bluuebunny/crossref_metadata_2025_split huggingface dataset:
FAKTOR PENGHAMBAT DALAM PENEGAKAN QANUN JINAYAT DI ACEH
Authors: Berutu Ali Geno 
Published: January 2019

Abstrak
Tulisan ini membuktikan bahwa pelaksanaan Qanun Aceh No. 14 Tahun 2003 tentang khalwat di Kota Subulussalam belum sepenuhnya berjalan dengan baik. Banyak kendala yang dihadapi baik dari pelaksananya (pemerintah) maupun masyarakat sebagai objek hukum penerapan syariat Islam itu sendiri. Faktor hukum yang merupakan salah satu faktor utama penyebab stagnan-nya penindakan terhadap pelanggar Qanun No. 14 Tahun 2003 di Kota Subulussalam disamping faktor-faktor lainnya. Tulisan ini berusaha menguraikan kendala dalam efektivitas penegakan hukum yang merupakan suatu indikator penilaian terhadap penegakan suatu hukum, dalam artian untuk mengukur keberhasilan atau target yang telah ditetapkan dalam penerapan suatu hukum khususnya terhadap penegakan Qanun No. 14 Tahun 2003 di wilayah hukum Kota Subulussalam, Aceh.

Kata kunci: Khalwat, Aceh, Syariat Islam, Jinayat, Subulussalam

Abstract
This paper proves that the implementation of Qanun Aceh no. 14 of 2003 on khalwat in Subulussalam city has not fully run well. Many obstacles faced both from the executor (government) and the community as the object of the law of the application of Islamic Shari'a itself. The legal factor is one of the main factors causing its stagnant action against the violation of Qanun. 14 Year 2003 in Subulussalam City in addition to other factors. This paper attempts to outline the obstacles in the effectiveness of law enforcement which is an indicator of the assessment of the enforcement of a law, in order to measure the success or targets set in the application of a law especially to the enforcement of Qanun. 14 Year 2003 in the jurisdiction of Subulussalam City, Aceh.

Keywords: Khalwat, Aceh, Syariat Islam, Jinayat, Subulussalam
ВПЛИВ ДОДАТКОВОГО ШТУЧНОГО ОСВІТЛЕННЯ НА ПОЧАТКОВІ ЕТАПИ РОСТУ ТА РОЗВИТКУ РОЗСАДИ ПОМІДОРА І ОГІРКА
Authors: Popovich H. B. , Malinina A. O. , Aksenyuk I. I. , Hrytsak R. V. 
Published: January 2019

Мета. Вивчення впливу додаткового штучного освітлення на початкові етапи росту та розвитку розсади огірка і помідора в умовах закритого ґрунту. Методи. Фенологічні спостереження, біометричні вимірювання, статистичні методи дослідження. Результати. Встановлено, що відмінності у швидкості росту гібридів помідора й огірка проявилися вже на ранніх етапах. Найбільш різкі відмінності спостерігали у помідора. У варіанті з досвічуванням вже на п’ятий день відмічали добре розвинені сім’ядольні листки, висота гіпокотиля при цьому становила в середньому 3,6 см, площа листкової поверхні першого справжнього листка – 3,08 см2. У той самий час у контролі рослини перебували на стадії розгортання сім’ядольних листків. У фазі двох – чотирьох справжніх листків як за висотою стебла, так і за площею листкової поверхні виділялася розсада варіанту з досвічуванням. Встановлено, що рослини при досвічуванні були більш вирівняні за висотою, мали міцне, сильно опушене, більшого діаметру стебло, сира маса рослин у середньому на 19% перевищувала варіант із природним освітленням. За фенологічними спостереженнями рослини огірка розвивалися майже однаково, за морфометричними даними рослини, які додатково досвічували, перевищували контроль. У фазі розгорнених сім’ядольних листків висота гіпокотиля в середньому на 23% перевищувала контроль. На цей період рослини обох варіантів досліду перебували на початковій стадії формування першого справжнього листка. У подальшому спостерігали значне прискорення росту в рослин, які додатково досвічували. У фазі двох справжніх листків висота рослин у досліді на 45% перевищувала контроль, а площа листкової поверхні – на 30%, товщина стебла при цьому у контролі на 7,9% була меншою. Висновки. Проведені дослідження свідчать про ефективність застосування світлодіодних фотоламп 30 Вт у весняний період для вирощування розсади в умовах закритого ґрунту. Протягом усього досліду у варіанті з додатковим досвічуванням у рослин помідора й огірка спостерігали прискорений ріст, більші висоту, площу поверхні листків та масу надземної частини. Крім того, при досвічуванні у рослин помідора одного віку спостерігали суттєві відмінності за темпами розвитку справжніх листків.
Distribution of Aedes aegypti and Aedes albopictus in different eco zones of Thiruvananthapuram city with special reference to dengue viremia in humans
Authors: Sunil Kumar S. , Evans D.A. , Muthulakshmi K. , DilipKumar T. , Heera Pillai R. , Nair R. Radhakrishnan , Sunny Francis 
Published: January 2019

Mosquito index study of three ecologically different ecozones of the Thiruvananthapuram district, Kerala showed sharp difference on the proportionate distribution of Aedes aegypti and Aedes albopictus. Human dengue viremia (HDV) was very high in those ecozones where A.aegypti density was high and HDV was low where A.albopictus was high. In a coastal zone of Thiruvananthapuram city, A. aegypti was the most abundant vector and in a hilly, arid suburban zone, A.albopictus was the abundant vector. In the urban zone both species of mosquitoes showed equal distribution. Study on the circulating serotypes in the serum of HDV by Single step single tube Multiplex PCR showed all the four serotypes viz DENV1, DENV2, DENV3 and DENV4 in patients of Thiruvananthapuram city, which indicated the possibility of Dengue Shock Syndrome, unless there is efficient vector management. Among the four dengue serotypes, Type 1 was the most abundant virus. Abundance of microhabitats in Thiruvananthapuram city, which support A. aegypti may be the reason for high prevalence of dengue fever in the urban zone.
AGN Feedback in Galaxy Groups: A Detailed Study of X-Ray Features and Diffuse Radio Emission in IC 1262
Authors: Pandge M. B. , Sonkamble S. S. , Parekh Viral , Dabhade Pratik , Parmar Avni , Patil M. K. , Raychaudhury Somak 
Published: January 2019

Abstract
This paper reports a systematic search of X-ray cavities, density jumps, and shocks in the intergalactic environment of the galaxy group IC 1262 using Chandra, GMRT, and Very Large Array archival observations. The X-ray imaging analysis reveals a pair of X-ray cavities to the north and south of the X-ray peak, at projected distances of 6.48 kpc and 6.30 kpc respectively. Total mechanical power contained in both of these cavities is found to be ∼12.37 × 1042 erg s−1, and compares well with the X-ray luminosity, within the cooling radius, measured to be ∼3.29 × 1042 erg s−1, suggesting that the mechanical power injected by the central AGN efficiently balances the radiative loss. We detect a previously unknown X-ray cavity at the position of the southern radio lobe in the intra-group medium and find a loop of excess X-ray emission extending ∼100 kpc southwest from the central galaxy. The X-ray cavity at the position of the southern radio lobe probably represents a first generation X-ray cavity. Two surface brightness edges are evident to the west and northeast of the center of this group. The radio galaxy at the core of the IC 1262 group is a rare low-redshift ultra-steep radio galaxy, its spectral index being α ∼ −1.73 (including the central AGN) and α ∼ −2.08 (excluding the central AGN). We detect a radio phoenix embedded within the southern radio lobe, for the first time in a poor group, with a spectral index (α ≤ −1.92). The spectral index distribution across the phoenix steepens with increasing distance from its intensity peak.
A Study of the Merger History of the Galaxy Group HCG 62 Based on X-Ray Observations and Smoothed Particle Hydrodynamic Simulations
Authors: Hu Dan , Xu Haiguang , Kang Xi , Li Weitian , Zhu Zhenghao , Ma Zhixian , Shan Chenxi , Zhang Zhongli , Gu Liyi , Liu Chengze , Zheng Qian , Wu Xiang-ping 
Published: January 2019

Abstract
We chose the bright compact group HCG 62, which has been found to exhibit both excess X-ray emission and high Fe abundance to the southwest of its core, as an example to study the impact of mergers on chemical enrichment in the intragroup medium. We first reanalyze the high-quality Chandra and XMM-Newton archive data to search for evidence of additional SN II yields, which is expected to be a direct result of the possible merger-induced starburst. We reveal that, similar to the Fe abundance, the Mg abundance also shows a high value in both the innermost region and the southwest substructure, forming a high-abundance plateau. Meanwhile, all the SN Ia and SN II yields show rather flat distributions in >0.1r
200 in favor of an early enrichment. Then, we carry out a series of idealized numerical simulations to model the collision of two initially isolated galaxy groups by using the TreePM-SPH GADGET-3 code. We find that the observed X-ray emission and metal distributions, as well as the relative positions of the two bright central galaxies with reference to the X-ray peak, can be well reproduced in a major merger with a mass ratio of 3 when the merger-induced starburst is assumed. The “best-match” snapshot is pinpointed after the third pericentric passage when the southwest substructure is formed due to gas sloshing. By following the evolution of the simulated merging system, we conclude that the effects of such a major merger on chemical enrichment are mostly restricted to within the core region when the final relaxed state is reached.
Compton-thick AGNs in the NuSTAR Era. II. A Deep NuSTAR and XMM-Newton View of the Candidate Compton-thick AGN in NGC 1358
Authors: Zhao X. , Marchesi S. , Ajello M. , Marcotulli L. , Cusumano G. , Parola V. La , Vignali C. 
Published: January 2019

Abstract
We present the combined NuSTAR and XMM-Newton 0.6–79 keV spectral analysis of a Seyfert 2 galaxy, NGC 1358, which we selected as a candidate Compton-thick (CT) active galactic nucleus (AGN) on the basis of previous Swift/BAT and Chandra studies. According to our analysis, NGC 1358 is confirmed to be a CT-AGN using physically motivated models, at >3σ confidence level. Our best fit shows that the column density along the line of sight of the obscuring material surrounding the accreting supermassive black hole is N
H = (1.96–2.80) × 1024 cm−2. The high-quality data from NuSTAR give the best constraints on the spectral shape above ∼10 keV to date on NGC 1358. Moreover, by combining NuSTAR and XMM-Newton data, we find that the obscuring torus has a low covering factor (f

c
< 0.17), and the obscuring material is distributed in clumps, rather than uniformly. We also derive an estimate of NGC 1358's Eddington ratio, finding it to be λ
Edd ∼

× 10−2, which is in acceptable agreement with previous measurements. Finally, we find no evidence of short-term variability, over a ∼100 ks time span, in terms of both line-of-sight column density and flux.
Energetic Neutral Atoms from the Heliosheath as an Additional Population of Neutral Hydrogen in the Inner Heliosphere
Authors: Bzowski M. , Galli A. 
Published: January 2019

Abstract
Interstellar neutral hydrogen (ISN H) gas penetrates freely the heliopause. Inside the inner heliosheath, the charge-exchange interaction of this gas with the shocked solar wind and pickup ions creates energetic neutral atoms (ENAs). ISN H is strongly depleted inside the termination shock but a fraction reaches the Earth’s orbit. In these regions of the heliosphere, ISN H is the source population for interstellar pickup ions and for the heliospheric backscatter glow. The globally distributed flux (GDF) of ENAs created in the inner heliosheath has been sampled directly by the Interstellar Boundary Explorer. Based on these measurements, we calculate the density of the GDF ENA population at the Earth’s orbit. We find that this number density is between 10−4 and 10−3 cm−3, i.e., comparable in magnitude to the number density of ISN H in the downwind portion of the Earth’s orbit. Half of this atom population has energies less than ∼80 eV. This GDF population of neutral hydrogen is likely to provide a significant contribution to the intensity of heliospheric glow in the downwind hemisphere, may be the source of the inner source of hydrogen pickup ions, and may be responsible for the excess of production of pickup ions found in the analysis of magnetic wave events induced by the proton pickup process in the downwind region at 1 au from the Sun.
An Enormous Molecular Gas Flow in the RX J0821+0752 Galaxy Cluster
Authors: Vantyghem A. N. , McNamara B. R. , Russell H. R. , Edge A. C. , Nulsen P. E. J. , Combes F. , Fabian A. C. , McDonald M. , Salomé P. 
Published: January 2019

Abstract
We present recent Chandra X-ray observations of the RX J0821.0+0752 galaxy cluster, in addition to ALMA observations of the CO(1–0) and CO(3–2) line emission tracing the molecular gas in its central galaxy. All of the CO line emission, originating from a

molecular gas reservoir, is located several kiloparsecs away from the nucleus of the central galaxy. The cold gas is concentrated into two main clumps surrounded by a diffuse envelope. They form a wide filament coincident with a plume of bright X-ray emission emanating from the cluster core. This plume encompasses a putative X-ray cavity that is only large enough to have uplifted a small percent of the molecular gas. Unlike other brightest cluster galaxies, stimulated cooling, where X-ray cavities lift low-entropy cluster gas until it becomes thermally unstable, cannot have produced the observed gas reservoir. Instead, the molecular gas has likely formed as a result of sloshing motions in the intracluster medium induced by a nearby galaxy. Sloshing can emulate uplift by dislodging gas from the galactic center. This gas has the shortest cooling time, so it will condense if disrupted for long enough.
Bright Gamma-Ray Flares Powered by Magnetic Reconnection in QED-strength Magnetic Fields
Authors: Schoeffler K. M. , Grismayer T. , Uzdensky D. , Fonseca R. A. , Silva L. O. 
Published: January 2019

Abstract
Strong magnetic fields in the magnetospheres of neutron stars (NSs) (especially magnetars) and other astrophysical objects may release their energy in violent, intense episodes of magnetic reconnection. While reconnection has been studied extensively, the extreme field strength near NSs introduces new effects: radiation cooling and electron–positron pair production. Using massively parallel particle-in-cell simulations that self-consistently incorporate these new radiation and quantum-electrodynamic effects, we investigate relativistic magnetic reconnection in the strong-field regime. We show that reconnection in this regime can efficiently convert magnetic energy to X-ray and gamma-ray radiation and thus power bright, high-energy astrophysical flares. Rapid radiative cooling causes strong plasma and magnetic field compression in compact plasmoids. In the most extreme cases, the field can approach the quantum limit, leading to copious pair production.
Heating Effects from Driven Transverse and Alfvén Waves in Coronal Loops
Authors: Guo Mingzhe , Van Doorsselaere Tom , Karampelas Konstantinos , Li Bo , Antolin Patrick , De Moortel Ineke 
Published: January 2019

Abstract
Recent numerical studies revealed that transverse motions of coronal loops can induce the Kelvin–Helmholtz instability (KHI). This process could be important in coronal heating because it leads to dissipation of energy at small spatial scale plasma interactions. Meanwhile, small-amplitude decayless oscillations in coronal loops have been discovered recently in observations of SDO/AIA. We model such oscillations in coronal loops and study wave heating effects, considering a kink and Alfvén driver separately and a mixed driver at the bottom of flux tubes. Both the transverse and Alfvén oscillations can lead to the KHI. Meanwhile, the Alfvén oscillations established in loops will experience phase mixing. Both processes will generate small spatial scale structures, which can help the dissipation of wave energy. Indeed, we observe the increase of internal energy and temperature in loop regions. The heating is more pronounced for the simulation containing the mixed kink and Alfvén driver. This means that the mixed wave modes can lead to a more efficient energy dissipation in the turbulent state of the plasma and that the KHI eddies act as an agent to dissipate energy in other wave modes. Furthermore, we also obtained forward-modeling results using the FoMo code. We obtained forward models that are very similar to the observations of decayless oscillations. Due to the limited resolution of instruments, neither Alfvén modes nor the fine structures are observable. Therefore, this numerical study shows that Alfvén modes probably can coexist with kink modes, leading to enhanced heating.
The Pain Game: Pain Assessment, Management, and Related JCAHO Standards
Authors: Morton Paula G , Tarvin Leslie 
Published: January 2019

ABSTRACT
Background: It is a challenge to educators to assist nursing staff in maintaining up-to-date knowledge of pain assessment and management.
Method: A learning game, "The Pain Game/' was developed to deliver information on current practices and standards related to patient pain assessment and management.
Results: The advantages of using this gaming technique included minimal instructor preparation time, low cost materials, inclusion of participants as peer teachers, and a high level of participant involvement in the learning process.
Conclusions: The Pain Game has been a wellreceived educational activity. Not only did knowledge acquisition occur, but the game also provided an enjoyable alternative to more traditional content delivery methods.
Immune Responses to Avian Influenza Viruses
Authors: Koutsakos Marios , Kedzierska Katherine , Subbarao Kanta 
Published: January 2019

Abstract
Avian influenza A viruses (IAVs) naturally infect different avian species, and aquatic birds are their natural reservoir. Sporadically, avian IAVs can be transmitted to humans, and some, such as H5N1 and H7N9 viruses, cause severe disease in humans. Antigenically novel avian influenza viruses that infect and cause disease in humans pose a potential pandemic threat if they are able to spread efficiently from person to person. The immune response of the host is crucial in determining disease pathogenesis and is the basis for the development of control strategies. In this review, we examine the innate and adaptive immune responses to avian influenza viruses and their role in disease and recovery. Furthermore, we discuss the progress in developing vaccines against avian IAVs and summarize obstacles in designing universal and pandemic influenza vaccines.
Influenza Virus–Specific Human Antibody Repertoire Studies
Authors: Crowe James E. 
Published: January 2019

Abstract
The diversity of Ag-specific adaptive receptors on the surface of B cells and in the population of secreted Abs is enormous, but increasingly, we are acquiring the technical capability to interrogate Ab repertoires in great detail. These Ab technologies have been especially pointed at understanding the complex issues of immunity to infection and disease caused by influenza virus, one of the most common and vexing medical problems in man. Influenza immunity is particularly interesting as a model system because the antigenic diversity of influenza strains and proteins is high and constantly evolving. Discovery of canonical features in the subset of the influenza repertoire response that is broadly reactive for diverse influenza strains has spurred the recent optimism for creating universal influenza vaccines. Using new technologies for sequencing Ab repertoires at great depth is helping us to understand the central features of influenza immunity.
A Simulation-Based Workshop to Improve Residents' Collaborative Clinical Practice
Authors: Crawford Scott B. , Monks Stormy M. , Mendez Melissa , Quest Dale , Mulla Zuber D. , Plavsic Sanja Kupesic 
Published: January 2019

ABSTRACT

Background
The Accreditation Council for Graduate Medical Education expects residents to attain competency in systems-based practice by advocating for quality patient care, working in interprofessional teams, and implementing system solutions to prevent errors. Diabetes in pregnancy was identified as an area for improvement through comprehensive interdisciplinary and interprofessional care.

Objective
An interdisciplinary and interprofessional workshop was created by 3 regional academic institutions to improve collaborative practice, clinical knowledge, and clinical judgment of residents.

Methods
A workshop consisting of 4 clinical simulation stations for ultrasound assessment, glycemic control, hyperglycemic emergencies, and macrosomia complications was designed to address gaps in quality of care. Workshop participants were residents from 6 programs and students in nursing, pharmacy, and sonography. Attitude and clinical knowledge were measured preworkshop and postworkshop, and at 3-month and 6- to 7-month follow-up.

Results
There were increases in average clinical knowledge scores across time points from residents: 56.4% preworkshop, 64.8% postworkshop, 66.0% at 3-month follow-up, and 68.1% at 6- to 7-month follow-up. Additionally, participants reported positive attitudes toward interprofessional education and indicated high overall satisfaction.

Conclusions
Residents demonstrated improved knowledge and attitudes toward interprofessional training after participating in a large-scale simulation workshop focused on the care of patients with diabetes in pregnancy.
O Cartel Psicanalítico e os Limites de sua Escala Lógica
Authors: Ferreira Patrícia Do Prado 
Published: January 2019

A proposta deste trabalho é abordar o limite de escala lógica do cartel. Esse dispositivo de transmissão é proposto por Jacques Lacan e chamado de “órgão de base” do funcionamento de sua Escola. O cartel pode ser entendido como uma forma coletiva que emerge de diversas tentativas – inclusive fracassadas – de constituição que se estrutura para-além dos efeitos de ‘grupo’ descritos por Freud em Psicologia das massas e análise do eu. Portanto, objetiva-se que o cartel escape às tradicionais estruturas hierárquicas e verticalizadas, além de tentar esvaziar o sentido das identificações entre os pares e do ‘Um ideal’. Para tanto, a proposta é de um arranjo lógico limitado a 4+1, em que os membros do cartel se reúnam em torno de um tema (que funcionaria como elo entre o pequeno grupo), apresentando um argumento de trabalho que simultaneamente faz o grupo – uma vez que os membros estão articulados por uma produção de saber, uma tarefa – e particulariza a questão. Pensando com base na teoria dos discursos (que se utiliza de matemas para demonstrar os engendramentos dos laços sociais) proposta por Lacan em 1969-70, a estrutura de um cartel pode ser associada a uma inscrição no discurso do analista. Os outros discursos – do mestre, do universitário e da histérica – de certo modo mapeiam o aparelhamento de gozo de maneira indiferente às escalas sociais. A qualificação ‘numérica’ do cartel é pouco estudada na psicanálise e, em nosso entender, diz de um compromisso implícito da teoria lacaniana com certas teses da filosofia política e da sociologia a respeito da origem dos fenômenos de massa. Partindo-se dessas idéias é que nos perguntamos o que seria um ‘laço pelo discurso analítico’ que não corroborasse com esse corolário restritivo, que, ao contrário dos outros discursos, incide sobre a escala do laço social. Tentamos nos servir da psicanálise – sobretudo da proposta lacaniana do cartel – para pensarmos na estrutura grupal como também potencialmente emancipatória. Acreditamos que isso está posto no fundamento do ‘órgão basal’ da Escola, ao sugerir pensar para-além da alienação grupal.