bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENGARUH FAKTOR-FAKTOR SPIP TERHADAP KUALITAS LAPORAN KEUANGAN PEMERINTAH KOTAMADYA BANDA ACEH
Authors: - Irmawati 
Published: January 2021

Penelitian ini bertujuan untuk mengetahui faktor-faktor SPIP terhadap kualitas laporan keuangan pemerintah Kotamadya Banda Aceh. Responden penelitian ini sebanyak 52 orang yang terdiri dari: Kuasa Pengguna Anggaran dan PPK (Pejabat Penatausahaan Keuangan). Metode yang digunakan dalam penelitian ini adalah metode sensus yaitu seluruh elemen populasi diselidiki satu persatu dalam pengumpulan data. Metode analisis yang digunakan adalah regresi linier berganda.Hasil penelitian menunjukkan bahwa lingkungan pengendalian, aktivitas pengendalian, penilaian resiko, informasi dan komunikasi dan pemantauan secara bersama-sama dan sendiri-sendiri berpengaruh kualitas laporan keuangan pemerintah Kotamadya Banda AcehÂ Kata kunci: Lingkungan pengendalian, aktvitas pengendalian, penilaian resiko, kualitas laporan keuangan.
Pengaruh Kompetensi Terhadap Kinerja Dosen Universitas Muhammadiyah Aceh
Authors: Gadeng Tarmizi 
Published: January 2021

Tujuan utama dari penelitian ini adalah untuk menguji dan menganalisis pengaruh Kompetensi Pedagogik, Kompetensi Profesional, Kompetensi Kepribadian dan Kompetensi Sosial terhadap kenerja dosen Universitas Muhammadiyah Aceh.
Populasi dalam penelitian ini adalah dua ratus delapan puluh lima orang dosen dan mengambil tiga puluh lima persen sebagai sampel yaitu sebanyak seratus orang dosen Universitas Muhammadiyah Aceh.
Alat ukur yang digunakan adalah dengan menggunakan regresi linear berganda, dari penelitian menghasilkan persamaan sebagai berikut : Y = 0,940+0,149X1+0,319X2+0,325X3+0,046X4+e
Hasil yang diperoleh dari penelitian ini adalah secara parsial kompetensi pedagogic berpengaruh secara signifikan terhadap kinerja dosen universitas Muhammadiyah Aceh, kompetensi professional berpengaruh secara signifikan terhadap kinerja dosen Universitas Muhammadiyah Aceh, kompetensi kepribadian berpengaruh secara signifikan terhadap kinerja dosen Universitas Muhammdiyah Aceh dan kompetensi Sosial tidak berpengaruh secara signifikan terhadap kinerja dosen Universitas Muhammadiyah Aceh. Dan Secara simultan kompetensi berpengaruh terhadap kinerja dosen Universitas Muhammadiyah Aceh
Kata kunci : Kompetensi Pedagogik, Profesional, Kepribadian dan Sosial.
ANALISIS KINERJA KEUANGAN PADA PT. ASURANSI JASA INDONESIA (PERSERO) CABANG BANDA ACEH PERIODE 2013-2015
Authors: Syamsidar Syamsidar , Jawiyah Jawiyah 
Published: January 2021

Tujuan dari penelitian ini adalah untuk mengetahui kinerja keuangan pada PT Asuransi Jasa Indonesia (Persero) Cabang Banda Aceh periode 2013-2015 ditinjau dari rasio likuiditas, solvabilitas dan rentabilitas. Data penelitian ini merupakan pooled data yang bersifat kuantitatif yang dikumpulkan menggunakan teknik library research, yang kemudian diolah dan dianalisis secara deskriptif.Â Â Â Â Â Â Â Â Â Kesimpulan yang bisa diambil dari hasil analisis penelitian ini bahwa secara keseluruhan kinerja keuangan PT. Asuransi Jasa Indonesia (Persero) Cabang Banda Aceh berada pada kriteria sangat baik. Kinerja keuangan berdasarkan current ratio, Debt to Total Assets RatioÂ (DAR), Long Term Debt to Equity Rasio, dan Return on Equity berada pada kriteria sangat baik berturut-turut selama 3 tahun (2013-2015). Sedangkan kinerja berdasarkan cash ratio, kondisi keuangan PT. Asuransi Jasindo Cabang Banda Aceh berada pada kriteria buruk selama 3 tahun berturut-turut (2013-2015).
READING IN THE RUSSIAN LANGUAGE TEACHING OF BI-LINGUAL CHILDREN OUTSIDE RUSSIA
Authors: Запрометова Е.С. 
Published: January 2021

В статье рассматриваются вопросы, связанные с чтением и выбором текстов при обучении русскому языку детей-билингвов. Особое внимание уделено тому, какие жанры литературы привлекают детей сегодня и что нравится читать детям-билингвам младшего и среднего школьного возраста. Основываясь на собственном опыте воспитания двух детей-билингвов и опыте знакомых мам, автор разбирает данный вопрос и предлагает некоторые советы родителям и учителям при выборе текстов для чтения и работы с ними.
The article studies the role of reading the russian literature in the bilingual families living outside Russia. It recommands which texts arent necessary for bilingual children.
PENGEMBANGAN KONFIGURASI HOTSPOT DAN VOUCHER LOGIN MENGGUNAKAN MIKROTIK RB952ui DENGAN WEB TOP UP (STUDI KASUS : NORALONA COFFEE ROASTERY)
Authors: Romadon Indra 
Published: January 2021

The current internet access needs are very high, both to find the latest information, articles and seek entertainment. There are several places that provide internet access, one of which is a coffee shop. Many coffee shops implement Wi-fi facilities as a service to attract customers. Noralona Coffee and Roastery is a coffee shop located in the city of Cirebon that provides Wi-fi facilities for its customers. Wi-fi facilities available at the coffee shop have not restricted user access to the internet. One of them uses a hotspot and the calculation of hotspot access is done using a voucher system. Hotspot with this voucher system will be configured with MikroTik. On the proxy there is a hotspot service feature, then there are additional features, namely User Manager, which is a web interface for hotspot management. Vouchers are calculated based on time. and each voucher can be used by 1 user. This study aims to produce hotspot vouchers that can be topped up through the hotspot login website to make it easier for consumers to use Wi-fi, do top ups and reduce the use of ¬ Wi-fi that is too long for each visitor. The results of this study indicate that in a time-limited and user-vouched test, users cannot log in if the voucher is being used by 1 user, and if the voucher deadline has expired, the voucher can be Top Up again and consumers can only Top Up 1x voucher in a day.
Keywords : Hotspot, Voucher, User Manager, Web Top Up, Top Up Voucher
Potential of Multispectral Satellite Data for Superficial Iron Oxide Detection in Sulaimaniyah, Iraqi Kurdistan Region
Authors: Al-Quraishi Ayad , Mustafa Banaz , Gopinathan P. , Yuvaraj Divya 
Published: January 2021

This study primarily investigates the total (Fe) iron presence in Sulaimaniyah Governorate, the Iraqi Kurdistan Region (IKR), which has an abundance of iron mines. Spatial quantification and frequent monitoring of mineral existence in the soil are essential in the mining regions. To achieve this goal, a remote sensing technique was utilized to predict soil minerals, particularly iron existence in the study area using a multispectral satellite image, Landsat-7 Enhanced Thematic Mapper Plus (ETM+). A robust methodology was perceived and developed from image processing to estimate and map iron oxides rich soils, and soil’s spectral indices were obtained after algorithms applied in processing on the bands of Landsat image. Soil samples were collected and analyzed in the laboratory to determine the chemical, physical, and mineralogical characteristics of soils. Correlation coefficients were carried out between soil properties and spectral band values retrieved from image analysis to examine the band potentials of Landsat. The statistical results showed that there was a significant relationship between the 3rd band of the ETM+ image and each of the total iron (R2 = 0.643), the free iron oxide (R2 = 0.659), and sand particles (R2 = 0.561). The predicted soil mineral maps were generated for the study area to visualize the study site's soil characterization and total iron spread. This study results could help primarily identify the spatial distribution of some soil properties in Sulaimaniyah, Iraq.
Methods for Comprehensive Analysis of the Economic Effectiveness of Business Activities
Authors: Kim Gang-Sok , Kim Gwang-Ik , Rim Gwang-Nam , Jang Sun-Nam 
Published: January 2021

Purpose: This paper suggests the methodology for comprehensively and dynamically evaluating the economic effectiveness of business activities in a view of scientific and technological development.
Methods: Authors analyze the previous studies related to evaluating the economic effectiveness of business activities and suggest the methodology using the weight coefficients and pair-evaluation standards.
Results: The findings reveal that comprehensive economic effectiveness of business activities reflects the effective use of various resources including labor, material, fixed asset, liquid materials, and R&D expenditure into the business activities in a certain period of time and it must be assessed by using the integrated indicator.
Implications: The findings may contribute to the theories related to the economic effectiveness of business activities. It is also likely to improve organizational decision-making.
The K2 M67 Study: Precise Mass for a Turnoff Star in the Old Open Cluster M67
Authors: Sandquist Eric L. , Latham David W. , Mathieu Robert D. , Leiner Emily , Vanderburg Andrew , Stello Dennis , Orosz Jerome A. , Bedin Luigi R. , Libralato Mattia , Malavolta Luca , Nardiello Domenico 
Published: January 2021

Abstract
We present a study of the bright detached eclipsing main-sequence binary WOCS 11028 (Sanders 617) in the open cluster M67. Although the binary has only one eclipse per orbital cycle, we show that the masses of the stars can be derived very precisely thanks to a strong constraint on the orbital inclination: M

A
= 1.222 ± 0.006M
⊙ and M

B
= 0.909 ± 0.004M
⊙. We use a spectral energy distribution fitting method to derive characteristics of the component stars in lieu of the precise radii that would normally be derived from a doubly eclipsing binary. The deconvolution of the SEDs reveals that the brighter component of the binary is at the faint turnoff point for the cluster—a distinct evolutionary point that occurs after the convective core has been established and while the star is in the middle of its movement toward lower surface temperatures, before the so-called hook at the end of the main sequence. The measurements are in distinct disagreement with evolution models at solar metallicity: higher metal abundances are needed to reproduce the characteristics of WOCS 11028 A. We discuss the changes to model physics that are likely to be needed to address the discrepancies. The clearest conclusions are that diffusion is probably necessary to reconcile spectroscopic abundances of M67 stars with the need for higher metallicity models and that reduced strength convective overshooting is occurring for stars at the turnoff. At super-solar bulk metallicity, various indicators agree on a cluster age between about 3.5 and 4.0 Gyr.
On the Occurrence of Type IV Solar Radio Bursts in Solar Cycle 24 and Their Association with Coronal Mass Ejections
Authors: Kumari Anshu , Morosan D. E. , Kilpua E. K. J. 
Published: January 2021

Abstract
Solar activities, in particular coronal mass ejections (CMEs), are often accompanied by bursts of radiation at meter wavelengths. Some of these bursts have a long duration and extend over a wide frequency band, namely, type IV radio bursts. However, the association of type IV bursts with CMEs is still not well understood. In this article, we perform the first statistical study of type IV solar radio bursts in solar cycle 24. Our study includes a total of 446 type IV radio bursts that occurred during this cycle. Our results show that a clear majority, ∼81% of type IV bursts, were accompanied by CMEs, based on a temporal association with white-light CME observations. However, we found that only ∼2.2% of the CMEs are accompanied by type IV radio bursts. We categorized the type IV bursts as moving or stationary based on their spectral characteristics and found that only ∼18% of the total type IV bursts in this study were moving type IV bursts. Our study suggests that type IV bursts can occur with both “Fast” (≥500 km s−1) and “Slow” (<500 km s−1), and also both “Wide” (≥60°) and “Narrow” (<60°), CMEs. However, the moving type IV bursts in our study were mostly associated with “Fast” and “Wide” CMEs (∼52%), similar to type II radio bursts. Contrary to type II bursts, stationary type IV bursts have a more uniform association with all CME types.
Statistical Properties of Superflares on Solar-type Stars: Results Using All of the Kepler Primary Mission Data
Authors: Okamoto Soshi , Notsu Yuta , Maehara Hiroyuki , Namekata Kosuke , Honda Satoshi , Ikuta Kai , Nogami Daisaku , Shibata Kazunari 
Published: January 2021

Abstract
We report the latest statistical analyses of superflares on solar-type (G-type main-sequence; effective temperature is 5100–6000 K) stars using all of the Kepler primary mission data and Gaia Data Release 2 catalog. We updated the flare detection method from our previous studies by using a high-pass filter to remove rotational variations caused by starspots. We also examined the sample biases on the frequency of superflares, taking into account gyrochronology and flare detection completeness. The sample sizes of solar-type and Sun-like stars (effective temperature is 5600–6000 K and rotation period is over 20 days in solar-type stars) are ∼4 and ∼12 times, respectively, compared with Notsu et al. As a result, we found 2341 superflares on 265 solar-type stars and 26 superflares on 15 Sun-like stars; the former increased from 527 to 2341 and the latter from three to 26 events compared with our previous study. This enabled us to have a more well-established view on the statistical properties of superflares. The observed upper limit of the flare energy decreases as the rotation period increases in solar-type stars. The frequency of superflares decreases as the stellar rotation period increases. The maximum energy we found on Sun-like stars is 4 × 1034 erg. Our analysis of Sun-like stars suggests that the Sun can cause superflares with energies of ∼7 × 1033 erg (∼X700-class flares) and ∼1 × 1034 erg (∼X1000-class flares) once every ∼3000 and ∼6000 yr, respectively.
Dust Temperature of Compact Star-forming Galaxies at z ∼ 1–3 in 3D-HST/CANDELS
Authors: Chen Zuyi , Fang Guanwen , Lin Zesen , Zhang Hongxin , Chen Guangwen , Kong Xu 
Published: January 2021

Abstract
Recent simulation studies suggest that the compaction of star-forming galaxies (SFGs) at high redshift might be a critical process, during which the central bulge is being rapidly built, followed by quenching of the star formation. To explore dust properties of SFGs with compact morphology, we investigate the dependence of dust temperature, T
dust, on their size and star formation activity, using a sample of massive SFGs with

at 1 < z < 3, drawn from the 3D-HST/CANDELS database in combination with deep Herschel observations. T
dust is derived via fitting the mid-to-far-infrared photometry with a mid-infrared power law and a far-infrared modified blackbody. We find that both extended and compact SFGs generally follow a similar T
dust − z evolutionary track as that of the main-sequence galaxies. The compact SFGs seem to share similar dust temperature with extended SFGs. Despite the frequent occurrence of active galactic nuclei (AGNs) in compact SFGs, we do not observe any effect on dust caused by the presence of AGNs in these galaxies during the compaction. Our results disfavor different ISM properties between compact and extended SFGs, suggesting that a rapid and violent compaction process might be not necessary for the formation of compact SFGs.
Torsional Alfvén Wave Cascade and Shocks Evolving in Solar Jets
Authors: Farahani S. Vasheghani , Hejazi S. M. , Boroomand M. R. 
Published: January 2021

Abstract
The aim of this study is to model the nature of nonlinear torsional magnetohydrodynamic waves propagating in solar jets as they are elevated to the outer solar atmosphere. The contribution of sequential processes to the transfer of energy is taken under consideration: the nonlinear cascade and shock formation. Thus a straight magnetic cylinder embedded in a plasma with an initial magnetic field and parallel flow to the cylinder axis is implemented. To resemble a jet where the oscillation wavelength highly exceeds the radius, the second-order thin flux tube approximation proves adequate. A Cohen–Kulsrud type equation is presented, and its solution highly depends on the parameter presented in this study, which itself is constituted of various environmental and equilibrium conditions that affect the perturbations of the variables as well as the nonlinear forces connected to Alfvén wave propagation. The shock formation time of torsional waves is inversely proportional to the density contrast of the jet, while the efficiency of energy transfer to shorter scales is directly proportional to the density contrast. While the parallel flow with a shear at the boundary expedites shock formation, its efficiency regarding energy transfer is dramatically enhanced by the plasma-β, significantly contributing to coronal heating. The observational and seismological aspect of the present study is that faster jets are less probable for observations at higher altitudes, as they experience energy transfer mostly at the base of the corona, while slow speed jets may be observed at higher altitudes contributing to solar wind acceleration.
Properties of Galaxies in Cosmic Filaments around the Virgo Cluster
Authors: Lee Youngdae , Kim Suk , Rey Soo-Chang , Chung Jiwon 
Published: January 2021

Abstract
We present the properties of galaxies in filaments around the Virgo cluster with respect to their vertical distance from the filament spine using the NASA–Sloan Atlas catalog. The filaments are mainly composed of low-mass, blue dwarf galaxies. We observe that the g − r color of galaxies becomes blue and stellar mass decreases with increasing vertical filament distance. The galaxies were divided into higher-mass (

) and lower-mass (

) subsamples. We also examine the distributions of g − r color, stellar mass, Hα equivalent width (EW(Hα)), near-ultraviolet (NUV) − r color, and H i fraction of the two subsamples with the vertical distance. The lower-mass galaxies exhibit a negative g − r color gradient, whereas higher-mass galaxies have a flat g − r color distribution. We observe a negative EW(Hα) gradient for higher-mass galaxies, whereas lower-mass galaxies show no distinct EW(Hα) variation. In contrast, the NUV − r color distribution of higher-mass galaxies shows no strong trend, whereas the lower-mass galaxies show a negative NUV − r color gradient. We do not see clear gradients of H i fraction in either the higher- or lower-mass subsample. We propose that the negative color and stellar mass gradients of galaxies can be explained by mass assembly from past galaxy mergers at different vertical filament distances. In addition, galaxy interactions might be responsible for the contrasting features of EW(Hα) and NUV − r color distributions between the higher- and lower-mass subsamples. The distributions of H i fraction of the two subsamples suggest that the processes of ram pressure stripping and gas accretion may be ignored in the Virgo filaments.
Épreuves révolutionnaires
Authors: Lancereau Guillaume 
Published: January 2021

Au gré des bouleversements des premières années de la Révolution, les identités, hiérarchies et autres catégories de l’entendement social admises sous l’Ancien Régime n’ont soudainement plus cours, sans qu’aucun ordre stable et lisible ne vienne immédiatement s’y substituer. Parmi d’autres catégories sociales, les pédagogues de la Révolution présentent un profil spécifique. Les velléités parlementaires de régénération de la nation par le truchement de ses enseignants, dont témoignent de célèbres discours d’assemblée, n’aboutissent qu’à une législation mouvante et contradictoire, abandonnée aussitôt que triomphalement adoptée. L’incertitude généralisée qui en résulte engendre une floraison d’adresses aux assemblées successives ou à leur Comité d’Instruction publique, portées par des citoyens soucieux de négocier leur statut social ou le maintien de leur état. Ces suppliques et pétitions, mobilisant des formes complexes de valorisation et de mise en récit de soi, traduisent ainsi des demandes explicites ou implicites visant à prémunir leur auteur contre les risques de déclassement ou à justifier une bifurcation de trajectoire, et plongent ainsi l’historien au cœur de l’expérience vécue des bouleversements sociaux de l’ère révolutionnaire.
The Annual Institutional Review—Key Performance Measures and Processes
Authors: Amos Shayla , Wiggins Jean B. , Shaw Eric K. , Hannah William N. 
Published: January 2021

ABSTRACT

Background
The Accreditation Council for Graduate Medical Education (ACGME) requires sponsoring institutions to demonstrate effective oversight through an annual institutional review (AIR). The ACGME only requires 3 elements to be reported, and it is up to the discretion of the designated institutional official (DIO) whether other supporting information should be included. This leads to uncertainty and inconsistency for DIOs as they decide what to report.

Objective
We surveyed DIOs in an effort to provide national data on key performance indicators and other relevant components of the AIR process.

Methods
In July 2019, we conducted a national survey of 847 DIOs. The survey had 16 questions that explored basic institutional demographics, timelines, and processes for the AIR and key performance indicators. Written answers were grouped by similar responses, and we performed descriptive statistics on all variables to assess distributions of responses. We also explored associations between variables using cross-tabulation and chi-square statistics.

Results
A total of 267 DIOs responded to the survey (32% response rate). There were 7 institutional performance measures that achieved over 50% consensus. These reviews required the majority of DIOs (62%, 167 of 267) 5 to 20 hours to complete. Less than one-third of sponsoring institutions reported diversity data. The majority of DIOs (68%, 182 of 267) felt the AIR process added substantial value.

Conclusions
This survey reports key performance measures and processes included by DIOs in the AIR. Our results show a wide range of institutional responses though consensus was achieved on 7 key performance measures.
DO PERSONALITY TRAITS PREDICT BIASEDNESS WHILE MAKING INVESTMENT DECISIONS?
Authors: Yadav Ashutosh , Narayanan G. Badri 
Published: January 2021

The Investors’ rationality assumption of traditional finance theories has long been contested by behavioural finance over the past few decades. Various non-financial factors, responsible for shaping investors’ behaviour, including individual personality characteristics and the social environments surrounding the decisions to be made, have emerged in recent studies. With the advancement of behavioural finance, it is important to recuperate our understanding of how an individual’s personality make-up influences her susceptibility towards behavioural biases while making investment decisions. In this study, we explore the effect of the five personality traits on select behavioural biases (overconfidence, disposition and herding) in financial decision-making. A questionnaire comprising measures of personality traits, overconfidence and herding along with demographic variables was circulated to a representative sample (n=251) of Indian investors. Our findings suggest a significant impact of personality traits on the vulnerability of individuals while making investment decisions. Extrovert investors are more balanced, not overconfident, and do not follow the herd. Openness, extroversion, and agreeableness negatively impact the susceptibility of investors towards overconfidence and herding. The results can be used by financial advisors to develop personality specific financial tools to customise to the requirements of their clients.
JEL Classification Codes: D14, D90, D91, G11.