bluuebunny/crossref_metadata_2025_split huggingface dataset:
Penyuluhan Kesehatan : Panduan Penggunaan Obat Tradisional yang Benar dan Aman
Authors: Wahyu Tusi Wardani  
Published: February 2021

Indonesian people still believe in traditional medicine. This can be seen from the number of sellers of various traditional medicine products on the market. Meanwhile, the current healthy lifestyle has led people to return using products derived from nature. Therefore, traditional medicine can be one of the treatment options. Through this community service activity, it is hoped that there will be an increase in public knowledge about how to use traditional medicines properly and safely and that people can self-medicate traditional medicines properly and rationally. The methods were lecture and discussion. The participants of health counseling consisted of members of Baiturrahman Mosque recitation and visitors of Islamic Book Fair exhibition. This activity was held on Saturday, August 3, 2019. 09.00 - 11.30. The venue for the main stage of the Islamic Book Fair, Yogyakarta State University Sports Hall. Participants who attended were 61 people. Participants were quite enthusiastic during the question and answer time, because it was related to the experience of using traditional medicine. Before the speaker starts delivering the material, the speaker first asks the participants about the habits of using traditional medicine. It turns out that there are still some habits that are not in accordance with the guidelines for the correct and safe use of traditional medicine. In the discussion session, it was seen that the participants had increased their knowledge about how to use traditional medicines correctly and safely. They become more careful in consuming traditional medicine. The conclusion is that health education activities on guidelines for the use of traditional medicines can increase public knowledge about how to use traditional medicines properly.
Edukasi Kesehatan kerja: Upaya Promotif dan Preventif Musculoskeletal Disorder (MSDs) pada Pekerja Batik Tulis di Kelompok Batik Suka Maju
Authors: Nurwahida Puspitasari  , Arifin Asyhara Naela 
Published: February 2021

Kelompok Batik Suka Maju yang berlokasi di Giriloyo, Wukirsari, Bantul, Daerah Istimewa Yogyakarta (DIY), merupakan industry batik (Home Industri). Berdasarkan hasil studi pendahuluan yang dilakukan pada bulan November 2018 terhadap 10 pekerja di dapatkan hasil bahwa seluruh pekerja merasakan keluhan MSDs (100%). MSDs dapat menjadi suatu permasalahan penting karena dapat menyebabkan antara lain waktu kerja yang hilang, menurunkan produktivitas kerja, penanganannya membutuhkan biaya yang tinggi, penurunan kewaspadaan, meningkatkan resiko terjadinya kecelakaan, dll. Berdasarkan observasi dan diskusi langsung dengan Pengurus kelompok batik suka maju didapatkan beberapa permasalahan yang dihadapi yaitu: Rendahnya pengetahuan pekerja batik tentang gangguan musculoskeletal disorder (MSDs) dan Pekerja Batik tidak mengetahui cara mencegah terjadinya gangguan musculoskeletal disorder (MSDs). Tujuan pengabdian masyarakat ini adalah meningkatkan pengetahuan pekerja batik tulis tentang gangguan Musculoskeletal Disorder (MSDs) dan pemberian pelatihan tentang upaya promotif dan preventif terjadinya gangguan Musculoskeletal Disorder (MSDs). Metode pengabdian yang digunakan guna peningkatan pengetahuan pekerja batik tentang gangguan musculoskeletal disorder (MSDs) dengan metode presentasi, ceramah dan diskusi, serta pelatihan tentang cara mencegah gangguan muscukolskeletal disorder (MSDs) dengan metode praktek langsung berupa stretching exercise. Hasil pengabdian didapatkan peningkatan pengetahuan pekerja batik tentang gangguan musculoskeletal disorder (MSDs) dibuktikan dengan penyebaran kuesioner evaluasi setelah kegiatan dilaksanakan dan pekerja batik mampu mempraktekkan langsung program latihan pencegahan gangguan muscukolskeletal disorder (MSDs) berupa stretching exercise di buktikan dengan foto hasil pelaksanaan kegiatan.
Pelatihan Pencegahan Dan Deteksi Kelompok Risiko HIV/AIDS Ibu Hamil Pada Kader Kesehatan di Desa Slarang
Authors: Sohimah  , Apriani Evy , Lestari Yogi andhi 
Published: February 2021

HIV/AIDS merupakan masalah kesehatan di dunia sejak tahun 1981, penyakit ini berkembang secara pandemik. Obat dan Vaksin untuk mengatasi masalah tersebut belum ditemukan, yang dapat mengakibatkan kerugian tidak hanya di bidang kesehatan tetapi juga di bidang sosial, ekonomi, politik, budaya dan demografi. Penderita HIV biasanya sulit untuk dibedakan dengan orang sehat masa inkubasi virus HIV adalah selama 10 tahun (Depkes RI, 2006; Maryunani dan Aeman, 2009).
Berdasarkan hasil penelitian Sohimah dkk tahun 2019 yang berjudul Analisis Faktor-faktor yang berhubungan dengan Kejadian HIV (+) pada Ibu hamil di Rumah Sakit Umum Daerah Cilacap, bahwa faktor umur tidak berpengaruh signifikan terhadap Kejadian HIV (+) pada Ibu hamil tetapi faktor pekerjaan dan pendidikan berpengaruh signifikan terhadap Kejadian HIV (+) pada Ibu hamil (Sohimah, 2019).
Di Wilayah kerja Puskesmas Kesugihan 2 telah diberlakukan bahwa kepda seluruh ibu hamil untuk dilakukan pemeriksaan VCT sebagai langkah antisipati terhadap HIV/AIDS. Namun demikian belum semua ibu hamil dan kader memahami tentang HIV/AIDS dan dampak terhadapa kehamilan serta bagaimana cara pencegahannya. Berdasarkan uraian diatas menjadi penting untuk dilakukan pelatihan tentang Pelatihan Pencegahan dan Deteksi Faktor Risiko HIV/AIDS Ibu hamil Pada Kader Kesehatan di Desa Slarang Wilayah kerja Puskesmas Kesugihan II.
Berdasarkan pemikiran tersebut diatas, maka perlu diadakan suatu langkah preventif kepada kelompok kader kesehatan yang telah terbentuk tersebut sebagai upaya untuk meningkatkan minat dan peran semua kader kesehatan sehingga dapat meningkatkan pengetahuan dan kemampuan dalam melakukan upaya pencegahan terhadap penularanHIV/AIDS dan identifikasi kelompok risiko tinggi HIV/AIDS sehingga mampu melakukan upaya-upaya pencegahan dan mengenali kelompok-kelompok risiko tinggi penularan HIV/AIDS Pendekatan yang dilakukan untuk mengatasi masalah keterbatasan tersebut maka perlu dilakukan upaya untuk meningkatkan pengetahuan dan ketrampilan upaya pencegahan penularan HIV/AIDS dan deteksi kelompok risiko HIV/AIDS.
Pengabdian dilaksanakan pada hari Kamis tanggal 22 Juli 2020. Acara dihadiri oleh 19 Kader kesehatan yang ada didesa slarang. Terdapat peningkatan pengetahuan dan kemampuan ibu kader kesehatan terhadap upaya pencegahan dan deteksi kelompok risiko HIV/AIDS ibu hamil pada kader kesehatan di desa Slarang.

Kata kunci : Kader Kesehatan.,HIV/AIDS
Determinación in silico de las propiedades inmunogénicas de la glicoproteína E de Zika virus
Authors: Asturias Karla María , Tercero Estuardo , Tuna María Antonieta 
Published: February 2021

Introducción: La infección por Zika virus (ZIKV) ha sido asociada a múltiples complicaciones y nuevas formas de transmisión. La descripción del genoma y la estructura cristalizada permiten desarrollar análisis moleculares, incluyendo las propiedades inmunológicas. Objetivos: En este trabajo, se analiza a la glicoproteína E de ZIKV, con el fin de determinar su utilidad en la creación de una vacuna proteica recombinante. Métodos: Se analizó la glicoproteína E, por medio del software DNASTAR, en base a su antigenicidad de epítopos de células B y MHC-II, estructura secundaria, hidrofilizada, flexibilidad y accesibilidad a solvente en el virión maduro e hidratado. Resultados: Se identificaron 14 sitios antigénicos para células B, de los cuales, 7 comparten su antigenicidad para MHC-II. Al tomar en cuenta los demás parámetros analizados, los sitios se reducen a 3, con longitudes de 13, 9 y 5 aminoácidos. Conclusiones: La glicoproteína E de ZIKV podría desencadenar una respuesta inmune T-dependiente, por tanto, ser útil para la creación de una vacuna proteica recombinante.
Prevalencia de Trastorno de Ansiedad Generalizada según el Trimestre de Embarazo
Authors: Cheang Geraldine , Soldini Aldo , Montenegro Miguel 
Published: February 2021

Introducción: El trastorno de ansiedad generalizado (TAG) es una entidad clínica caracterizada por preocupación excesiva y no controlada que puede causar discapacidad funcional, durante un período mínimo de 6 meses. La prevalencia global de TAG en las pacientes en estado de gestación es de 8.5% a 10.5%, la cual es mayor en comparación a la población general (reportada de 1.2% a 6.4%). Entre los factores de riesgo se incluyen: bajo nivel educacional y socioeconómico, pobreza, desintegración familiar, etc. Se ha reportado como complicaciones de TAG durante el embarazo: incremento de consumo de alcohol, riesgo de parto pre término, bajo peso al nacer, etc. Objetivo: Determinar la prevalencia de trastorno de ansiedad generalizada según el trimestre de embarazo en mujeres gestantes de San Juan Sacatepéquez ya que no existen datos de dicha población. Metodología: Se empleó la escala GAD-7. Se escogió como población a pacientes que asistieron a la consulta externa del Centro de Salud Bárbara durante el mes de junio del 2018. Resultados: La prevalencia de TAG hallada fue: 7.40% en el primer trimestre, 8.82% en el segundo trimestre y 7.31% en el tercer trimestre.
Thermal and Turbulent Properties of the Warm Neutral Medium in the Solar Neighborhood
Authors: Marchal Antoine , Miville-Deschênes Marc-Antoine 
Published: February 2021

Abstract
The transition from the diffuse warm neutral medium (WNM) to the dense cold neutral medium (CNM) is what set the initial conditions to the formation of molecular clouds. The properties of the turbulent cascade in the WNM, essential to describe this radiative condensation process, have remained elusive in part due to the difficulty in mapping out the structure and kinematics of each H i thermal phase. Here we present an analysis of a 21 cm hyper-spectral data cube from the GHIGLS H i survey where the contribution of the WNM is extracted using ROHSA, a Gaussian decomposition tool that includes spatial regularization. The distance and volume of the WNM emission is estimated using 3D dust extinction map information. The thermal and turbulent contributions to the Doppler line width of the WNM were disentangled using two techniques, one based on the statistical properties of the column density and centroid velocity fields, and the other on the relative motions of CNM structures as a probe of turbulent motions. We found that the volume of WNM sampled here (5.2 × 105 pc3), located at the outer edge of the Local Bubble, shows thermal properties in accordance with expected values for heating and cooling processes typical of the solar neighborhood: P
th/k
B = (4.4 ± 2.6) × 103 K cm−3, n = 0.74 ± 0.41 cm−3, and T

k
= (6.0 ± 1.3) × 103 K. The WNM has the properties of sub/trans-sonic turbulence, with a turbulent Mach number at the largest scale probed here (l = 130 pc) of

, a density contrast of

, and velocity and density power spectra compatible with k
−11/3. The low Mach number of the WNM provides dynamical conditions that allow the condensation mode of thermal instability to grow freely and form CNM structures, as predicted by theory.
Evidence for the Accretion of Gas in Star-forming Galaxies: High N/O Abundances in Regions of Anomalously Low Metallicity
Authors: Luo Yuanze , Heckman Timothy , Hwang Hsiang-Chih , Rowlands Kate , Sánchez-Menguiano Laura , Riffel Rogério , Bizyaev Dmitry , Andrews Brett H. , Fernández-Trincado José G. , Drory Niv , Almeida Jorge Sánchez , Maiolino Roberto , Lane Richard R. , Argudo-Fernández Maria 
Published: February 2021

Abstract
While all models for the evolution of galaxies require the accretion of gas to sustain their growth via on-going star formation, it has proven difficult to directly detect this inflowing material. In this paper we use data of nearby star-forming galaxies in the SDSS IV Mapping Nearby Galaxies at Apache Point Observatory survey to search for evidence of accretion imprinted in the chemical composition of the interstellar medium. We measure both the O/H and N/O abundance ratios in regions previously identified as having anomalously low values of O/H. We show that the unusual locations of these regions in the N/O versus O/H plane indicate that they have been created through the mixing of disk gas having higher metallicity with accreted gas having lower metallicity. Taken together with previous analysis on these anomalously low-metallicity regions, these results imply that accretion of metal-poor gas can probably sustain star formation in present-day late-type galaxies.
Acceleration of Ring Current Protons Driven by Magnetosonic Waves: Comparisons of Test Particle Simulations with Quasilinear Calculations
Authors: Fu Song , Ge Yasong 
Published: February 2021

Abstract
Wave–particle interactions play important roles in local acceleration and pitch angle scattering loss of charged particle dynamics in astrophysics and space physics, and energy transfer between plasma waves and particles is a key problem in plasma physics. Using full relativistic test particle simulations, we quantitatively evaluate the magnetosonic wave-driven acceleration of Earth's ring current protons both inside and outside the plasmapause at L = 4.5. Analysis of resonance conditions indicates that the broadband magnetosonic waves can affect protons by multiple harmonic cyclotron resonances. With a representative amplitude ∼200 pT, magnetosonic waves can produce energy diffusion coefficients, obtained from test particle simulations, at rates of ∼10−4 s−1 for protons ∼1–3 keV inside the plasmapause and ∼3–30 keV outside the plasmapause, both at equatorial pitch angles ∼75°–90°. Compared with the quasilinear theory calculations, the test particle diffusion coefficients exhibit a difference due to the nonresonant transit time effect outside the plasmapause. Subsequent 2D Fokker–Planck simulations indicate that on a timescale of ∼2 days, magnetosonic waves can effectively enhance the phase space density of the ring current protons ∼10 keV inside the plasmapause and ∼100 keV outside the plasmapause at equatorial pitch angles ∼60°–90°, thereby leading to the evolvement of the ring current proton distribution from a Kappa-type to a 90°-peaked profile. Our results demonstrate that the local acceleration of the ring current protons by magnetosonic waves is an important process of energy transfer between different populations of magnetospheric protons and hence contributes to the dynamic evolution of Earth's ring current.
Multimessenger Parameter Estimation of GW170817: From Jet Structure to the Hubble Constant
Authors: Wang Hao , Giannios Dimitrios 
Published: February 2021

Abstract
The electromagnetic radiation that followed the neutron star merger event GW170817 revealed that gamma-ray burst afterglows from jets misaligned with our line of sight exhibit a light curve with slowly rising flux. The slope of the rising light curve depends sensitively on the angle of the observer with respect to the jet axis, which is likely to be perpendicular to the merger plane of the neutron star binary. Therefore, the afterglow emission can be used to constrain the inclination of the merging system. Here, we calculate the gamma-ray burst afterglow emission based on the realistic jet structure derived from general-relativistic magnetohydrodynamical simulations of a black hole torus system for the central engine of the gamma-ray burst. Combined with gravitational wave parameter estimation, we fit the multi-epoch afterglow emission of GW170817. We show that with such a jet model, the observing angle can be tightly constrained by multimessenger observations. The best fit observing angle of GW170817 is θ
v = 0.38 ± 0.02 rad. With such a constraint, we can break the degeneracy between inclination angle and luminosity distance in gravitational wave parameter estimation, and substantially increase the precision with which the Hubble constant is constrained by the standard siren method. Our estimation of the distance is D
L = 43.4 ± 1 Mpc and the Hubble constant constraint is 69.5 ± 4 km s−1 Mpc−1. As a result, multimessenger observations of short-duration gamma-ray bursts, combined with a good theoretical understanding of the jet structure, can be powerful probes of cosmological parameters.
The Extraordinary Outburst in the Massive Protostellar System NGC 6334 I-MM1: Spatiokinematics of Water Masers during a Contemporaneous Flare Event
Authors: Chibueze James O. , MacLeod Gordon C. , Vorster Jakobus M. , Hirota Tomoya , Brogan Crystal L. , Hunter Todd R. , van Rooyen Ruby 
Published: February 2021

Abstract
Following an eruptive accretion event in NGC 6334I-MM1, flares in the various maser species, including water masers, were triggered. We report the observed relative proper motion of the highly variable water masers associated with the massive star-forming region, NGC 6334I. High velocity H2O maser proper motions were detected in five maser clusters, CM2-W2 (bow-shock structure), MM1-W1, MM1-W3, UCHII-W1, and UCHII-W3. The overall average of the derived relative proper motion is 85 km s−1. This mean proper motion is in agreement with the previous results from VLA multiepoch observations. Our position as well as the velocity variance and covariance matrix analyses of the maser proper motions show its major axis to have a position angle of −79.°4, cutting through the dust cavity around MM1B and being aligned in the northwest–southeast direction. We interpret this as the axis of the jet driving the CM2 shock and the maser motion. The complicated proper motions in MM1-W1 can be explained by the combined influence of the MM1 northeast–southwest bipolar outflow, the CS(6−5) north–south collimated bipolar outflow, and the radio jet. The relative proper motions of the H2O masers in UCHII-W1 are likely not driven by the jets of the MM1B protostar but by MM3-UCHII. Overall, the post-accretion burst relative proper motions of the H2O masers trace shocks of jet motion.
ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies Selected by Herschel: Discovery of Spatially Extended SMGs and Implications
Authors: Sun Fengwu , Egami Eiichi , Rawle Timothy D. , Walth Gregory L. , Smail Ian , Dessauges-Zavadsky Miroslava , Pérez-González Pablo G. , Richard Johan , Combes Francoise , Ebeling Harald , Pelló Roser , Van der Werf Paul , Altieri Bruno , Boone Frédéric , Cava Antonio , Chapman Scott C. , Clément Benjamin , Finoguenov Alexis , Nakajima Kimihiko , Rujopakarn Wiphu , Schaerer Daniel , Valtchanov Ivan 
Published: February 2021

Abstract
We present an ALMA 1.3 mm (Band 6) continuum survey of lensed submillimeter galaxies (SMGs) at z = 1.0 to ∼3.2 with an angular resolution of ∼0.″2. These galaxies were uncovered by the Herschel Lensing Survey and feature exceptionally bright far-infrared continuum emission (S
peak ≳ 90 mJy) owing to their lensing magnification. We detect 29 sources in 20 fields of massive galaxy clusters with ALMA. Using both the Spitzer/IRAC (3.6/4.5 μm) and ALMA data, we have successfully modeled the surface brightness profiles of 26 sources in the rest-frame near- and far-infrared. Similar to previous studies, we find the median dust-to-stellar continuum size ratio to be small (R
e,dust/R
e,star = 0.38 ± 0.14) for the observed SMGs, indicating that star formation is centrally concentrated. This is, however, not the case for two spatially extended main-sequence SMGs with a low surface brightness at 1.3 mm (≲0.1 mJy arcsec−2), in which the star formation is distributed over the entire galaxy (R
e,dust/R
e,star > 1). As a whole, our SMG sample shows a tight anticorrelation between (R
e,dust/R
e,star) and far-infrared surface brightness (ΣIR) over a factor of ≃1000 in ΣIR. This indicates that SMGs with less vigorous star formation (i.e., lower ΣIR) lack central starburst and are likely to retain a broader spatial distribution of star formation over the whole galaxies (i.e., larger R
e,dust/R
e,star). The same trend can be reproduced with cosmological simulations as a result of central starburst and potentially subsequent “inside-out” quenching, which likely accounts for the emergence of compact quiescent galaxies at z ∼ 2.
Random Walk and Trapping of Interplanetary Magnetic Field Lines: Global Simulation, Magnetic Connectivity, and Implications for Solar Energetic Particles
Authors: Chhiber Rohit , Ruffolo David , Matthaeus William H. , Usmanov Arcadi V. , Tooprakai Paisan , Chuychai Piyanate , Goldstein Melvyn L. 
Published: February 2021

Abstract
The random walk of magnetic field lines is an important ingredient in understanding how the connectivity of the magnetic field affects the spatial transport and diffusion of charged particles. As solar energetic particles propagate away from near-solar sources, they interact with the fluctuating magnetic field, which modifies their distributions. We develop a formalism in which the differential equation describing the field line random walk contains both effects due to localized magnetic displacements and a non-stochastic contribution from the large-scale expansion. We use this formalism together with a global magnetohydrodynamic simulation of the inner-heliospheric solar wind, which includes a turbulence transport model, to estimate the diffusive spreading of magnetic field lines that originate in different regions of the solar atmosphere. We first use this model to quantify field line spreading at 1 au, starting from a localized solar source region, and find rms angular spreads of about 20°–60°. In the second instance, we use the model to estimate the size of the source regions from which field lines observed at 1 au may have originated, thus quantifying the uncertainty in calculations of magnetic connectivity; the angular uncertainty is estimated to be about 20°. Finally, we estimate the filamentation distance, i.e., the heliocentric distance up to which field lines originating in magnetic islands can remain strongly trapped in filamentary structures. We emphasize the key role of slab-like fluctuations in the transition from filamentary to more diffusive transport at greater heliocentric distances.
The Large Far-ultraviolet Flux Deficiency of α Doradus (B8 IIIp Si)
Authors: Monier Richard 
Published: February 2021

Abstract
The far-UV spectral energy distribution of α Dor recorded by IUE is compared to that of the constant and normal star ζ Dra, which has similar fundamental parameters. α Dor has much less flux than ζ Dra shortwards of 1800 Å, due to the accumulation of very strong absorption lines of Si ii, in particular autoionization lines around 1400 Å. Two spectra of α Dor separated by 9 hr (i.e., much less than the rotational period) show evidence of modest variability shortwards of 1800 Å.
Torpedo Maculopathy: A Systematic Review of Case Reports
Authors: Menezes Kimberly , Mancera Norberto , Patel Hershel , Kattih Zein , Mhaskar Rahul 
Published: February 2021

BACKGROUND AND OBJECTIVE:
Torpedo maculopathy (TM) is a rare macular lesion involving the retinal pigment epithelium (RPE). This paper describes a retrospective case report of TM. In addition, the authors present a comprehensive systematic review of 110 cases found in the literature.

PATIENTS AND METHODS:
A search for the term “torpedo maculopathy” was conducted on PubMed, Embase, and Web of Science databases and yielded 62 relevant studies.

RESULTS:
The majority of cases in the literature, including this case, reported an asymptomatic hypopigmented temporal lesion with occasional satellite lesions. Fluorescein angiography generally revealed hypofluorescence, whereas optical coherence tomography demonstrated RPE thinning as well as choroid hyperreflectivity.

CONCLUSIONS:
This is the largest systematic review of torpedo maculopathy to date. The authors' findings confirm that it is a benign, nonprogressive, predominantly unilateral temporal lesion thought to arise during macular development.

[
Ophthalmic Surg Lasers Imaging Retina
. 2021;52:78–83.]