bluuebunny/crossref_metadata_2025_split huggingface dataset:
ANALISIS TEMPERATUR DAN UAP AIR BERBASIS SATELIT TERRA/AQUA (MODIS, LEVEL-2)
Authors: Sipayung Sinta Berliana , Krismianto . , Risyanto . 
Published: February 2018

Terra and Aqua satellites that consist of multiple sensors including MODIS instruments, which is operated to detect the phenomena that exist on land, sea and atmosphere. Not a lot of data extracted especially for Indonesia region the associated with atmospheric data, because the product is still in the raw data (level-0). For data extraction of level-0 to level-2 needed software IMAPP (International MODIS/airs Processing Package) so displays some data atmospheric parameters including MOD 04 - Aerosol, MOD 05 - Total precipitable Water (Water Vapor), MOD 06 - Cloud, MOD 07 - Atmospheric Profiles, MOD 08 - gridded Atmospheric and MOD 35 in HDF4 format (Hierarchical Data Format-4) swath. This paper discussed only MOD07/MYD07 atmospheric profiles level-2 related parameters such as the temperature of the atmosphere at an altitude of 780 hPa and water vapor at a height of 700 hPa. This study aimed to analyze the phenomena in the atmosphere, based on extraction method Atmospheric Profiles in the resolution 1km, that consists of temperature and moisture level-2, in the format hdf4 daily swath into data daily and monthly grid in .dat format, in the period of December 2014, January, July, and August 2015, especially in the area of Indonesia. The comparison between the results of the extraction swath and grid data from Terra/Aqua MODIS, that parameter atmospheric for the temperature has R-sqare an average of 0.72 and water vapor 0.74, while the RMSE temperature and water vapor are 0.88 and 0.29. Abstrak Satelit Terra dan Aqua yang terdiri dari beberapa sensor diantaranya instrumen MODIS, yang dioperasikan untuk mendeteksi fenomena yang ada di darat, laut, dan atmosfer. Belum banyak data yang diekstrak khususnya untuk wilayah Indonesia yang terkait dengan data atmosfer, karena produk MODIS masih berupa data mentah (level-0). Untuk ekstraksi data dari level-0 menjadi level-2 dibutuhkan software International MODIS/AIRS Processing Package (IMAPP) sehingga menampilkan beberapa data parameter atmosfer diantaranya MOD 04 - Aerosol, MOD 05 - Total Precipitable Water (Water Vapor), MOD 06 - Cloud, MOD 07 - Atmospheric Profiles, MOD 08 - Gridded Atmospheric dan MOD 35 swath dalam format Hierarchical Data Format-4 (HDF4). Pada makalah ini yang dibahas hanya MOD07/MYD07 atmospheric profiles level-2 yang berkaitan dengan parameter atmosfer seperti temperatur pada ketinggian 780 hPa dan uap air pada ketinggian 700 hPa. Penelitian ini bertujuan untuk menganalisis hasil ekstraksi data Atmospheric Profiles dari format HDF4 swath harian menjadi data grided harian, bulanan dalam format .dat serta aplikasinya pada periode bulan Desember 2014, Januari, Juli, dan Agustus 2015, khususnya wilayah Indonesia dalam resolusi 1km yang terdiri dari temperatur dan uap air level-2. Perbandingan antara hasil ekstraksi data MODIS swath dan data MODIS grided Terra/Aqua untuk parameter temperatur atmosfer mempunyai R-sqare rata-rata 0.72 dan uap air 0.74, sedangkan RMSE untuk temperatur dan uap air sebesar 0.88 dan 0.29.
Analisa Kualitas Delay Video on Demand Useetv Menggunakan Serat Optik Di Area Purwokerto
Authors: Purnomo Widhiatmoko Herry , Asrian Farida 
Published: February 2018

Video on Demand adalah salah satu layanan UseeTV IndiHome PT. Telekomunikasi Indonesia, Tbk berbasis IP (Internet Protocol). Video on Demand (VoD) merupakan salah satu fitur dari UseeTV yang memungkinkan pelanggan untuk dapat melakukan perekaman, penyimpanan dan penayangan kembali acara televise tertentu. Untuk mendapatkan kinerja yang baik maka layanan ini membutuhkan bandwidth yang cukup besar. Teknologi Gigabit-Capable Passive Optical Network (GPON) menjadi teknologi yang dapat mendukung layanan ini. Dalam layanan UseeTV, aktifitas jalur downstream menjadi perlakuan khusus, sehingga Quality of Service (QoS) dan kepadatan trafik perlu diperhatikan.Salah satu parameter yang berpengaruh terhadap layanan UseeTV adalah delay. Semakin kecil nilai delay maka akan semakin baik juga layanan UseeTV yang diterima oleh pelanggan.
Akurasi Penggalian Informasi Pada Data Rekam Medis ICD-10
Authors: Kurniawan Edy 
Published: February 2018

Banyaknya variabel dalam data rekam medis menyebabkan proses input data oleh tenaga administrasi sering mengalami keterlambatan. Akurasi data sangat diperlukan bagi berbagai pihak yang akan menggunakan data tersebut untuk mencari informasi yang terkandung didalamnya. Sering terjadi adanya data rusak diakibatkan tidak lengkapnya dalam proses input data. Jika data tersebut langsung dianalisa tanpa melewati proses pembersihan, maka akan menyebabkan informasi yang dianalisa tidak bisa dipertanggung jawabkan.Sebagai langkah untuk mengolah atau menggali informasi yang ada didalam tumpukan data rekam medis maka diperlukan pembersihan data dari noise. Hal ini dimaksudkan untuk menjaga keakuratan informasi yang nantinya dihasilkan. Penyelarasan struktur atribut dalam variabel data rekam medis dilakukan satu persatu. Sebab disetiap variabel tersebut mempunyai kode sendiri-sendiri yang tidak bisa dikerjakan secara bersama-sama. Untuk memudahkan dalam pembersihan data maka perlu dilakukan pembersihan variabel yang akan di proses saja, sedangkan variabel yang tidak diperlukan dihilangkan terlebih dahulu.Dari kumpulan data rekam medis yang akan di gali informasinya mempunyai cacat data yang cukup tinggi. Dari total data yang ada hampir 74% data mengalami kerusakan. Kerusakan ini dikarenakan proses inputan pertama yang tidak lengkap maupun adanya singkatan-singkatan, sehingga menyebabkan informasi tidak bisa dipertanggung jawabkan.
A Preliminary Exposé of Systemic Functional Theory Fundamentals
Authors: Dalamu Taofeek Olaiwola 
Published: February 2018

The study attempted to explain fundamentals of Systemic Functional Theory as textual analytical instruments. The basis was to demonstrate the applications of Ideational, Interpersonal and Textual Metafunctions as alternative semiotic resources that provide composite meaning potential to the structure of the clause. For illustration, six clauses in the advert of Premium Pension Limited were used as textual elements which the three metafunctions were applied. The study revealed conditionality, sensitizationality, judgmentality as well as integrity as the nuggets of the message. In addition, the ad tends to propound solutions to the financial security of the future of the people. The solution is for the recipients to negotiate and begin savings with Premium Pension Limited whose concern is how to care for the people in their old age. Above all, the study concluded that Halliday’s theory as a very practicable tool of textual analysis for researchers.
Challenges in measuring interprofessional–interorganisational collaboration with a questionnaire
Authors: Meijer Loes J , de Groot Esther , van Smeden Maarten , Schellevis François G , Damoiseaux Roger AMJ 
Published: February 2018

BackgroundCollaboration between medical professionals from separate organisations is necessary to deliver good patient care. This care is influenced by professionals’ perceptions about their collaboration. Until now, no instrument to measure such perceptions was available in the Netherlands. A questionnaire developed and validated in Spain was translated to assess perceptions about clinicians’ collaboration in primary and secondary care in the Dutch setting.AimValidation in the Dutch setting of a Spanish questionnaire that aimed to assess perceptions of clinicians about interorganisational collaboration.Design & settingAfter translation, cultural adaptation, and pre-testing, the questionnaire was sent to GPs and secondary care clinicians (SCCs) in three regions in the Netherlands. The responses of 445 responders were used to assess the validity and reliability of the questionnaire.MethodA confirmatory factor analysis (CFA) and an exploratory factor analysis (EFA) were performed to study the construct validity of the hypothesised factor model underlying the questionnaire. Test-retest reliability was evaluated using weighted Kappa statistics.ResultsResults of the CFA indicated poor fit of the hypothesised factor structure. EFA, executed separately for each region, showed a highly unstable factor structure. The test-retest reliability analysis demonstrated low re-test reliability.ConclusionThe underlying factor structure of a Spanish questionnaire could not be reproduced. The construct validity and reliability of this questionnaire were insufficient to warrant use in the Dutch setting. This study demonstrates the need for evaluating validity and reliability of questionnaires in local settings.
Magneto-optical Effects in the Scattering Polarization Wings of the Ca i 4227 Å Resonance Line
Authors: Alsina Ballester E. , Belluzzi L. , Trujillo Bueno J. 
Published: February 2018

Abstract
The linear polarization pattern produced by scattering processes in the Ca i 4227 Å resonance line is a valuable observable for probing the solar atmosphere. Via the Hanle effect, the very significant Q/I and U/I line-center signals are sensitive to the presence of magnetic fields in the lower chromosphere with strengths between 5 and 125 G, approximately. On the other hand, partial frequency redistribution (PRD) produces sizable signals in the wings of the Q/I profile, which have always been thought to be insensitive to the presence of magnetic fields. Interestingly, novel observations of this line revealed a surprising behavior: fully unexpected signals in the wings of the U/I profile and spatial variability in the wings of both Q/I and U/I. We show that the magneto-optical (MO) terms of the Stokes-vector transfer equation produce sizable signals in the wings of U/I and a clear sensitivity of the Q/I and U/I wings to the presence of photospheric magnetic fields with strengths similar to those that produce the Hanle effect in the line core. This radiative transfer investigation on the joint action of scattering processes and the Hanle and Zeeman effects in the Ca i 4227 Å line should facilitate the development of more reliable techniques for exploring the magnetism of stellar atmospheres. To this end, we can now exploit the circular polarization produced by the Zeeman effect, the magnetic sensitivity caused by the above-mentioned MO effects in the Q/I and U/I wings, and the Hanle effect in the line core.
The Effects of Barycentric and Asymmetric Transverse Velocities on Eclipse and Transit Times
Authors: Conroy Kyle E. , Prša Andrej , Horvat Martin , Stassun Keivan G. 
Published: February 2018

Abstract
It has long been recognized that the finite speed of light can affect the observed time of an event. For example, as a source moves radially toward or away from an observer, the path length and therefore the light travel time to the observer decreases or increases, causing the event to appear earlier or later than otherwise expected, respectively. This light travel time effect has been applied to transits and eclipses for a variety of purposes, including studies of eclipse timing variations and transit timing variations that reveal the presence of additional bodies in the system. Here we highlight another non-relativistic effect on eclipse or transit times arising from the finite speed of light—caused by an asymmetry in the transverse velocity of the two eclipsing objects, relative to the observer. This asymmetry can be due to a non-unity mass ratio or to the presence of external barycentric motion. Although usually constant, this barycentric and asymmetric transverse velocity (BATV) effect can vary between sequential eclipses if either the path length between the two objects or the barycentric transverse velocity varies in time. We discuss this BATV effect and estimate its magnitude for both time-dependent and time-independent cases. For the time-dependent cases, we consider binaries that experience a change in orbital inclination, eccentric systems with and without apsidal motion, and hierarchical triple systems. We also consider the time-independent case which, by affecting the primary and secondary eclipses differently, can influence the inferred system parameters, such as the orbital eccentricity.
Probing the Small-scale Structure in Strongly Lensed Systems via Transdimensional Inference
Authors: Daylan Tansu , Cyr-Racine Francis-Yan , Rivero Ana Diaz , Dvorkin Cora , Finkbeiner Douglas P. 
Published: February 2018

Abstract
Strong lensing is a sensitive probe of the small-scale density fluctuations in the Universe. We implement a pipeline to model strongly lensed systems using probabilistic cataloging, which is a transdimensional, hierarchical, and Bayesian framework to sample from a metamodel (union of models with different dimensionality) consistent with observed photon count maps. Probabilistic cataloging allows one to robustly characterize modeling covariances within and across lens models with different numbers of subhalos. Unlike traditional cataloging of subhalos, it does not require model subhalos to improve the goodness of fit above the detection threshold. Instead, it allows the exploitation of all information contained in the photon count maps—for instance, when constraining the subhalo mass function. We further show that, by not including these small subhalos in the lens model, fixed-dimensional inference methods can significantly mismodel the data. Using a simulated Hubble Space Telescope data set, we show that the subhalo mass function can be probed even when many subhalos in the sample catalogs are individually below the detection threshold and would be absent in a traditional catalog. The implemented software, Probabilistic Cataloger (PCAT) is made publicly available at https://github.com/tdaylan/pcat.
Metal-rich, Metal-poor: Updated Stellar Population Models for Old Stellar Systems
Authors: Conroy Charlie , Villaume Alexa , Dokkum Pieter G. van , Lind Karin 
Published: February 2018

Abstract
We present updated stellar population models appropriate for old ages (>1 Gyr) and covering a wide range in metallicities (−1.5 ≲ [Fe/H] ≲ 0.3). These models predict the full spectral variation associated with individual element abundance variation as a function of metallicity and age. The models span the optical–NIR wavelength range (0.37–2.4 μm), include a range of initial mass functions, and contain the flexibility to vary 18 individual elements including C, N, O, Mg, Si, Ca, Ti, and Fe. To test the fidelity of the models, we fit them to integrated light optical spectra of 41 Galactic globular clusters (GCs). The value of testing models against GCs is that their ages, metallicities, and detailed abundance patterns have been derived from the Hertzsprung–Russell diagram in combination with high-resolution spectroscopy of individual stars. We determine stellar population parameters from fits to all wavelengths simultaneously (“full spectrum fitting”), and demonstrate explicitly with mock tests that this approach produces smaller uncertainties at fixed signal-to-noise ratio than fitting a standard set of 14 line indices. Comparison of our integrated-light results to literature values reveals good agreement in metallicity, [Fe/H]. When restricting to GCs without prominent blue horizontal branch populations, we also find good agreement with literature values for ages, [Mg/Fe], [Si/Fe], and [Ti/Fe].
Molecular Cloud Structures and Massive Star Formation in N159
Authors: Nayak O. , Meixner M. , Fukui Y. , Tachihara K. , Onishi T. , Saigo K. , Tokuda K. , Harada R. 
Published: February 2018

Abstract
The N159 star-forming region is one of the most massive giant molecular clouds (GMCs) in the Large Magellanic Cloud (LMC). We show the 12CO, 13CO, CS molecular gas lines observed with ALMA in N159 west (N159W) and N159 east (N159E). We relate the structure of the gas clumps to the properties of 24 massive young stellar objects (YSOs) that include 10 newly identified YSOs based on our search. We use dendrogram analysis to identify properties of the molecular clumps, such as flux, mass, linewidth, size, and virial parameter. We relate the YSO properties to the molecular gas properties. We find that the CS gas clumps have a steeper size–linewidth relation than the 12CO or 13CO gas clumps. This larger slope could potentially occur if the CS gas is tracing shocks. The virial parameters of the 13CO gas clumps in N159W and N159E are low (<1). The threshold for massive star formation in N159W is 501 M
⊙ pc−2, and the threshold for massive star formation in N159E is 794 M
⊙ pc−2. We find that 13CO is more photodissociated in N159E than N159W. The most massive YSO in N159E has cleared out a molecular gas hole in its vicinity. All the massive YSO candidates in N159E have a more evolved spectral energy distribution type in comparison to the YSO candidates in N159W. These differences lead us to conclude that the giant molecular cloud complex in N159E is more evolved than the giant molecular cloud complex in N159W.
Dielectronic and Trielectronic Recombination Rate Coefficients of Be-like Ar14+
Authors: Huang Z. K. , Wen W. Q. , Xu X. , Mahmood S. , Wang S. X. , Wang H. B. , Dou L. J. , Khan N. , Badnell N. R. , Preval S. P. , Schippers S. , Xu T. H. , Yang Y. , Yao K. , Xu W. Q. , Chuai X. Y. , Zhu X. L. , Zhao D. M. , Mao L. J. , Ma X. M. , Li J. , Mao R. S. , Yuan Y. J. , Wu B. , Sheng L. N. , Yang J. C. , Xu H. S. , Zhu L. F. , Ma X. 
Published: February 2018

Abstract
Electron–ion recombination of Be-like 40Ar14+ has been measured by employing the electron–ion merged-beams method at the cooler storage ring CSRm. The measured absolute recombination rate coefficients for collision energies from 0 to 60 eV are presented, covering all dielectronic recombination (DR) resonances associated with 2s
2 → 2s2p core transitions. In addition, strong trielectronic recombination (TR) resonances associated with 2s
2 → 2p
2 core transitions were observed. Both DR and TR processes lead to series of peaks in the measured recombination spectrum, which have been identified by the Rydberg formula. Theoretical calculations of recombination rate coefficients were performed using the state-of-the-art multi-configuration Breit–Pauli atomic structure code AUTOSTRUCTURE to compare with the experimental results. The plasma rate coefficients for DR+TR of Ar14+ were deduced from the measured electron–ion recombination rate coefficients in the temperature range from 103 to 107 K, and compared with calculated data from the literature. The experimentally derived plasma rate coefficients are 60% larger and 30% lower than the previously recommended atomic data for the temperature ranges of photoionized plasmas and collisionally ionized plasmas, respectively. However, good agreement was found between experimental results and the calculations by Gu and Colgan et al. The plasma rate coefficients deduced from experiment and calculated by the current AUTOSTRUCTURE code show agreement that is better than 30% from 104 to 107 K. The present results constitute a set of benchmark data for use in astrophysical modeling.
Capture of Time-Loss Overuse Soccer Injuries in the National Collegiate Athletic Association's Injury Surveillance System, 2005–2006 Through 2007–2008
Authors: Roos Karen , Kucera Kristen L. , Golightly Yvonne , Myers Joseph B. , Rosamond Wayne , Marshall Stephen W. 
Published: February 2018

Context:
Overuse injuries are reported to account for nearly 50% of sports injuries and, due to their progressive nature and the uncertainty regarding date of onset, are difficult to define and categorize. Comparing the capture rates of overuse injuries between injury-surveillance systems and medical records can clarify completeness and determinants of how overuse injuries are represented in injury-surveillance data.

Objective:
To estimate the capture rate of time-loss medical-attention overuse injuries in men's and women's soccer in the National Collegiate Athletic Association Injury Surveillance System (NCAA ISS) compared with medical records maintained by certified athletic trainers and assess the differences in completeness of capture and factors contributing to those differences.

Design:
Capture-recapture study.

Setting:
Fifteen NCAA institutions provided NCAA ISS and medical record data from men's and women's soccer programs from 2005–2006 through 2007–2008.

Patients or Other Participants:
National Collegiate Athletic Association men's and women's soccer players.

Main Outcome Measure(s):
Time-loss medical-attention overuse injuries were defined as injuries with an overuse mechanism of injury in the NCAA ISS or medical records. Capture rates were calculated as the proportion of total overuse injuries classified as having overuse mechanisms in the NCAA ISS and the NCAA ISS and medical records combined.

Results:
The NCAA ISS captured 63.7% of the total estimated overuse mechanisms of injury in men's and women's soccer players. The estimated proportion of overuse injury mechanisms captured by both the NCAA ISS and medical records was 37.1%. The NCAA ISS captured more overuse injury mechanisms in men's soccer than in women's soccer (79.2% versus 45.0%, χ2 = 9.60; P = .002) athletes.

Conclusions:
From 2005–2006 through 2007–2008, the NCAA ISS captured only two thirds of time-loss medical-attention overuse mechanisms of injury in men's and women's soccer players. Future researchers should consider supplementing injury-surveillance data with a clinical record review to capture the burden of these injuries.
Naar zinvolle evaluatiemethoden voor community-projecten
Authors: Baerveldt Chris 
Published: February 2018

Abstract
The paper discusses the evaluation of two community-based intervention projects that were evaluated using a methodology that appears to differ strongly from traditional quasi-experimental designs. The main reason for this deviation is that traditional designs do not match the way community projects develop over time. Moreover, these designs do not provide enough information to improve these intervention projects in the future. It is argued that traditional designs can be partially tailored, but not sufficiently to address these needs. The evaluation methods that were actually used, also have drawbacks. It is argued that both the traditional and the here described evaluation methods do not provide enough information about what communities offer to children. Moreover, they do not account sufficiently for the democratic dynamics of community-based projects. A different direction is proposed, suggesting that not projects and interventions should be evaluated, but the children’s experience of (change of the) quality of the entire network of people and organizations in their community.
Leidende principes voor bestuurlijke innovatie: naar een robuust referentiekader
Authors: Hendriks Frank 
Published: February 2018

Leading principles for administrative innovation: towards a robust frame of reference
In administrative practice as well as in administrative science administrative innovation is a much desired good. In this article the author makes an attempt to describe the good, or the better, that can be pursued with administrative innovation, much sharper than has been done in the past. The result is a substantive framework for qualifying and evaluating administrative innovations. The article arises from a special interaction research, that started with a question from administrative practice (about the leading principles for administrative innovation in the Dutch municipality of Breda) and ended in a confrontation between desiderata from administrative practice on the one hand and foundations from administrative science on the other hand. Finally, these six leading principles emerged out of the investigation: responsiveness, productivity, involvement, counter-pressure, creativity, and good governance. The author also discusses how the resulting framework can be used and understood. The framework is robust because it not only is theoretically (the literature on governance and democratic innovation) inspired and founded, but also recognizable and manageable for administrative practice.