bluuebunny/crossref_metadata_2025_split huggingface dataset:
DEWAN REDAKSI
Authors: Redaksi Dewan 
Published: December 2019

Susunan Redaksi
Jurnal Manajemen & Bisnis Kreatif

Pelindung	:	Dr. H. Dedi Mulyadi, S.E., M.M.
Ketua Penyunting	:	Sari Marliani, S.E.,M.M.
Dewan Penyunting	:	-	H. Tarpan Suparman, S.Pd.,M.Pd (UBP Karawang)
-	Nelly Martini, S.E., M.M. (Unsika)
-	H. Acim Supriadi, S.E.,M.M. (UBP Karawang)
-	Rahmat Hasbullah, S.E., M.M. (Unsika)
-	Abdul Yusuf, S.E., M.M. (Unsika)
-	Yudin Wahyudin, S.E., M.M. (STIE YPN)
-	Jajang Sugiat, S.E.,M.M. (STIE Yasa Anggana)
-	Yudi Suwandi, S.E., M.M. (STIE Ekuitas)

Penyunting Pelaksana	:	-	Ajat Sudrajat, S.E., M.M.
-	Ina Ratnasari, SE., M.M.

Sirkulasi dan Pemasaran	:	-	Chandra Zonyfar, S.Kom
-	Yogi Ginanjar
-	Alifya Nurzehan

Diterbitkan oleh Lembaga Penelitian dan Pengabdian Pada Masyarakat
Universitas Buana Perjuangan Karawang

Alamat Redaksi :
Jl. HS Ronggowaluyo Telukjambe Timur Karawang 41361
Telp. / Fax. 0267 8403140 email : jurnalmanajemen@ubpkarawang.ac.id
site : lppm.ubpkarawang.ac.id
Sustained Mentoring of Students of Color
Authors: Aguilar Nadia , Ulanoff Sharon H. 
Published: December 2019

Using a testimonio (Beverley, 1989) in two voices, we discuss the mentoring practices in one Ed.D. Program in Educational Leadership at a large urban public university in California through the eyes of one mentee, Author1, and her mentor, Author2. We discuss our relative roles, how we learned from each other, and the practices that supported Author1’s success through the lens of shared authority (Frisch, 2003; Wong, 2016), a term used to describe the interviewee-interviewer relationship in oral histories. We borrow the term shared authority as it embodies “the cultivation of trust, the development of collaborative relationships, and shared decision-making” (High, 2009, p. 13) that became part of our shared story as Author1 navigated her doctoral studies through graduation and beyond. The following testimonio describes how we both approached this relationship and how it evolved over the course of Author1’s Ed.D. journey and beyond.
Удосконалений метод χ 2-кластеризації та його застосування до аналізу аварійності на автомобільному транспорті.
Authors: Ханін O. , Лотиш В. , Гуменюк Л. , Гуменюк П. 
Published: December 2019

Існує чимало методів кластеризації даних, але вони мають ряд недоліків, зокрема, з одного боку, це – неоднозначність розбиття масиву даних на групи, а з іншого – неможливість оцінити ступінь однорідності об’єктів, що належать одному і тому ж кластеру. Мета цієї роботи - розробити метод кластерного аналізу багатовимірних даних різної природи, який забезпечить однозначність розбиття набору незалежних вибірок на кластери, що не перетинаються, так, щоб ймовірність помилкової кластеризації не перевищувала певного наперед заданого рівня. Метод кластеризації ґрунтується на використанні критерію узгодженості χ2 .
З іншої сторони, проблема аварійності на автомобільному транспорті є достатньо гострою у вітчизняних реаліях, оскільки рівень ДТП з потерпілими значно перевищує середній європейський. В той же час, кластеризація регіонів України за видами дорожньо-транспортних пригод з постраждалими, їх причинами та винуватцями дозволить зрозуміти спільні регіональні фактори, що впливають на рівень аварійності, визначити та впровадити кращі практики її запобігання. Саме тому представляється актуальним застосування запропонованого методу до аналізу аварійності на автомобільному транспорті в Україні.Розроблений метод реалізований програмно та застосований до порівняльного аналізу рівня аварійності на автомобільному транспорті по регіонах України.
Визначення трендів на ринку праці. Аналіз та структурування отриманої інформації.
Authors: Єрошенко О. , Степаніщева В. С. , Єременко О. 
Published: December 2019

У даній роботі розглянуто способи визначення трендів на ринку праці. Проведено огляд провідних веб сервісів з надання інформації про вимоги роботодавців до майбутніх працівників. Представлено алгоритми парсингу HTML коду сайтів вакансій. Запропоновані методи пост обробки та аналізу результатів парсингу. Наведені моделі зберігання результатів парсингу та критерії подальшого використання результатів в системі дистанційного навчання. Для парсингу та аналізу використовувались можливості мови Python.
KOMUNIKASI PENGEMBANGAN MASYARAKAT ISLAM ANALISIS TEORI DIALEKTIKA RELASIONAL
Authors: Muniruddin Muniruddin 
Published: December 2019

<p>Komunikasi merupakan cabang ilmu sosial yang bersifat multidisipliner, hal ini disebabkan karena kajian komunikasi yang sedemikian kompleksnya dan berkaitan dengan berbagai disiplin ilmu pengetahuan termasuk di dalamnya dialektika relasional. <em>Relational Dialectics Theory</em> atau yang lazim disebut dengan teori dialektika relasional merupakan penjabaran ide Mikhail Bakhtin, bahwa hidup adalah sebuah monolog terbuka dan manusia mengalami tabrakan antara menentang keinginan dan kebutuhan dalam komunikasi relasional. Baxter termasuk bagian dari ketegangan dialektis yang mengingatkan kita bahwa hubungan yang terus berubah, dan bahwa hubungan yang sukes dan memuaskan membutuhkan perhatian konstan. Meskipun deskripsi Baxter dari relational dialektika menyeluruh, itu tidak berarti tepat atau semua termasuk karena kita semua memiliki pengalaman ketegangan yang berbeda dengan cara yang berbeda pula. Pran komunikasi ditinjau dari teori dialektika relasional adalah berupaya untuk mengelola dan menegosiasikan ketegangan serta kontradiksi-kontradiksi dalam hubungan antar manusia.</p>
Neumonía atípica por influenza A H1N1: reporte de casos en Lambayeque, Perú, 2018
Authors: Calderón-Flores Armando , Yazawa-Ballena Yiro 
Published: December 2019

La influenza A H1N1 se diagnosticó por primera vez en México y Estados Unidos en abril del 2009. Esta pandemia es el resultado de una nueva cepa de virus de Influenza A que no se había identificado previamente en el humano. Los síntomas clínicos habituales de esta enfermedad pueden no distinguirse de la influenza estacional, e incluyen: tos, fiebre, mal estado general, odinofagia y dolores musculares. La complicación pulmonar de la influenza más frecuente es la neumonía. Se reportan dos casos de varones adultos provenientes de Bagua (ciudad de Perú con clima tropical); uno sin antecedentes patológicos, y el otro, inmunocomprometido. Ambos pacientes cursan con patrones clínico laboratoriales similares. La infección se confirmó mediante la prueba de reacción en cadena de la polimerasa con transcriptasa inversa (RT-PCR).
Carcinoma in situ conjuntival: reporte de un caso clínico
Authors: Chin-Wong Jorge Luis 
Published: December 2019

El carcinoma in situ de conjuntiva forma parte de un grupo de entidades denominadas Neoplasias escamosas de la superficie ocular (NESO), que consisten en un amplio rango de lesiones corneo-conjuntivales que abarcan desde displasias conjuntivales hasta carcinomas escamosos invasivos. De presentación rara, geográficamente son más frecuentes cerca de la línea ecuatorial y se asocian a diversos factores ambientales (exposición a rayos ultravioleta), infecciosos (Virus de papiloma humano, Virus de inmunodeficiencia humana), Carcinógenos químicos, entre otros. Presentamos el caso de un paciente con tumoración conjuntival diagnosticada inicialmente como pterigión por médico general, de crecimiento rápido, su manejo y su evolución
Collisional N-body Dynamics Coupled to Self-gravitating Magnetohydrodynamics Reveals Dynamical Binary Formation
Authors: Wall Joshua E. , McMillan Stephen L. W. , Low Mordecai-Mark Mac , Klessen Ralf S. , Zwart Simon Portegies 
Published: December 2019

AbstractWe describe a star cluster formation model that includes individual star formation from self-gravitating, magnetized gas, coupled to collisional stellar dynamics. The model uses the Astrophysical Multi-purpose Software Environment to integrate an adaptive-mesh magnetohydrodynamics code (FLASH) with a fourth order HermiteN-body code (ph4), a stellar evolution code (SeBa), and a method for resolving binary evolution (multiples). This combination yields unique star-formation simulations that allow us to study binaries formed dynamically from interactions with both other stars and dense, magnetized gas subject to stellar feedback during the birth and early evolution of stellar clusters. We find that for massive stars, our simulations are consistent with the observed dynamical binary fractions and mass ratios. However, our binary fraction drops well below observed values for lower mass stars, presumably due to unincluded binary formation during initial star formation. Further, we observe a buildup of binaries near the hard-soft boundary that may be an important mechanism driving early cluster contraction.
Perpendicular Ion Heating by Cyclotron Resonant Dissipation of Turbulently Generated Kinetic Alfvén Waves in the Solar Wind
Authors: Isenberg Philip A. , Vasquez Bernard J. 
Published: December 2019

Abstract
Solar wind ions are observed to be heated in the directions perpendicular to the large-scale magnetic field, with preferential heating given to heavy ions. In the solar corona, this heating may be responsible for the generation of the wind itself. It is likely that this heating results from the dissipation of plasma turbulence, but the specific kinetic mechanism that produces these preferential effects is not known. Solar wind turbulence at proton scales is often characterized in terms of highly oblique kinetic Alfvén waves (KAWs), which have been thought to dissipate through the Landau resonance and yield parallel heating. We show that the quasilinear resonant cyclotron interaction between KAWs and solar wind ions can actually produce perpendicular ion heating. We present an illustrative calculation of a steady, critically balanced spectrum of KAWs acting on homogeneous ion distributions with a plasma β = 0.1, representative of turbulent conditions in the fast solar wind near 20 R

s
. The KAWs are described here by a two-fluid dispersion relation. We find that thermal protons are strongly heated in the perpendicular direction within a typical quasilinear time of several thousand gyroperiods, which corresponds to only a few minutes at 20 R

s
. Alpha particles in the same fluctuation field are heated to similar perpendicular thermal speeds, equivalent to the greater than mass proportional perpendicular temperatures that are commonly observed. We discuss improvements to this simple model that may determine whether this mechanism can be responsible for the observed coronal and solar wind ion heating.
Astrochemical Bistability: Autocatalysis in Oxygen Chemistry
Authors: Dufour Gwénaëlle , Charnley Steven B. 
Published: December 2019

Abstract
The origin of bistable solutions in the kinetic equations describing the chemistry of dense interstellar clouds is explained as being due to the autocatalysis and feedback of oxygen nuclei from the oxygen dimer (O2). We identify four autocatalytic processes that can operate in dense molecular clouds, driven respectively by reactions of H+, He+, C+, and S+ with O2. We show that these processes can produce the bistable solutions found in previous studies, as well as the dependence on various model parameters such as the helium ionization rate, the sulfur depletion and the

electron recombination rate. We also show that ion–grain neutralizations are unlikely to affect the occurrence of bistability in dense clouds. It is pointed out that many chemical models of astronomical sources should have the potential to show bistable solutions.
Discovery of an X-Ray Quasar Wind Driving the Cold Gas Outflow in the Ultraluminous Infrared Galaxy IRAS F05189-2524
Authors: Smith Robyn N. , Tombesi Francesco , Veilleux Sylvain , Lohfink Anne M. , Luminari Alfredo 
Published: December 2019

Abstract
We present new XMM-Newton and NuSTAR observations of the galaxy merger IRAS F05189-2524, which is classified as an ultraluminous infrared galaxy and optical Seyfert 2 at z = 0.0426. We test a variety of spectral models that yield a best fit consisting of an absorbed power law with emission and absorption features in the Fe K band. Remarkably, we find evidence for a blueshifted Fe K absorption feature at E = 7.8 keV (rest frame) which implies an ultrafast outflow (UFO) with v
out = 0.11 ± 0.01c. We calculate that the UFO in IRAS F05189-2524 has a mass outflow rate of

yr−1, a kinetic power of

8% L
AGN, and a momentum rate (or force) of

. Comparing the energetics of the UFO to the observed multi-phase outflows at kiloparsec scales yields an efficiency factor of f ∼ 0.05 for an energy-driven outflow. Given the uncertainties, however, we cannot exclude the possibility of a momentum-driven outflow. Comparing IRAS F05189-2524 with nine other objects with observed UFOs and large-scale galactic outflows suggests that there is a range of efficiency factors for the coupling of the energetics of the nuclear and galaxy-scale outflows that likely depend on specific physical conditions in each object.
Laboratory Formation and Photochemistry of Fullerene/Anthracene Cluster Cations
Authors: Zhen Junfeng , Zhang Weiwei , Yang YuanYuan , Zhu Qingfeng , Tielens Alexander G. G. M. 
Published: December 2019

Abstract
Besides buckminsterfullerene (C60), other fullerenes and their derivatives may also reside in space. In this work, we study the formation and photodissociation processes of astronomically relevant fullerene/anthracene (C14H10) cluster cations in the gas phase. Experiments are carried out using a quadrupole ion trap in combination with time-of-flight mass spectrometry. The results show that fullerene (C60 and C70)/anthracene (i.e., [(C14H10)
n
C60]+ and [(C14H10)
n
C70]+), fullerene (C56 and C58)/anthracene (i.e., [(C14H10)
n
C56]+ and [(C14H10)
n
C58]+), and fullerene (C66 and C68)/anthracene (i.e., [(C14H10)
n
C66]+ and [(C14H10)
n
C68]+) cluster cations, are formed in the gas phase through an ion–molecule reaction pathway. With irradiation, all the fullerene/anthracene cluster cations dissociate into monoanthracene and fullerene species without dehydrogenation. The structure of newly formed fullerene/anthracene cluster cations and the bonding energy for these reaction pathways are investigated with quantum chemistry calculations. Our results provide a growth route toward large fullerene derivatives in a bottom-up process and insight into their photoevolution behavior in the interstellar medium, and clearly, when conditions are favorable, fullerene/polycyclic aromatic hydrocarbon clusters can form efficiently. In addition, these clusters (from 80 to 154 atoms or ∼2 nm in size) offer a good model for understanding the physical–chemical processes involved in the formation and evolution of carbon dust grains in space, and provide candidates of interest for the diffuse interstellar bands that could motivate spectroscopic studies.
Observation of All Pre- and Post-reconnection Structures Involved in Three-dimensional Reconnection Geometries in Solar Eruptions
Authors: Dudík Jaroslav , Lörinčík Juraj , Aulanier Guillaume , Zemanová Alena , Schmieder Brigitte 
Published: December 2019

Abstract
We report on observations of the two newly identified reconnection geometries involving erupting flux ropes. In 3D, a flux rope can reconnect either with a surrounding coronal arcade (recently named “ar–rf” reconnection) or with itself (“rr–rf” reconnection), and both kinds of reconnection create a new flux-rope field line and a flare loop. For the first time, we identify all four constituents of both reconnections in a solar eruptive event, the filament eruption of 2011 June 7 observed by Solar Dynamics Observatory/Atmospheric Imaging Assembly. The ar–rf reconnection manifests itself as shift of one leg of the filament by more than 25″ northward. At its previous location, a flare arcade is formed, while the new location of the filament leg previously corresponded to a footpoint of a coronal loop in 171 Å. In addition, the evolution of the flare ribbon hooks is also consistent with the occurrence of ar–rf reconnection as predicted by MHD simulations. Specifically, the growing hook sweeps footpoints of preeruptive coronal arcades, and these locations become inside the hook. Furthermore, the rr–rf reconnection occurs during the peak phase above the flare arcade, in an apparently X-type geometry involving a pair of converging bright filament strands in the erupting filament. A new flare loop forms near the leg of one of the strands, while a bright blob, representing a remnant of the same strand, is seen ascending into the erupting filament. All together, these observations vindicate recent predictions of the 3D standard solar-flare model.
Modeling Energetic Particle Acceleration and Transport in a Solar Wind Region with Contracting and Reconnecting Small-scale Flux Ropes at Earth Orbit
Authors: Le Roux J. A. , Webb G. M. , Khabarova O. V. , Zhao L.-L. , Adhikari L. 
Published: December 2019

Abstract
New analytical steady-state and time-dependent solutions for the acceleration of energetic particles by contracting and reconnecting small-scale flux ropes (SMFRs) in the solar wind are presented. For this purpose, a telegrapher-type Parker transport equation was derived from the existing underlying focused transport equation. The solutions unify all SMFR acceleration mechanisms present in the transport equation, showing that SMFR acceleration by the reconnection electric field in the mixed-derivative transport term is constrained by and requires the presence of second-order Fermi SMFR acceleration. We explore the potential of these solutions in reproducing energetic proton flux enhancements and spectral evolution between ∼50 keV and 5 MeV in dynamic SMFR regions near large-scale reconnecting current sheets in the solar wind at Earth orbit. It is shown that second-order Fermi SMFR acceleration involving the variance in SMFR compression and incompressible parallel shear flow and confirmed that first-order SMFR Fermi acceleration, due to mean SMFR compression (successfully used before in data fits), are both workable options in reproducing observed flux amplification factors when using reasonable SMFR parameters. However, the predicted substantial quantitative differences in the spatial evolution of the accelerated spectra through the SMFR region might provide a way to distinguish between first- and second-order Fermi SMFR acceleration in observations. It is concluded that more detailed data analysis of SMFR parameters in SMFR acceleration events is needed before the relative role of first- and second-order SMFR acceleration mechanisms can be determined.
Nonstationary Fast-driven, Self-organized Criticality in Solar Flares
Authors: Aschwanden Markus J. 
Published: December 2019

Abstract
The original concept of self-organized criticality, applied to solar flare statistics, assumed a slow-driven and stationary flaring rate, which implies timescale separation (between flare durations and interflare waiting times). The concept reproduces power-law distributions for flare peak fluxes and durations, but predicts an exponential waiting time distribution. In contrast to these classical assumptions, we observe (i) multiple energy dissipation episodes during most flares, (ii) violation of the principle of timescale separation, (iii) a fast-driven and nonstationary flaring rate, (iv) a power-law distribution for waiting times Δt, with a slope of α
Δt
≈ 2.0, as predicted from the universal reciprocality between mean flaring rates and mean waiting times, and (v) pulses with rise times and decay times of the dissipated magnetic free energy on timescales of 12 ± 6 minutes, and up to 13 times in long-duration (≲4 hr) flares. These results are inconsistent with coronal long-term energy storage, but require photospheric–chromospheric current injections into the corona.
Mass–Metallicity Trends in Transiting Exoplanets from Atmospheric Abundances of H2O, Na, and K
Authors: Welbanks Luis , Madhusudhan Nikku , Allard Nicole F. , Hubeny Ivan , Spiegelman Fernand , Leininger Thierry 
Published: December 2019

Abstract
Atmospheric compositions can provide powerful diagnostics of formation and migration histories of planetary systems. We investigate constraints on atmospheric abundances of H2O, Na, and K, in a sample of transiting exoplanets using the latest transmission spectra and new H2 broadened opacities of Na and K. Our sample of 19 exoplanets spans from cool mini-Neptunes to hot Jupiters, with equilibrium temperatures between ∼300 and 2700 K. Using homogeneous Bayesian retrievals we report atmospheric abundances of Na, K, and H2O, and their detection significances, confirming 6 planets with strong Na detections, 6 with K, and 14 with H2O. We find a mass–metallicity trend of increasing H2O abundances with decreasing mass, spanning generally substellar values for gas giants and stellar/superstellar for Neptunes and mini-Neptunes. However, the overall trend in H2O abundances, from mini-Neptunes to hot Jupiters, is significantly lower than the mass–metallicity relation for carbon in the solar system giant planets and similar predictions for exoplanets. On the other hand, the Na and K abundances for the gas giants are stellar or superstellar, consistent with each other, and generally consistent with the solar system metallicity trend. The H2O abundances in hot gas giants are likely due to low oxygen abundances relative to other elements rather than low overall metallicities, and provide new constraints on their formation mechanisms. The differing trends in the abundances of species argue against the use of chemical equilibrium models with metallicity as one free parameter in atmospheric retrievals, as different elements can be differently enhanced.
Intelligence collective et organisation co-dépendante : le rôle de l’expert-comptable dans le crowdlending
Authors: Berkowitz Héloïse , Souchaud Antoine 
Published: December 2019

Quel rôle l’expert-comptable (EC) peut-il jouer dans l’exploitation de l’intelligence collective (IC) par le crowdlending, et à quelles conditions ? Cet article s’appuie sur une étude de cas approfondie d’une tentative inaboutie d’exploiter l’IC grâce à l’expertise-comptable dans le cadre d’un partenariat entre une plateforme de crowdlending et l’Ordre des Experts-Comptables. Nos résultats décrivent certaines actions de l’EC permettant d’activer diverses fonctions de l’intelligence collective sur les forums, en amont et en aval de la collecte. Mais l’article révèle aussi deux facteurs organisationnels d’échec de l’exploitation de cette ressource : le non-respect d’un principe de co-dépendance et l’hypocrisie organisationnelle. Cette analyse nous conduit à proposer un modèle élargi de co-dépendance entre plateforme, porteurs de projet, foule et experts-comptables dans le crowdlending, permettant une « ingénierie » de l’intelligence collective, c’est-à-dire son expression, sa transformation et son exploitation.
Discussion du rapport de Jean-Michel Lévy : Lumière et ombre ?
Authors: Deburge Anne 
Published: December 2019

À propos du rapport de Jean-Michel Lévy, l’auteur soulève un certain nombre de questions concernant le concept de bisexualité : la place du biologique et de l’environnement, le rapport entre théorie des pulsions et rôle de l’objet, tout particulièrement lors de l’assignation identitaire, le recours à la bisexualité chez les fonctionnements non névrotiques, les possibilités et les limites de la notion de bisexualité pour appréhender la sexualité de l’autre au cœur du couple homme/femme ou patient/analyste.
Modification du corps et bisexualité. De Lili Elbe à Paul B. Preciado
Authors: Lorenzon Schaffa Sandra 
Published: December 2019

Pour contribuer à la réflexion sur les questions de genre, l’auteure propose de suivre sur un siècle l’évolution des discours et des représentations et d’analyser l’impact de ces transformations sur les formations subjectives. En s’appuyant sur les témoignages de Lili Elbe et de Paul B. Preciado, l’auteure montre comment on est passé d’une conception absolument binaire à un refus des « assignations » produites par une culture commune.