bluuebunny/crossref_metadata_2025_split huggingface dataset:
Лагунные берега Тихоокеанской России: факторы эволюции и природопользование
Authors: Brovko P.F. , Dzen G.N. , Zhukovina M.G. , Malyugin A.V. 
Published: April 2020

Прибрежная зона восточно-арктических и дальневосточных морей Тихоокеанской России имеет широкий спектр морфогенетических типов берегов. Наиболее полно среди них представлены лагунные берега. Эволюция лагун связана с повышением уровня Мирового океана. На этом фоне отмечено увеличение штормовой активности, что приводит к существенному преобразованию рельефа: формированию новых проливов и островов, преобразованию дельт. Существенно проявление географической зональности в динамике берегов. Показано, что в Охотском море ледовый фактор играет важную роль в морфологии и динамике лагун, а природные условия формирования побережий позволяют считать их субарктическими. Прибрежно-морское природопользование носит разносторонний характер: добыча рыбы, водорослей и беспозвоночных гидротехническое строительство разработка прибрежно-морских россыпей тяжелых металлов освоение бальнеологических ресурсов. Широко развиты марикультура и экологический туризм. Лагунные берега формируются иногда в условиях активного техногенного воздействия.The coastal zone of the East Arctic and Far-Eastern seas of Pacific Russia has a wide range of the morphogenetic types of the shores. The lagoon shores are most fully presented among them. The lagoons evolution is caused by the world ocean level increase. An increase in storm activity leads to a significant transformation of the terrain. New straits and islands are formed and the deltas are transformed. The manifestation of the geographic zonality in the dynamics of shores is essential. It is shown that the ice factor plays an important role in the morphology and dynamics of lagoons in the Sea of Okhotsk. The natural conditions for the formation of coasts make it possible to consider them as subarctic. The coastal-marine management is of versatile nature: catch of fish, algae and invertebrates hydrotechnical construction mining of seashore placers of the heavy metals development of balneal resources. The mariculture and eco-tourism are well represented. Sometimes the lagoon shores are formed under conditions of active technogenic impact.
Академик Виктор Борисович Сочава как исследователь Дальнего Востока
Authors: Snytko V.A. 
Published: April 2020

Рассмотрен вклад Виктора Борисовича Сочавы (19051978) в познание природы Дальнего Востока. Его исследования региона были начаты в конце 1920-х гг. и продолжались десятилетиями. Им был решен ряд проблем ботаники и физической географии, предложено районирование территории.The contribution of Viktor Borisovich Sochava (1905-1978) to the knowledge of the Far East nature was considered. His investigations of the region were begun in the late 1920s and continued over the course of decades. He has solved a number of problems of botany and physical geography and proposed the zonation of territory.
CRITÉRIOS DIAGNÓSTICOS PARA EJACULAÇÃO PRECOCE
Authors: Finotelli Jr. Itor 
Published: April 2020

As pesquisas sobre a ejaculação precoce (EP) são dificultadas pela falta de consenso sobre quais critérios a definem como uma disfunção. Observa-se que a mesma dificuldade é encontrada para sua nomenclatura e também que critérios comuns, mas com diferenças substanciais, são propostos pelos sistemas de classificação de doenças. Nesse sentido, este estudo identificou e comparou os critérios utilizados nas pesquisas publicadas em artigos, nas bases de dados Science Citation Index, MEDLINE, PsycInfo, LILACS, SciELO, CLASE. As buscas partiram de palavras-chaves e o período de revisão foi de 2000 a 2013. Os resultados apresentaram um número expressivo de artigos, mas foram considerados aqueles cuja investigação fosse primária utilizando metodologia científica. Observaram-se quatro critérios principais utilizados que apresentaram diferenças significativas nessa avaliação. O primeiro trata-se do tempoejaculatório, caracterizado como uma mensuração objetiva e útil para triagens, porém sem consenso sobre sua estimativa. O segundo, o senso de controle, apresentou resultados expressivos, todavia caracterizado como uma medida subjetiva. Pesquisas relacionadas a ele demonstraram que homens sem EP relataram um controle bastante elevado sobre a ejaculação em comparação a homens com tempos curtos de latência ejaculatória. Os dois últimos critérios foram a satisfação sexual e o sofrimento, não sendo específico da EP e presentes em todas as disfunções sexuais. Para ambos, a insatisfação foi relatada na existência de uma EP, geralmente, acompanhada de incômodo e dificuldades interpessoais. Os dados apresentados organizaram de maneira sistemática os critérios utilizados na avaliação da EP, uma compilação útil para diferentes frentes de pesquisa.
Penerapan Pendekatan Saintifik Dengan Bantuan LKS-Induktif Dalam Pembelajaran Faktor-faktor Yang Mempengaruhi Laju Reaksi Pada Siswa Kelas XI SMAN-5 Palangka Raya Tahun Ajaran 2015/2016
Authors: Nopriani Christina , Abudarin  , Damsyik Akhmad 
Published: April 2020

Penelitian ini bertujuan untuk: (1) mendeskripsikan kemampuan belajar siswa kelas XI SMA Negeri 5 Palangka Raya tahun pelajaran 2015/2016 yang meliputi kemampuan mengamati, menanya, mengumpulkan data, mengasosiasi dan mengomunikasikan dengan bantuan LKS-Induktif; (2) mendeskripsikan pemahaman konsep siswa kelas XI SMA Negeri 5 Palangka Raya tahun pelajaran 2015/2016 tentang faktor-faktor yang mempengaruhi laju reaksi pasca pembelajaran menggunakan pendekatan saintifik dengan bantuan LKS-Induktif.Penelitian ini melibatkan siswa kelas XI Peminatan MIPA SMA Negeri 5 Palangka Raya sebanyak 57 siswa. Instrumen yang digunakan adalah lembar soal pretes dan postes, LKS-Induktif dengan pendekatan saintifik, dan pedoman wawancara. Data dikumpulkan melalui tiga tahap, yaitu pretes, pelaksanaan pembelajaran dengan pendekatan saintifik berbantuan LKS-Induktif, dan postes. Setelah menganalisis pemahaman konsep siswa pada tiap indikator, maka untuk memperkuat hasil pendeskripsian pemahaman konsep dan kemampuan belajar, dilakukan wawancara terhadap beberapa perwakilan siswa.Hasil penelitian menunjukkan bahwa dengan menggunakan LKS-Induktif, kemampuan belajar siswa dalam pembelajaran dengan pendekatan saintifik rata-rata sebesar 83,14%. Secara rinci kemampuan belajar siswa adalah sebagai berikut: (a) kemampuan mengamati sebesar 84,19%; (b) kemampuan menanya sebesar 48,17%; (c) kemampuan mengumpulkan informasi sebesar 89,39%; (d) kemampuan mengasosiasi sebesar 96,09%; dan (e) kemampuan mengomunikasikan sebesar 87,25%. Kemampuan siswa memahami konsep tentang faktor-faktor yang mempengaruhi laju reaksi dalam pembelajaran dengan pendekatan saintifik menggunakan LKS-Induktif rata-rata sebesar 85,09% dengan kategori sangat baik. Proporsi jumlah siswa yang dapat memahami dengan benar pada setiap konsep adalah: (a) sebanyak 100% siswa dapat menjelaskan pengaruh konsentrasi dengan laju reaksi; (b) sebanyak 92,99% siswa dapat menjelaskan pengaruh konsentrasi terhadap laju reaksi berdasarkan teori tumbukan; (c) sebanyak 100% siswa dapat menjelaskan pengaruh luas permukaan terhadap laju reaksi; (d) sebanyak 57,90% siswa dapat menjelaskan pengaruh luas permukaan terhadap laju reaksi berdasarkan teori tumbukan; (e) sebanyak 100% siswa dapat menjelaskan pengaruh suhu terhadap laju reaksi; (f) sebanyak 73,68% siswa dapat menjelaskan pengaruh suhu terhadap laju reaksi berdasarkan teori tumbukan; (g) sebanyak 100% siswa dapat menjelaskan pengaruh katalis terhadap laju reaksi; dan (h) sebanyak 56,14% siswa dapat menjelaskan pengaruh katalis terhadap laju reaksi dan hubungannya dengan energi aktivasi (Ea).
PELAKSANAAN PENINGKATAN KEPATUHAN PELAPORAN LAPORAN HARTA KEKAYAAN PENYELENGGARA NEGARA (LHKPN)
Authors: Ingnuan Yuniarty Veronika , Lutfi Mohamad 
Published: April 2020

This study aims to test and analyze the Implementation of Enhancing the Compliance of Reporting the Statutory Assets of State Assets (LHKPN) in the Scope of Regional Agencies at the Directorate of Registration and Examination of LHKPN. In this study the authors used a Qualitative Descriptive Data analysis method using the Interative Analysis model. The author uses the Triangulation technique to test the validity of the data that has been obtained during the study. Purposive Sampling Method is a sample determination technique with certain considerations. The results of the research prove that the level of LHKPN Reporting Compliance in the Scope of Regional Agencies has decreased from 2016-2017. This percentage can still increase if it is supported by the role and awareness of the Obligatory Report to report their assets and the commitment of the Regional Head / Head of Institution related to the application of sanctions for compulsory reporting who do not report LHKPN to the KPK. The next level of LHKPN Reporting Compliance in the Bangka Belitung Islands Provincial Government in 2017 has increased. Because since the beginning the Governor of the Bangka Belitung Islands Provincial Government has committed in the framework of preventing corruption, one of them is by reporting the LHKPN and issuing the Bangka Belitung Islands Governor Regulation No. 56 of 2017 concerning Management of State Organizer Asset Management in the Province of Bangka Belitung Provincial Government and issuing Circular Number : 840/0098 / VII / 2018 dated April 3, 2018 concerning the delay in payment of the Income Improvement Allowance (TPP).
Mekanisme Menumbuh Kembangkan Minat Baca Siswa Madrasah di Perpustakaan
Authors: Sahrandi Akhmad 
Published: April 2020

Perpustakaan merupakan sumber informasi dan ilmu pengetahuan. Mengingat begitu pentingnya keberadaan perpustakaan, maka perlulah kiranya adanya sarana perpustakaan di semua jenis dan jenjang pendidikan. Kemudian agar tujuan didirikanya perpustakaan sekolahan yang antara lain adalah agar tumbuh kecintaan terhadap membaca serta menanamkan minat dan kegemaran membaca, maka peyelenggaraan (pengelolaan) perpustakaan harus dilakukan secara sistematis dan profesional sesuai dengan pedoman penyelengganaan yang berlaku. Dalam upaya untuk meningkatkan mutu pendidikan di negara kita ini, maka penyelenggaraan (pengelolaan) perpustakaan harus dilakukan secara sistematis dan sesuai dengan pedoman penyelenggaraan yang berlaku, agar sesuai dengan tujuan didirikannya perpustakaan itu sendiri, antara lain agar tumbuh (timbul) kecintaan terhadap membaca, memupuk dan menanamkan kebiasaan membaca sehingga tumbuh kecintaan terhadap buku.
Kemampuan membaca yang dimiliki oleh seseorang merupakan modal utama dalam proses belajar mengajar. Dengan kata lain kemampuan membaca merupakan prasyarat utama dan merupakan kebutuhan pokok bagi seseorang untuk mencapai keberhasilan. Karena dengan membaca seseorang dapat dengan mudah untuk mengkaji berbagai ilmu pengetahuan. Aktifitas membaca ini dipengaruhi oleh beberapa faktor yang dapat mendorong terwujudnya kegiatan tersebut. Adapun salah satu faktor yang mempengaruhi kegiatan membaca adalah minat. Minat mempunyai peran sangat penting dan menempati posisi vital dalam aktifitas membaca (belajar) mahasiswa, karena minat mempunyai daya dorong yang kuat terhadap terwujudnya suatu aktifitas
NARCISISMO, O CONCEITO DE FLYING MONKEYS E O COMPORTAMENTO SOCIAL
Authors: César Dias Lopes Gabriel 
Published: April 2020

O artigo em questão aborda o Transtorno de Personalidade Narcisista (TPN), enquanto patologia catalogada enquanto doença ental no DSM IV, enfocando principalmente os flying monkeys (macacos voadores), que apesar de não serem formalmente econhecidos na medicina psiquiátrica, tem uma incidência muito grande na sociedade e com um alcance de ação negativa ncalculável. Justamente por não ter esse reconhecimento, o estudo acerca de sua ação é restrito a artigos de opinião ou a chamada sicologia popular. Diante disso busca-se aqui através de uma pesquisa bibliográfica e descritiva enriquecer a literatura acerca da emática, buscando identificar e avaliar a ação e o comportamento dos flying monkeys na sociedade.
Quasiperiodic Velocity Fluctuations in Eruptive Prominences Observed by AIA/SDO
Authors: Tsvetkov Tsvetan , Petrov Nikola 
Published: April 2020

Abstract
The current study presents an investigation of the behavior of prominences during eruptions. Variations in the distribution of their velocities are detected at altitudes <0.6 R
⊙. Detailed analyses are carried out for 304 Å Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observations. To track the behavior of prominences during eruptions, 41 events in the period 2010–2017 are studied. To follow the rise of a filament on higher altitudes (up to 32 R
⊙), Solar and Heliospheric Observatory/Large Angle and Spectrometric Coronagraph (SOHO/LASCO) data are also inspected. They are used to obtain kinematic profiles of eruptions. Obtained height–time and speed–time plots of the eruptions show velocity fluctuations in 83% of the explored cases, detected only in the SDO/AIA field of view, and not in any of the prominences observed at higher altitudes by SOHO/LASCO. Time intervals between fluctuations and heights at which they are detected are estimated. Strong periodicity cannot be determined.
Fluorine in the Solar Neighborhood: The Need for Several Cosmic Sources
Authors: Ryde Nils , Jönsson Henrik , Mace Gregory , Cunha Katia , Spitoni Emanuele , Afşar Melike , Jaffe Daniel , Forsberg Rebecca , Kaplan Kyle F. , Kidder Benjamin T. , Lee Jae-Joon , Oh Heeyoung , Smith Verne V. , Sneden Christopher , Sokal Kimberly R. , Strickland Emily , Thorsbro Brian 
Published: April 2020

Abstract
The cosmic origin of fluorine is still not well constrained. Several nucleosynthetic channels at different phases of stellar evolution have been suggested, but these must be constrained by observations. For this, the fluorine abundance trend with metallicity spanning a wide range is required. Our aim is to determine stellar abundances of fluorine for

. We determine the abundances from HF lines in infrared K-band spectra (

) of cool giants, observed with the IGRINS and Phoenix high-resolution spectrographs. We derive accurate stellar parameters for all our observed K giants, which is important as the HF lines are very temperature-sensitive. We find that [F/Fe] is flat as a function of metallicity at [F/Fe]∼0, but increases as the metallicity increases. The fluorine slope shows a clear secondary behavior in this metallicity range. We also find that the [F/Ce] ratio is relatively flat for

, and that for two metal-poor (

), s-process element-enhanced giants, we do not detect an elevated fluorine abundance. We interpret all of these observational constraints as indications that several major processes are at play for the cosmic budget of fluorine over time: from those in massive stars at low metallicities, through the asymptotic giant branch star contribution at

, to processes with increasing yields with metallicity at supersolar metallicities. The origins of the latter, and whether or not Wolf–Rayet stars and/or novae could contribute at supersolar metallicities, is currently not known. To quantify these observational results, theoretical modeling is required. More observations in the metal-poor region are required to clarify the processes there.
Reinflation of Warm and Hot Jupiters
Authors: Komacek Thaddeus D. , Thorngren Daniel P. , Lopez Eric D. , Ginzburg Sivan 
Published: April 2020

Abstract
Understanding the anomalous radii of many transiting hot gas-giant planets is a fundamental problem of planetary science. Recent detections of reinflated warm Jupiters orbiting post-main-sequence stars and the reinflation of hot Jupiters while their host stars evolve on the main sequence may help constrain models for the anomalous radii of hot Jupiters. In this work, we present evolution models studying the reinflation of gas giants to determine how varying the depth and intensity of deposited heating affects both main-sequence reinflation of hot Jupiters and post-main-sequence reinflation of warm Jupiters. We find that deeper heating is required to reinflate hot Jupiters than is needed to suppress their cooling, and that the timescale of reinflation decreases with increasing heating rate and depth. We find a strong degeneracy between heating rate and depth, with either strong shallow heating or weak deep heating providing an explanation for main-sequence reinflation of hot Jupiters. This degeneracy between heating rate and depth can be broken in the case of post-main-sequence reinflation of warm Jupiters, as the inflation must be rapid to occur within post-main-sequence evolution timescales. We also show that the dependence of heating rate on the incident stellar flux inferred from the sample of hot Jupiters can explain reinflation of both warm and hot Jupiters. TESS will obtain a large sample of warm Jupiters orbiting post-main-sequence stars, which will help to constrain the mechanism(s) causing the anomalous radii of gas-giant planets.
Plasma Diagnostics from Active Region and Quiet-Sun Spectra Observed by Hinode/EIS: Quantifying the Departures from a Maxwellian Distribution
Authors: Lörinčík Juraj , Dudík Jaroslav , del Zanna Giulio , Dzifčáková Elena , Mason Helen E. 
Published: April 2020

Abstract
We perform plasma diagnostics, including that of the non-Maxwellian κ-distributions, in several structures observed in the solar corona by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on board the Hinode spacecraft. To prevent uncertainties due to the in-flight calibration of EIS, we selected spectral atlases observed shortly after the launch of the mission. One spectral atlas contains an observation of an active region, while the other is an off-limb quiet-Sun region. To minimize the uncertainties of the diagnostics, we rely only on strong lines and average the signal over a spatial area within selected structures. Multiple plasma parameters are diagnosed, such as the electron density, the differential emission measure, and the non-Maxwellian parameter κ. To do that, we use a simple, well-converging iterative scheme based on refining the initial density estimates via the differential emission measure (DEM) and κ. We find that while the quiet-Sun spectra are consistent with a Maxwellian distribution, the coronal loops and moss observed within the active region are strongly non-Maxwellian with κ ⪅ 3. These results were checked by calculating synthetic ratios using DEMs obtained as a function of κ. Ratios predicted using the DEMs assuming κ-distributions converged to the ratios observed in the quiet Sun and coronal loops. To our knowledge, this work presents a strong evidence of the presence of different electron distributions between two physically distinct parts of the solar corona.
A Binary Comb Model for Periodic Fast Radio Bursts
Authors: Ioka Kunihito , Zhang Bing 
Published: April 2020

Abstract
We show that the periodic FRB 180916.J0158+65 can be interpreted by invoking an interacting neutron star binary system with an orbital period of ∼16 days. The FRBs are produced by a highly magnetized pulsar, whose magnetic field is “combed” by the strong wind from a companion star, either a massive star or a millisecond pulsar. The FRB pulsar wind retains a clear funnel in the companion’s wind that is otherwise opaque to induced Compton or Raman scatterings for repeating FRB emission. The 4 day active window corresponds to the time when the funnel points toward Earth. The interaction also perturbs the magnetosphere of the FRB pulsar and may trigger emission of FRBs. We derive the physical constraints on the comb and the FRB pulsar from the observations and estimate the event rate of FRBs. In this scenario, a lower limit on the period of observable FRBs is predicted. We speculate that both the intrinsic factors (strong magnetic field and young age) and the extrinsic factor (interaction) may be needed to generate FRBs in neutron star binary systems.
In Situ Measurement of Curvature of Magnetic Field in Turbulent Space Plasmas: A Statistical Study
Authors: Bandyopadhyay Riddhi , Yang Yan , Matthaeus William H. , Chasapis Alexandros , Parashar Tulasi N. , Russell Christopher T. , Strangeway Robert J. , Torbert Roy B. , Giles Barbara L. , Gershman Daniel J. , Pollock Craig J. , Moore Thomas E. , Burch James L. 
Published: April 2020

Abstract
Using in situ data, accumulated in the turbulent magnetosheath by the Magnetospheric Multiscale Mission, we report a statistical study of magnetic field curvature and discuss its role in the turbulent space plasmas. Consistent with previous simulation results, the probability distribution function of the curvature is shown to have distinct power-law tails for both high and low value limits. We find that the magnetic-field-line curvature is intermittently distributed in space. High curvature values reside near weak magnetic-field regions, while low curvature values are correlated with small magnitude of the force acting normal to the field lines. A simple statistical treatment provides an explanation for the observed curvature distribution. This novel statistical characterization of magnetic curvature in space plasma provides a starting point for assessing, in a turbulence context, the applicability and impact of particle energization processes, such as curvature drift, that rely on this fundamental quantity.
EAGLE and Illustris-TNG Predictions for Resolved eROSITA X-Ray Observations of the Circumgalactic Medium around Normal Galaxies
Authors: Oppenheimer Benjamin D. , Bogdán Ákos , Crain Robert A. , ZuHone John A. , Forman William R. , Schaye Joop , Wijers Nastasha A. , Davies Jonathan J. , Jones Christine , Kraft Ralph P. , Ghirardini Vittorio 
Published: April 2020

Abstract
We simulate stacked observations of nearby hot X-ray coronae associated with galaxies in the EAGLE and Illustris-TNG hydrodynamic simulations. A forward modeling pipeline is developed to predict 4 yr eROSITA observations and stacked image analysis, including the effects of instrumental and astrophysical backgrounds. We propose an experiment to stack z ≈ 0.01 galaxies separated by specific star formation rate (sSFR) to examine how the hot (T ≥ 106 K) circumgalactic medium (CGM) differs for high- and low-sSFR galaxies. The simulations indicate that the hot CGM of low-mass (

), high-sSFR (defined as the top one-third ranked by sSFR) central galaxies will be detectable to a galactocentric radius r ≈ 30–50 kpc. Both simulations predict lower luminosities at fixed stellar mass for the low-sSFR galaxies (the lower third of sSFR) with Illustris-TNG predicting 3× brighter coronae around high-sSFR galaxies than EAGLE. Both simulations predict detectable emission out to r ≈ 150–200 kpc for stacks centered on high-mass (

) galaxies, with EAGLE predicting brighter X-ray halos. The extended soft X-ray luminosity correlates strongly and positively with the mass of circumgalactic gas within the virial radius (f
CGM). Prior analyses of both simulations have established that f
CGM is reduced by expulsive feedback driven mainly by black hole growth, which quenches galaxy growth by inhibiting replenishment of the interstellar medium. Both simulations predict that eROSITA stacks should not only conclusively detect and resolve the hot CGM around L* galaxies for the first time, but provide a powerful probe of how the baryon cycle operates, for which there remains an absence of consensus between state-of-the-art simulations.