Андреев Владимир Александрович 
Published: September 2020

Совокупность уникальных свойств термомеханической памяти формы (ПФ) и сверхэластичности (СЭ) соединений на основе никелида титана (TiNi), механизм и природа этих явлений до сих пор вызывает несомненный интерес у физиков и инженеров. Данное сообщение посвящено выходу в свет очередной книги, в которой изложены научные аспекты исследований и практического применения интерметаллидов никелида титана в различных аспектах сферы жизнедеятельности человека.
The combination of unique properties of thermomechanical shape memory (SM) and superelasticity (SE) of compounds based on titanium nickelide (TiNi), the mechanism and nature of these phenomena are still of great interest to physicists and engineers. This message is dedicated to the publication of the book, which sets out the scientific aspects of research and the use of titanium nickelide intermetallic compounds in various aspects of human life.
LEXICAL FEATURES OF THE ENGLISH LANGUAGE IN THE LEGAL SPHERE
Authors: Морохова Ольга Александровна 
Published: September 2020

В статье представлены результаты исследования по изучению лексических особенностей английского языка в правовой сфере. Автор статьи показывает, что английский язык является языком международного общения и занимает особое место в формировании международного правового поля. В статье особое внимание уделено анализу международного банка ключевых правовых понятий.
The article presents the results of a research on the study of the lexical features of the English language in the legal sphere. The author of the article shows that English is the language of international communication and occupies a special place in the formation of the legal field. The article pays special attention to the analysis of the international bank of key legal concepts.
Mass Estimation of Galaxy Clusters with Deep Learning. I. Sunyaev–Zel’dovich Effect
Authors: Gupta N. , Reichardt C. L. 
Published: September 2020

Abstract
We present a new application of deep learning to infer the masses of galaxy clusters directly from images of the microwave sky. Effectively, this is a novel approach to determining the scaling relation between a cluster’s Sunyaev–Zel’dovich (SZ) effect signal and mass. The deep-learning algorithm used is mResUNet, which is a modified feed-forward deep-learning algorithm that broadly combines residual learning, convolution layers with different dilation rates, image regression activation, and a U-Net framework. We train and test the deep-learning model using simulated images of the microwave sky that include signals from the cosmic microwave background, dusty and radio galaxies, and instrumental noise as well as the cluster’s own SZ signal. The simulated cluster sample covers the mass range 1 × 1014
M
⊙ < M
200c < 8 × 1014
M
⊙ at z = 0.7. The trained model estimates the cluster masses with a 1σ uncertainty ΔM/M ≤ 0.2, consistent with the input scatter on the SZ signal of 20%. We verify that the model works for realistic SZ profiles even when trained on azimuthally symmetric SZ profiles by using the Magneticum hydrodynamical simulations.
Constraints on Dynamical Dark Energy Models from the Abundance of Massive Galaxies at High Redshifts
Authors: Menci N. , Grazian A. , Castellano M. , Santini P. , Giallongo E. , Lamastra A. , Fortuni F. , Fontana A. , Merlin E. , Wang T. , Elbaz D. , Sanchez N. G. 
Published: September 2020

Abstract
We compare the maximal abundance of massive systems predicted in different dynamical dark energy (DDE) models at high redshifts z ≈ 4–7 with the measured abundance of the most massive galaxies observed to be already in place at such redshifts. The aim is to derive constraints for the evolution of the dark energy equation-of-state parameter w that are complementary to existing probes. We adopt the standard parameterization for the DDE evolution in terms of the local value w
0 and of the lookback time derivative of the equation of state w

a
. We derive constraints on combinations of (w
0, w

a
) in the different DDE models by using three independent probes: (i) the observed stellar mass function of massive objects at z ≥ 6 derived from the CANDELS survey; (ii) the estimated volume density of massive halos derived from the observation of massive, star-forming galaxies detected in the submillimeter range at z ≈ 4; (iii) the rareness of the most massive system (with an estimated gas mass exceeding 3 × 1011
M
⊙) observed to be in place at z ≈ 7, a far-infrared–luminous object recently detected in the South Pole Telescope survey. Finally, we show that the combination of our results from the three above probes excludes a sizable fraction of the DDE parameter space w

a
≳ −3/4 − (w
0 + 3/2) presently allowed (or even favored) by existing probes.
Vanadium Abundance Derivations in 255 Metal-poor Stars*
Authors: Ou 欧 Xiaowei 筱葳 , Roederer Ian U. , Sneden Christopher , Cowan John J. , Lawler James E. , Shectman Stephen A. , Thompson Ian B. 
Published: September 2020

Abstract
We present vanadium (V) abundances for 255 metal-poor stars derived from high-resolution optical spectra from the Magellan Inamori Kyocera Echelle spectrograph on the Magellan Telescopes at Las Campanas Observatory, the Robert G. Tull Coudé Spectrograph on the Harlan J. Smith Telescope at McDonald Observatory, and the High Resolution Spectrograph on the Hobby–Eberly Telescope at McDonald Observatory. We use updated V i and V ii atomic transition data from recent laboratory studies, and we increase the number of lines examined (from one to four lines of V i, and from two to seven lines of V ii). As a result, we reduce the V abundance uncertainties for most stars by more than 20% and expand the number of stars with V detections from 204 to 255. In the metallicity range −4.0 < [Fe/H] < −1.0, we calculate the mean ratios [V i/Fe i] = −0.10 ± 0.01 (σ = 0.16) from 128 stars with ≥2 V i lines detected, [V ii/Fe ii] = +0.13 ± 0.01 (σ = 0.16) from 220 stars with ≥2 V ii lines detected, and [V ii/V i] = +0.25 ± 0.01 (σ = 0.15) from 119 stars. We suspect that this offset is due to departures from local thermodynamic equilibrium, and we recommend using [V ii/Fe ii], which is enhanced relative to the solar ratio, as a better representation of [V/Fe]. We provide more extensive evidence for abundance correlations detected previously among scandium, titanium, and vanadium, and we identify no systematic effects in the analysis that can explain these correlations.
A Diffuse Metal-poor Component of the Sagittarius Stream Revealed by the H3 Survey
Authors: Johnson Benjamin D. , Conroy Charlie , Naidu Rohan P. , Bonaca Ana , Zaritsky Dennis , Ting 丁源 Yuan-Sen 森 , Cargile Phillip A. , Han Jiwon Jesse , Speagle Joshua S. 
Published: September 2020

Abstract
The tidal disruption of the Sagittarius dwarf galaxy has generated a spectacular stream of stars wrapping around the entire Galaxy. We use data from Gaia and the H3 Stellar Spectroscopic Survey to identify

high-quality Sagittarius members based on their angular momenta. The H3 Survey is largely unbiased in metallicity, and so our sample of Sagittarius members is similarly unbiased. Stream stars span a wide range in [Fe/H] from −0.2 to ≈−3.0, with a mean overall metallicity of

. We identify a strong metallicity dependence to the kinematics of the stream members. At [Fe/H] > −0.8 nearly all members belong to the well-known cold (

) leading and trailing arms. At intermediate metallicities (−1.9 < [Fe/H] < −0.8) a significant population (24%) emerges of stars that are kinematically offset from the cold arms. These stars also appear to have hotter kinematics. At the lowest metallicities ([Fe/H] ≲ −2), the majority of stars (69%) belong to this kinematically offset diffuse population. Comparison to simulations suggests that the diffuse component was stripped from the Sagittarius progenitor at earlier epochs, and therefore resided at larger radius on average than the colder metal-rich component. We speculate that this kinematically diffuse, low-metallicity population is the stellar halo of the Sagittarius progenitor system.
On the Velocity Drift between Ions in the Solar Atmosphere
Authors: Martínez-Sykora Juan , Szydlarski Mikolaj , Hansteen Viggo H. , De Pontieu Bart 
Published: September 2020

Abstract
The solar atmosphere is composed of many species, which are populated at different ionization and excitation levels. The upper chromosphere, transition region, and corona are nearly collisionless. Consequently, slippage between, for instance, ions and neutral particles, or interactions between separate species, may play important roles. We have developed a 3D MFMS numerical code (Ebysus) to investigate such effects. Ebysus is capable of treating species (e.g., hydrogen, helium, etc.) and fluids (neutrals, excited and ionized elements) separately, including nonequilibrium ionization, momentum exchange, radiation, thermal conduction, and other complex processes in the solar atmosphere. Treating different species as different fluids leads to drifts between different ions and an electric field that couples these motions. The coupling for two ionized fluids can lead to an anti-phase rotational motion between them. Different ionized species and momentum exchange can dissipate this velocity drift, i.e., convert wave kinetic energy into thermal energy. High-frequency Alfvén waves driven by, e.g., reconnection thought to occur in the solar atmosphere, can drive such multi-ion velocity drifts.
Hydrodynamic Simulations of Pre-supernova Outbursts in Red Supergiants: Asphericity and Mass Loss
Authors: Leung Shing-Chi , Fuller Jim 
Published: September 2020

Abstract
The activity of a massive star approaching core-collapse can strongly affect the appearance of the star and its subsequent supernova. Late-phase convective nuclear burning generates waves that propagate toward the stellar surface, heating the envelope and potentially triggering mass loss. In this work, we improve on previous one-dimensional models by performing two-dimensional simulations of the pre-supernova mass ejection phase due to deposition of wave energy. Beginning with stellar evolutionary models of a 15 M
⊙ red supergiant star during core O-burning, we treat the rate and duration of energy deposition as model parameters and examine the mass-loss dependence and the pre-explosion morphology accordingly. Unlike one-dimensional models, density inversions due to wave heating are smoothed by Rayleigh–Taylor instabilities, and the primary effect of wave heating is to radially expand the star’s hydrogen envelope. For low heating rates with long durations, the expansion is nearly homologous, whereas high but short-lived heating can generate a shock that drives envelope expansion and results in a qualitatively different density profile at the time of core-collapse. Asymmetries are fairly small, and large amounts of mass loss are unlikely unless the wave heating exceeds expectations. We discuss implications for pre-supernova stellar variability and supernovae light curves.
Carbon Isotope Ratios in Planetary Nebulae: The Unexpected Enhancement of 13C
Authors: Ziurys L. M. , Schmidt D. R. , Woolf N. J. 
Published: September 2020

Abstract
The 12C/13C ratio has been measured toward a sample of planetary nebulae (PNe) using millimeter observations of CO, HCN, HNC, CN, and other species, conducted with the 12 m antenna and the Submillimeter Telescope of the Arizona Radio Observatory. The observed nebulae spanned the entire lifetime of PNe, from ∼900 to 12,000 yr, and include well-known objects such as NGC 7293 (Helix), NGC 6720 (Ring), and NGC 2440, as well as relatively unexplored nebulae (M3–28, M2–48, and M3–55). In most cases, multiple molecules and transitions were used in the ratio determination, resulting in the most accurate values available to date, with 10%–40% uncertainties. The ratios found were unexpectedly low, lying in the range 12C/13C ∼1.0 ± 0.7–13.2 ± 4.9, with an average value of 3.7—drastically less than found in the envelopes of C-rich AGB stars, and, in some cases, lower than the minimum value achieved in equilibrium CNO burning. Such low values are expected for the two O-rich nebulae studied (M2–9 and M2–48), because of insufficient third dredge-up events. However, most of the PNe observed were clearly carbon-rich, as deduced from the large number of C-bearing molecules present in them. Because nucleosynthesis ceases in the PN stage, both the C/O and the 12C/13C ratios must reflect abundances at the end of the AGB. These consistently low 12C/13C ratios, combined with the bipolar/multipolar morphologies of all planetary nebulae observed, suggest an explosive process involving proton-capture occurred at the AGB–PN transition.