bluuebunny/crossref_metadata_2025_split huggingface dataset:
EMPOWERMENT OF WARIA GUBUG SEBAYA GROUP THROUGH MAKING SKILL TRAINING TAS TALI KUR
Authors: Maryati Heni , Dwiningtyas Mumpuni 
Published: November 2018

Waria (gabungan dari wanita - pria) adalah laki –laki yang lebih suka berperan sebagai perempuan dalam kehidupannya sehari – hari. Waria merupakan salah satu penyandang masalah kesejahteraan social di Indonesia, baik ditinjau dari segi psikologis, sosial, norma, maupun secara fisik (AD.Prayudi, 2014). Di Kabupaten Jombang Provinsi Jawa Timur terdapat ± 100 waria yang rata – rata untuk memenuhi kebutuhan ekonominya mereka bekerja di salon, mengamen dan sebagian besar sebagai waria pekerja seksual (WPS) di sekitar Terminal Jombang. Hal ini akan menjadikan masalah ekonomi, sosial dan kesehatan apabila tidak ada penanganan yang baik untuk merubah hidupnya.
Memberdayakan waria melalui pelatihan ketrampilan membuat tas tali kur
Mengadakan pelatihan ketrampilan tas tali kur selama 12 hari yaitu tanggal 17 – 31 Juli 2018 kepada 5 orang waria perkumpulan gubug sebaya Jombang bekerja sama dengan pelatih home industri Desa Bongkot sekaligus merupakan tempat pelaksanaan kegiatan.
Hasil kegiatan ini meningkatkan ketrampilan waria yang bisa membuat mereka mandiri menghasilkan uang dengan membuat tas tali kur sehingga meningkatkan perekonomian, guna bekal hidup serta mencegah penyakit menular seksual dengan berhenti menjadi waria pekerja seksual yang akan membawa dampak perbaikan tata nilai di masyarakat secara sosial meningkatkan harkat dan martabat , ketentraman dan kesehatan.
Kata kunci : pemberdayaan, waria, ketrampilan tas tali kur
UPAYA PENINGKATAN GIZI BALITA DENGAN PEMBERIAN MAKANAN TAMBAHAN (PMT) BERKUALITAS DI DESA PANGKUR, KEC.PANGKUR, KABUPATEN NGAWI
Authors: Kurniasih Erwin , Prawoto Edy , Pariyem Pariyem 
Published: November 2018

Gizi buruk atau kurang di Indonesia masih menjadi permasalahan yang perlu mendapat perhatian dari berbagai pihak baik pemerintah, tenaga kesehatan, maupun masyarakat. Salah satu upaya untuk mengatasi gizi kurang atau buruk pada balita adalah dengan pemberian makanan tambahan (PMT) yang berkualitas. Sebagai tenaga kesehatan, tim pengabdi peduli untuk membantu menangani masalah gizi balita yang terjadi di masyarakat dengan melaksanakan kegiatan pemberian PMT berkualitas pada balita. Bentuk kegiatan yang dilakukan adalah penilaian status gizi balita dengan pendataan usia balita, menimbang dan mengukur tinggi badan. Selain itu juga dilakukan penyuluhan tentang PMT balita yang diakhiri dengan pembagian PMT bagi balita. Kegiatan ini dilakukan pada tanggal 9 April 2018 di Posyandu balita desa Pangkur, kec.Pangkur kota Ngawi. Jumlah balita yang hadir 42 anak. Dari hasil kegiatan, didapatkan data untuk status gizi balita baik sebanyak 34 anak (81%), gizi kurang 8 anak (19%), dan tidak ada gizi buruk.
Kata Kunci : Balita, Gizi, PMT
PEMBENTUKAN PROGRAM POS PEMBINAAN TERPADU (POSBINDU) PENYAKIT TIDAK MENULAR (PTM) DENGAN MEMANFAATKAN DANA DESA PEMERINTAH DESA NGROWO KECAMATAN BANGSAL – MOJOKERTO
Authors: Kusuma Yudha Laga Hadi , Puspitaningsih Dwiharini , Dwisyalfina Agustin , Widayanti Elok 
Published: November 2018

Penyakit tidak menular masih menjadi penyebab kematian terbesar masyarakat pada negara berkembang dan menengah. Faktor risiko penyakit tidak menular ini dapat diminimalkan melalui upaya kesehatan berbasis masyarakat (UKBM) dengan mengaktifkan program pos pembinaan terpadu penyakit tidak menular (Posbindu-PTM). Saat ini dengan lahirnya Undang – Undang Desa yang didalamnya telah mengatur penggunaan Dana Desa, maka penyelenggaraan Posbindu-PTM di Desa dapat di biayai dengan memanfaatkan penggunaan Dana Desa.
Pengabdian masyarakat yang di lakukan Tim Pengabdian Masyarakat STIKes Majapahit bersama Tim dari Puskesmas Bangsal di Desa Ngrowo Kecamatan Bangsal Kabupaten Mojokerto ini bertujuan untuk membentuk program Posbindu-PTM dengan memanfaatkan Dana Desa yang dimiliki oleh pemerintah Desa Ngrowo. Pengapdian masyarakat ini diharapkan pada akhirnya masyarakat akan aktif dalam mengikuti program Posbindu-PTM sehingga faktor risiko penyakit tidak menular masyarakat dapat terkontrol.
Kegiatan pengabdian masyarakat ini meliputi pendidikan kesehatan pada masyarakat tentang penyakit tidak menular, upaya advokasi pada pemerintah Desa Ngrowo tentang program Posbindu-PTM, pembentukan dan pelatihan Kader serta aplikasi pelaksanaan Posbindu-PTM langsung pada masyarakat. Hasil yang didapatkan, pemerintah Desa Ngrowo mengalokasikan biaya penyenggaraan Posbindu-PTM melalui Dana Desa 2018, sebagian besar 50 orang (90%) masyarakat memiliki antusias yang tinggi untuk mengikuti Posbindu-PTM. Masyarakat yang sukarela menjadi Kader Posbindu-PTM ada 21 orang dan pelaksanaan Posbindu-PTM dilaksanakan di 3 Dusun yang ada di Desa Ngrowo setiap satu bulan sekali pada masing – masing dusun.
Program Posbindu-PTM merupakan salah satu upaya untuk meminimalkan faktor risiko penyakit tidak menular pada masyarakat. Pembiayaan penyelenggaraan Posbindu-PTM dapat di alokasikan melalui pemanfaatan Dana Desa yang di miliki Desa sebagai bagian dari program pemberdayaan masyarakat.
Kata Kunci : Posbindu – PTM, Dana Desa
Analisis Brand Strategy pada Perguruan Tinggi Swasta Islam di Kota Medan
Authors: Kurnia Efry , Aisha Novi 
Published: November 2018

Perguruan tinggi swasta Islam yang ada di Kota Medan merupakan perguruan tinggi yang selalu berusaha mewujudkan apa yang dibutuhkan oleh masyarakat. Dengan berbagai model dan jenis sisitem pendidikan yang ditawarkan semakin membuat tingkat persaingan yang semakin kuat dan berbagai penerapan strategy yang dijalankan secara langsung membuat masyarakat memutuskan mana yang sesuai dengan keinginan dan kebutuhan yang umumnya pendidikan dengan dasar dan teknik yang berkualitas. Tujuan peneltian ini untuk mengetahui dan menganalisis brand strategy yang meliputi brand image, brand identity, religious value dan brand trust pada perguruan tinggi swasta islam yang ada di Kota Medan. Penelitian ini menggunakan alat analisis regresi berganda dengan program SPSS 16.0. Menggunakan jumlah sampel 115 mahasiswa/i di beberapa perguruan tinggi swasta islam yang ada di Kota Medan sebagai responden. Sifat penelitian ini adalah deskriptif explanatory research. Hasil penelitian menunjukkan variabel brand strategy yaitu brand image, brand identity, religious value memiliki pengrauh positif dan signifikan terhadap variabel brand trust.
POLA PERPINDAHAN PENGGUNAAN MEREK HANDPHONE DI KALANGAN MAHASISWA Studi Kasus Pada Mahasiswa STIE Binaniaga
Authors: Djan Ismulyana , Ruvendi Ramlan 
Published: November 2018

penelitian ini bertujuan untuk : 1. mengidentifikasi alasan mahasiswa STIE Binaniaga memilih merek handphone tertentu sebagai alat komunikasi, 2. untuk mengetahui perpindahan penggunaan suatu merek handphone ke merek lainnya, dan 3. membuat proyeksi pangsa pasar handphone dikalangan mahasiswa. Dengan responden mahasiswa STIE Binaniaga sebanyak 76 orang dan menggunakan analisis Rantai Markov diperoleh kesimpulan bahwa : • Merek handphone yang banyak diminati responden adalah Nokia, dipilih karena pengoperasiannya mudah serta fiturnya lengkap. Urutan kedua ditempati Sony Ericsson dipilih karena mudah pengoperasian, fiturnya lengkap dan sekedar mencoba-coba. Sedangkan Motorola dibeli karena fitur lengkap dan harganya murah. Merek lainnya juga dipilih karena murah harganya. • Merek handphone seperti Nokia, Siemen, Philips, Samsung, Motorola mengalami pergeseran peminatan kecuali Sony Ericsson dan merek handphone lainnya (merek-merek yang tidak diperhitungkan) mengalami kenaikkan. • Pangsa pasar yang tetap stabil dalam tahun 2007-2009 diprediksi adalah Sony Ericsson, sedangkan Nokia, Motorola dan Samsung mengalami penurunan..
The Effect of Job Motivation and Job Discipline upon Job Performance of Employees In The Personal Care Department at PT. Reckitt Benckiser Indonesia
Authors: Suwandi Andi , Syaefudin M Husaen 
Published: November 2018

In this case, the company must be able to manage the existing humanresources effectively and efficiently, so the company can achieve the goals that havebeen set-up. So, employee’s job performance has been a very important role to thesuccess or failure of a company. Several factors that affect employee job performanceare motivation and work discipline. Partial test results (T-test) about the influence ofmotivation on employee’ job performance has shown the value of T-count of 6.146with significance of 0.000. It indicates that the variable of motivation has positive andsignificant effect on employee job performance. Because value T-count > T-table or6.146 > 1.665 and level of significance < level significance or 0.000 < 0.050. and testresult regarding the influence of work discipline on employee job performance showsthe value of T-count of 3.019 with significance of 0.003. it indicates that the variable ofwork discipline have positive and significant effect on employee job performance.Because value T-count > T-table or 3.019 > 1,665 and level of significance < level ofsignificance or 0.003 < 0,050.While testing simultaneously (F-test) about the influenceof motivation and work discipline on employee job performance shows the value of Fcountof 47,215 with significant of 0,000. It indicates that the variable of motivation and work discipline have positive and significant effect on employee job performance.Because value F-count > F-table or 47,215 > 3,111 and level of significance < level ofsignificance or 0,000 < 0,050.
Les karsts littoraux des Alpes-Maritimes : inventaire des émergences sous-marines et captage expérimental de Cabbé
Authors: Gilli Eric 
Published: November 2018

Inventory of coastal and submarine springs in the Alpes-maritimes (France). Expérimental catchment at the Cabbé spring.
Several submarine freshwater springs are present on karstic shore in the Alpes-Maritimes (France). Salinity and conductivity measuring coupled with GPS location has permited to inventory these springs. Three main springs have an average flow around 500 Us. A balance on inland and offshore springs allows to explain the deficit observed on karstic units of Arc de Nice area. A dam was built in the submarine karstic spring of Cabbé Massottn (Roquebrune-Cap-Martin, France) to study the effects of an artificial augmentation of the pressure on the salinity of a karstic aquifer.
Trials in low and high water levels show the impossibility to increase the pressure. The presence of several springs and the important fracturation of limestone don't allow a sufficient impermeability of the dam site. Nevertheless, the salinity decreases, due to the physical separation between the two kinds of water.
Modes de positionnement topographique et électromagnétique d'un siphon. Exemple du Qattine Azar (Liban)
Authors: Courbon Paul 
Published: November 2018

La conjonction de paramètres aussi divers que l'explosion démographique, l'urbanisation galopante et la moindre alimentation des nappes est à l'origine d'une réelle pénurie d'eau dans de nombreux pays méditerranéens et du Proche Orient. La découverte d'une importante rivière souterraine dans les montagnes du Liban a fait naître un projet de captage nécessitant un forage de 280 mètres à travers la masse calcaire.
L'auteur décrit la méthode topographique utilisée pour lever la cavité et positionner le futur forage en surface. Cette détermination topographique a été complétée par un positionnement électromagnétique ARCAS mis au point par Joan Erra. La précision de ces deux approches est évaluée.
Turbidité, indicateur du fonctionnement perturbé du géosystème karstique de l'Atlas de Beni Mellal (Moyen Atlas méridional, Maroc)
Authors: El Khalki Yahia , Hafid Abdellatif 
Published: November 2018

La turbidité des eaux des sources karstiques est un phénomène général des montagnes calcaires méditerranéennes anthropisées.
Mais on constate, dans l'état actuel de nos connaissances, qu'elle est peu étudiée. Par ailleurs, elle représente un indicateur pertinent du dysfonctionnement des géosystèmes karstiques qui ont subi une forte pression anthropique. Cet article a pour objectif de déterminer, via la turbidité, l'importance de la perturbation de ce système karstique sous influence anthropique. Et de montrer ainsi le rôle joué par le karst de surface, par le climat et par l'homme dans l'aggravation de la turbidité. Car Aïn Asserdoune représente non seulement, la source qui assure l'alimentation en eau potable de la ville de Beni Mellal, mais un des sites touristiques les plus fréquentés de la région. La source de Aïn Asserdoune, exutoire principal de l'aquifère liasique, se caractérise par des eaux troubles. Après des périodes sèches suivies d'orages brutaux, la turbidité des eaux peut dépasser 2000 JTU (unité de turbidité Jackson).
Trois facteurs se combinent pour favoriser la turbidité des eaux : 1) Le climat : Les pluies orageuses d'automne, qui suivent une longue saison aride estivale, tombent sur des sols secs et mal protégés par la végétation. Elles provoquent une importante mobilisation de particules fines qui s'infiltrent dans l'épikarst. 2) La structure interne du karst :
le cheminement des eaux turbides vers l'exutoire principal du système karstique est facilité par l'existence de drains développés et hiérarchisés. traçages ont montré que le temps de transit des eaux était compris entre 24 et 72 heures.
3) L'impact anthropique : La modernisation agricole de la plaine du Tadla (140 000 ha irrigués) s'est accompagnée d'une forte pression sur les ressources forestières de l'Atlas de Beni Mellal. Les défrichements ont entraîné l'accentuation de l'érosion des sols qui a conduit à l'exhumation des lapiés couverts.
Le dysfonctionnement du géosystème karstique se traduit en outre par l'arrêt des phénomènes de travertinisation à l'aval des sources.
Atmospheric Characterization of Directly Imaged Exoplanets with JWST/MIRI
Authors: Danielski Camilla , Baudino Jean-Loup , Lagage Pierre-Olivier , Boccaletti Anthony , Gastaud René , Coulais Alain , Bézard Bruno 
Published: November 2018

Abstract
The Mid-Infrared instrument (MIRI) on board the James Webb Space Telescope will perform the first ever characterization of young giant exoplanets observed by direct imaging in the 5–28 μm spectral range. This wavelength range is key for both determining the bolometric luminosity of the cool known exoplanets and for accessing the strongest ammonia bands. In conjunction with shorter wavelength observations, MIRI will enable a more accurate characterization of the exoplanetary atmospheric properties. Here we consider a subsample of the currently known exoplanets detected by direct imaging, and we discuss their detectability with MIRI, either using the coronagraphic or the spectroscopic modes. By using the Exo-REM atmosphere model, we calculate the mid-infrared emission spectra of 14 exoplanets, and we simulate MIRI coronagraphic or spectroscopic observations. Specifically, we analyze four coronagraphic observational setups, which depend on (i) the target-star and reference-star offset (0, 3, 14 mas), (ii) the wavefront-error (130, 204 nm root mean square), and (iii) the telescope jitter amplitude (1.6, 7 mas). We then determine the signal-to-noise and integration time values for the coronagraphic targets whose planet-to-star contrasts range from 3.9 to 10.1 mag. We conclude that all the MIRI targets should be observable with different degrees of difficulty, which depends on the final in-flight instrument performances. Furthermore, we test for detection of ammonia in the atmosphere of the coolest targets. Finally, we present the case of HR 8799 b to discuss what MIRI observations can bring to the knowledge of a planetary atmosphere, either alone or in combination with shorter wavelength observations.
The Rotational Evolution of Young, Binary M Dwarfs
Authors: Stauffer John , Rebull Luisa M. , Cody Ann Marie , Hillenbrand Lynne A. , Pinsonneault Marc , Barrado David , Bouvier Jerome , David Trevor 
Published: November 2018

Abstract
We have analyzed K2 light curves for more than 3000 low-mass stars in the ∼8 Myr old Upper Sco association, the ∼125 Myr age Pleiades open cluster, and the ∼700 Myr old Hyades and Praesepe open clusters to determine stellar rotation rates. Many of these K2 targets show two distinct periods, and for the lowest-mass stars in these clusters, virtually all of these systems with two periods are photometric binaries. The most likely explanation is that we are detecting the rotation periods for both components of these binaries. We explore the evolution of the rotation rate in both components of photometric binaries relative to one another and to nonphotometric binary stars. In Upper Sco and the Pleiades, these low-mass binary stars have periods that are much shorter on average and much closer to each other than would be true if drawn at random from the M dwarf single stars. In Upper Sco, this difference correlates strongly with the presence or absence of infrared excesses due to primordial circumstellar disks—the single-star population includes many stars with disks, and their rotation periods are distinctively longer on average than their binary star cousins of the same mass. By Praesepe age, the significance of the difference in rotation rate between the single and binary low-mass M dwarf stars is much less, suggesting that angular momentum loss from winds for fully convective zero-age main-sequence stars erases memory of the rotation rate dichotomy for binary and single very low mass stars at later ages.
Dynamical Analysis of Three Distant Trans-Neptunian Objects with Similar Orbits
Authors: Khain T. , Becker J. C. , Adams F. C. , Gerdes D. W. , Hamilton S. J. , Franson K. , Zullo L. , Sako M. , Napier K. , Lin 林 Hsing Wen 省文 , Markwardt L. , Bernardinelli P. , Abbott T. M. C. , Abdalla F. B. , Annis J. , Avila S. , Bertin E. , Brooks D. , Rosell A. Carnero , Kind M. Carrasco , Carretero J. , Cunha C. E. , Costa L. N. da , Davis C. , Vicente J. De , Desai S. , Diehl H. T. , Doel P. , Eifler T. F. , Flaugher B. , Frieman J. , García-Bellido J. , Gruen D. , Gruendl R. A. , Gutierrez G. , Hartley W. G. , Hollowood D. L. , Honscheid K. , James D. J. , Krause E. , Kuehn K. , Kuropatkin N. , Lahav O. , Maia M. A. G. , Menanteau F. , Miquel R. , Nord B. , Ogando R. L. C. , Plazas A. A. , Romer A. K. , Sanchez E. , Scarpine V. , Schindler R. , Schubnell M. , Sevilla-Noarbe I. , Smith M. , Soares-Santos M. , Sobreira F. , Suchyta E. , Swanson M. E. C. , Tarle G. , Vikram V. , Walker A. R. , Wester W. , Zhang Y. ,   (DES Collaboration)
Published: November 2018

Abstract
This paper reports the discovery and orbital characterization of two extreme trans-Neptunian objects (ETNOs), 2016 QV89 and 2016 QU89, which have orbits that appear similar to that of a previously known object, 2013 UH15. All three ETNOs have semimajor axes a ≈ 172 au and eccentricities e ≈ 0.77. The angular elements (i, ω, Ω) vary by 6°, 15°, and 49°, respectively, between the three objects. The two new objects add to the small number of TNOs currently known to have semimajor axes between 150 and 250 au, and they serve as an interesting dynamical laboratory to study the outer realm of our solar system. Using a large ensemble of numerical integrations, we find that the orbits are expected to reside in close proximity in the (a, e) phase plane for roughly 100 Myr before diffusing to more separated values. We find that an explanation for the orbital configuration of the bodies as a collision product is disfavored. We then explore other scenarios that could influence their orbits. With aphelion distances over 300 au, the orbits of these ETNOs extend far beyond the classical Kuiper Belt and an order of magnitude beyond Neptune. As a result, their orbital dynamics can be affected by the proposed new solar system member, referred to as Planet Nine in this work. With perihelion distances of 35–40 au, these orbits are also influenced by resonant interactions with Neptune. A full assessment of any possible new solar system planets must thus take into account this emerging class of TNOs.
Concurrent Starbursts in Molecular Gas Disks within a Pair of Colliding Galaxies at z = 1.52
Authors: Silverman J. D. , Daddi E. , Rujopakarn W. , Renzini A. , Mancini C. , Bournaud F. , Puglisi A. , Rodighiero G. , Liu D. , Sargent M. , Arimoto N. , Béthermin M. , Fensch J. , Hayward C. C. , Kartaltepe J. , Kashino D. , Koekemoer A. , Magdis G. , McCracken H. J. , Nagao T. , Sheth K. , Smolčić V. , Valentino F. 
Published: November 2018

Abstract
We report on the discovery of a merger-driven starburst at z = 1.52, PACS-787, based on high signal-to-noise ALMA observations. CO(5–4) and continuum emission (850 μm) at a spatial resolution of 0.″3 reveal two compact (r
1/2 ∼ 1 kpc) and interacting molecular gas disks at a separation of 8.6 kpc, indicative of an early stage in a merger. With an SFR of 991 M
⊙ yr−1, this starburst event should occur closer to final coalescence, as is usually seen in hydrodynamical simulations. From the CO size, inclination, and velocity profile for both disks, the dynamical mass is calculated through a novel method that incorporates a calibration using simulations of galaxy mergers. Based on the dynamical mass, we measure (1) the molecular gas mass, independent from the CO luminosity, (2) the ratio of the total gas mass and the CO(1–0) luminosity (

), and (3) the gas-to-dust ratio, with the latter two being lower than typically assumed. We find that the high star formation triggered in both galaxies is caused by a set of optimal conditions: a high gas mass/fraction, a short depletion time (τ
depl = 85 and 67 Myr) to convert gas into stars, and the interaction of likely counter-rotating molecular disks that may accelerate the loss of angular momentum. The state of interaction is further established by the detection of diffuse CO and continuum emission, tidal debris that bridges the two nuclei and is associated with stellar emission seen by HST/WFC3. This observation demonstrates the power of ALMA to study the dynamics of galaxy mergers at high redshift.
The Relation between Escape and Scattering Times of Energetic Particles in a Turbulent Magnetized Plasma: Application to Solar Flares
Authors: Effenberger Frederic , Petrosian Vahé 
Published: November 2018

Abstract
A knowledge of the particle escape time from the acceleration regions of many space and astrophysical sources is of critical importance in the analysis of emission signatures produced by these particles and in the determination of the acceleration and transport mechanisms at work. This Letter addresses this general problem, in particular in solar flares, where in addition to scattering by turbulence, the magnetic field convergence from the acceleration region toward its boundaries also influences the particle escape. We test an (approximate) analytic relation between escape and scattering times, and the field convergence rate, based on the work of Malyshkin & Kulsrud, valid for both strong and weak diffusion limits and isotropic pitch-angle distributions of the injected particles, with a numerical model of particle transport. To this end, a kinetic Fokker–Planck transport model of particles is solved with a stochastic differential equation scheme, assuming different initial pitch-angle distributions. This approach enables further insights into the phase-space dynamics of the transport process, which would otherwise not be accessible. We find that in general the numerical results agree well with the analytic equation for the isotropic case; however, there are significant differences in the weak diffusion regime for non-isotopic cases, especially for distributions beamed along the magnetic field lines. The results are important in the interpretation of observations of energetic particles in solar flares and other similar space and astrophysical acceleration sites, and for the determination of acceleration-transport coefficients, commonly used in Fokker–Planck–type kinetic equations.