bluuebunny/crossref_metadata_2025_split huggingface dataset:
THE LEGACY OF THE WORKS OF YU.V. ROZHDESTVENSKY IN THE FORMATION OF THE FUNCTIONAL-SEMIOTIC SCIENTIFIC PARADIGM AND THE PLACE OF RHETORIC IN THE SYSTEM OF UNIVERSITY EDUCATION
Authors: Чижова Л.А. 
Published: August 2022

В статье рассматривается влияние идей Ю.В. Рождественского на формирование функционально-семиотической научной парадигмы в современной лингвистике, значимости преподавания курсов по общей филологии и риторике в системе университетского образования на филологическом факультете. Обращается внимание на необходимость формирования у учащихся понимания этических установок прецедентных текстов логосферы с целью избегнуть культурных конфликтов в обществе.
The article examines the influence of Yu.V. Rozhdestvensky's ideas on the formation of a functional-semiotic scientific paradigm in modern linguistics, the importance of teaching courses in general philology and rhetoric in the university education system at the Faculty of Philology, as well as the need, in order to preserve national culture, to form students' understanding of the ethical attitudes of precedent texts of the logosphere, in order to avoid cultural conflicts in society.
FUNCTIONAL TYPOLOGY OF SYNTAXEM AND INCOMPLETE SENTENCES IN RUSSIAN
Authors: Роговнева Ю.В. 
Published: August 2022

Настоящая статья представляет собой продолжение анализа предикативных единиц в нефикциональных описательных текстах. В более ранних работах были проанализированы конструкции, в которых говорящий не эксплицирует субъект; было показано, что эти предложения не всегда можно считать односоставными (в соответствии с оппозицией односоставности и двусоставности). В этой статье мы обратимся к проблеме так называемых неполных предложений и попытаемся взглянуть на эту закрепившуюся в русском синтаксисе оппозицию с точки зрения теории коммуникативной грамматики, в результате ответим на вопрос о том, какие предложения действительно можно считать неполными.
This article is a continuation of the analysis of predicative units in non-functional descriptive texts. In earlier works, constructions in which the speaker does not explicate the subject were analyzed, it was shown that these sentences cannot always be considered one-part (in accordance with the opposition of one-part and two-part). In this article we will address the problem of so-called incomplete sentences and try to look at this opposition fixed in Russian syntax from the point of view of the theory of communicative grammar.
Intonation of polar questions with indefinite pronouns produced by Italian learners of Russian
Authors: Дурягин П.В. 
Published: August 2022

Выбор просодического оформления высказывания на неродном языке является нетривиальной задачей для обучающихся, в особенности в тех случаях, когда предложение прагматически нагружено или содержит особые единицы, накладывающие ограничения на выбор тональной конфигурации. Одним из примеров такого типа фраз в русском языке являются общие вопросы, содержащие неопределенные местоимения. В статье представлены результаты экспериментального исследования произношения этого типа высказываний итальянцами, изучающими РКИ. В рамках эксперимента испытуемым предлагалось выбрать предпочитаемый порядок слов в коротких предложениях из трех слов и зачитать вслух с интонацией, соответствующей заданному контексту. Данные эксперимента позволили выделить основные стратегии, используемые италоговорящими для просодического оформления этого типа фраз в отсутствие эксплицитных инструкций. Большинство участников продемонстрировали склонность к трансферу на уровне просодии, но не при выборе порядка слов. Полученные результаты также демонстрируют необходимость учитывать эффект диалектных характеристик речи обучающихся при изучении закономерностей просодического трансфера.
The choice of prosodic structure for an utterance in a foreign language is a non-trivial task for learners, especially when the produced phrase is pragmatically loaded or contains the units that impose restrictions on the choice of tonal configuration. One example of such an utterance in Russian are polar questions with indefinite pronouns. The article presents the results of an experiment aimed to investigate the production of such phrases by Italian learners of Russian. The subjects were instructed to choose the word order in short polar questions and read them aloud with the intonation appropriate for the proposed context. The experimental data allowed to identify some common strategies used by Italian learners of Russian for prosodic marking in the lack of explicit instruction concerning this type of utterances. Most subjects demonstrated the tendency to transfer from their native language the prosody, but not the word order. In addition, the data highlight the necessity to consider dialectal differences when studying prosodic transfer phenomena.
GRANT ACTIVITY OF THE UNIVERSITY IN THE CONDITIONS OF A PANDEMIC: METHODOLOGICAL NOTES
Authors: Белгородский В.С. , Дембицкий С.Г. , Черкашина Т.Т. 
Published: August 2022

Настоящая статья посвящена анализу использования инструментов грантовой деятельности вуза для расширения образовательных, научно-методических, просветительских перспектив доступности и эффективности преподавания РКИ.
This article is devoted to the analysis of the use of the university grant activity tools to expand educational, scientific, methodological, educational prospects for the accessibility and effectiveness of teaching Russian as a foreign language.
RUSSIAN AS A FOREIGN LANGUAGE FOR ADVANCED NON-PHILOLOGISTS: IMMERSION METHOD
Authors: Саакян Л.Н. 
Published: August 2022

В статье анализируются методические основы метода погружения как рабочей среды для обучения РКИ в контексте межкультурной коммуникации. Рассматривается социокультурная составляющая современного и актуального языкового материала, на базе которого происходит формирование коммуникативной компетенции и умений и навыков межкультурной коммуникации учащихся, что должно быть положено в основу современных национально ориентированных средств обучения РКИ.
The article analyzes the methodological foundations of the immersion method as a working environment for teaching Russian as a foreign language in the context of intercultural communication. The article considers the socio-cultural component of modern and relevant language material, on the basis of which the formation of communicative competence and skills of intercultural communication of students takes place, which should be the basis of modern nationally-oriented means of teaching Russian as a foreign language.
CURRENT RAFL LEARNING MATERIALS FOR CHINESE MUSIC STUDENTS: A TEXT-CENTRIC APPROACH ("MUSIC THEORY")
Authors: Зацепин А.В. , Ли Ж. 
Published: August 2022

Разработанные учебные материалы представляют собой тексты и задания профессиональной направленности для китайских студентов-музыкантов и предназначены для обучения языку специальности. Учебный материал рассчитан на студентов, владеющих русским языком на уровне А2–B1+, и может быть использован как для аудиторных занятий, так и для самостоятельной работы. Основная задача дидактического ресурса – предоставить иностранным студентам дополнительный материал для чтения и накопить необходимый запас лексики для учебы по музыкальным специальностям, а также развить речевые навыки обучающихся. Разработанные тексты для чтения успешно прошли апробацию на занятиях с иностранными студентами музыкальных специальностей в РГПУ им. А.И. Герцена и в Даляньском университете иностранных языков в Китае.
The educational material is designed for students who speak Russian at the level A2-B1, and can be used both for classroom studies and for self-work. The main task of the didactic resource is providing to foreign students with additional reading material and accumulate the necessary vocabulary for studying in music specialties, as well as to develop students' speech skills. The developed texts for reading were successfully tested in the classroom with foreign students of musical specialties at the Herzen University and at the Dalian University of Foreign Studies in China. Due to many years of experience, the authors managed to take into account all the difficulties and specifics of teaching Russian as a foreign language.
Kajian Filsafat Ilmu dalam Pengembangan Ekonomi Moneter (Uang dan Bank)
Authors: Bhegawati Desak Ayu Sriary 
Published: August 2022

Filsafat dan ilmu mempunyai titik singgung dalam mencari kebenaran. Ilmu bertugas melukiskan dan filsafatbertugas menafsirkan fenomena semesta, kebenaran berada disepanjang pemikiran,sedangkan kebenaran ilmu berada disepanjang pengalaman.Berdasarkan uraian teroretis di atas, maka penulis akan membahas pengertianOntologi, Epistemologi dan Aksiologi serta segala permasalahannya sebagai unsuryang sangat penting dalam filsafat ilmu yang dipandang sebagai satu kesatuan yangtidak terpisahkan antara satu dengan yang lainnya.Keberadaan uang menyediakan alternatif transaksi yang lebih mudah daripada barter yang lebih kompleks, tidak efisien, dan kurang cocok digunakan dalam sistem ekonomi modern karena membutuhkan orang yang memiliki keinginan yang sama untuk melakukan pertukaran dan juga kesulitan dalam penentuan nilai. Efisiensi yang didapatkan dengan menggunakan uang pada akhirnya akan mendorong perdagangan dan pembagian tenaga kerja yang kemudian akan meningkatkan produktifitas dan kemakmuran.Penciptaan uang adalah proses memproduksi atau menghasilkan uang baru. Terdapat tiga cara untuk menciptakan uang, pertama dengan cara mencetak mata uang kertas atau uang logam, kedua melalui pengadaan utang dan pinjaman, serta ketiga melalui beragam kebijakan pemerintah, misalnya seperti pelonggaran kuantitatif. Bank merupakan lembaga keuangan yang sangat penting dalam perekonomian. Uang juga berfungsi sebagai satuan hitung (unit of account) karena uang dapat digunakan untuk menunjukan nilai berbagai macam barang/jasa yang diperjualbelikan, menunjukkan besarnya kekayaan, dan menghitung besar kecilnya pinjaman.Secara umum, bank didefinisikan sebagai lembaga keuangan yang usaha pokoknya adalah menghimpun dana dan menyalurkannya kepada masyarakat dalam bentuk kredit serta memberikan jasa dalam lalu lintas pembayaran dan peredaran uang.
PENGARUH STRES KERJA DAN KEPUASAN KERJA TERHADAP KINERJA PEGAWAI PADA BADAN PENGELOLAAN KEUANGAN DAN PENDAPATAN DAERAH KABUPATEN BULELENG
Authors: Astika Ida Ayu Kade 
Published: August 2022

Sumber daya manusia merupakan aset terpenting di dalam organisasi karena perannya yang membantu kelangsungan hidup organisasi. Sumber daya seperti modal, metode dan mesin tidak bisa memberikan hasil yang optimal apabila tidak didukung oleh sumber daya manusia yang mempunyai kinerja yang baik. Penelitian ini dilakukan dengan pendekatan kuisioner dengan sampel berjumlah 77 responden. Metode pengambilan sampel dengan menggunakan proporsional random sampling. Jenis penelitian yang digunakan adalah deskriptif kuantitatif dan kualitatif. Analisis statistik dan pengujian hipotesis menggunakan analisis korelasi berganda, analisis regresi liner berganda, koefisien determinasi, uji F dan uji t dengan menggunakan bantuan program Microsoft Excel dan program Statistical Product and Service Solution (SPSS) for windows Version 20,00. Berdasarkan simpulan maka dapat disarankan Pihak Badan Pengelolaan Keuangan dan Pendapatan Daerah Kabupaten Buleleng agar memperhatikan stres kerja dan kepuasan kerja karena kedua faktor tersebut berpengaruh terhadap kinerja. Badan Pengelolaan Keuangan dan Pendapatan Daerah Kabupaten Buleleng dapat melakukan program atau kegiatan yang dapat mengurangi stres kerja dan meningkatkan kepuasan kerja pegawai seperti family gathering ataupun memperhatikan hubungan interpersonal di antara pegawai. Untuk penelitian selanjutnya, disarankan agar lingkup penelitian diperluas dengan menambahkan beberapa variabel pendukung dan memilih lokasi penelitian di organisasi yang bergerak di bidang lain.
Observational Constraints on Cosmic-Ray Escape from Ultrahigh-energy Accelerators
Authors: Luce Quentin , Marafico Sullivan , Biteau Jonathan , Condorelli Antonio , Deligny Olivier 
Published: August 2022

Abstract
Interactions of ultra-high energy cosmic rays (UHECRs) accelerated in specific astrophysical environments have been shown to shape the energy production rate of nuclei differently from that of the secondary neutrons escaping from the confinement zone. Here, we aim at testing a generic scenario of in-source interactions through phenomenological modeling of the flux and composition of UHECRs. We fit a model in which nucleons and nuclei follow different particle energy distributions to the all-particle energy spectrum and proton spectrum below the ankle energy and distributions of maximum shower depths above this energy, as inferred at the Pierre Auger Observatory. We obtain that the data can be reproduced using a spatial distribution of sources that follows the density of extragalactic matter on both local and large scales, providing hence a realistic set of constraints for the emission mechanisms in cosmic accelerators, for their energetics, and for the abundances of elements at escape from their environments. While the quasi monoelemental increase of the cosmic-ray mass number observed on Earth from ≃2 EeV up to the highest energies calls for nuclei accelerated with a hard spectral index, the inferred flux of protons down to ≃0.6 EeV is shown to require for this population a spectral index significantly softer than that generally obtained up to now. We demonstrate that modeling UHECR data across the ankle substantiates the conjecture of in-source interactions in a robust statistical framework, although pushing the mechanism to the extreme.
Probing the Extent of Fe Kα Emission in Nearby Active Galactic Nuclei Using Multi-order Analysis of Chandra High Energy Transmission Grating Data
Authors: Masterson Megan , Reynolds Christopher S. 
Published: August 2022

Abstract
We present a study of the narrow Fe Kα line in seven bright, nearby active galactic nuclei (AGN) that have been observed extensively with the Chandra High Energy Transmission Grating (HETG). The HETG data reveal a wider Fe Kα line in the first-order spectrum than in the second- and third-order spectra, which we interpret as the result of spatially extended Fe Kα emission. We utilize these differences in narrow Fe Kα line widths in the multi-order Chandra HETG spectra to determine the spatial extent and intrinsic velocity width of the emitting material in each object. We find that there is modest evidence for spatially extended emission in each object, corresponding to extension of r ∼ 5–100 pc. These distances are significantly larger than those inferred from velocity widths assuming gravitational motions, which give r ∼ 0.01–1 pc. This implies either that the gas is emitting at a range of radii, with smaller radii dominating the velocity width and larger radii dominating the spatial extent, or that the gas is exhibiting nongravitational motions, which we suggest would be outflows due to slight excess redshift in the line and velocities that exceed the freefall velocity. We also use the spatial extent information to estimate the mass of the emitting gas by counting fluorescing iron atoms, finding masses on the order of M
gas ∼ 105–108
M
⊙. Future work with observatories like XRISM will be able to extend this study to a larger number of AGN and decrease uncertainties that arise as a result of the low signal-to-noise ratio of the higher-order HETG data.
Quiet Sun Center to Limb Variation of the Linear Polarization Observed by CLASP2 Across the Mg ii
h and k Lines
Authors: Rachmeler L. A. , Bueno J. Trujillo , McKenzie D. E. , Ishikawa R. , Auchère F. , Kobayashi K. , Kano R. , Okamoto T. J. , Bethge C. W. , Song D. , Ballester E. Alsina , Belluzzi L. , Pino Alemán T. del , Ramos A. Asensio , Yoshida M. , Shimizu T. , Winebarger A. , Kobelski A. R. , Vigil G. D. , Pontieu B. De , Narukage N. , Kubo M. , Sakao T. , Hara H. , Suematsu Y. , Štěpán J. , Carlsson M. , Leenaarts J. 
Published: August 2022

Abstract
The CLASP2 (Chromospheric LAyer Spectro-Polarimeter 2) sounding rocket mission was launched on 2019 April 11. CLASP2 measured the four Stokes parameters of the Mg ii
h and k spectral region around 2800 Å along a 200″ slit at three locations on the solar disk, achieving the first spatially and spectrally resolved observations of the solar polarization in this near-ultraviolet region. The focus of the work presented here is the center-to-limb variation of the linear polarization across these resonance lines, which is produced by the scattering of anisotropic radiation in the solar atmosphere. The linear polarization signals of the Mg ii
h and k lines are sensitive to the magnetic field from the low to the upper chromosphere through the Hanle and magneto-optical effects. We compare the observations to theoretical predictions from radiative transfer calculations in unmagnetized semiempirical models, arguing that magnetic fields and horizontal inhomogeneities are needed to explain the observed polarization signals and spatial variations. This comparison is an important step in both validating and refining our understanding of the physical origin of these polarization signatures, and also in paving the way toward future space telescopes for probing the magnetic fields of the solar upper atmosphere via ultraviolet spectropolarimetry.
Dark Matter Admixed Neutron Star Properties in the Light of X-Ray Pulse Profile Observations
Authors: Miao Zhiqiang , Zhu Yaofeng , Li Ang , Huang Feng 
Published: August 2022

Abstract
The distribution of the dark matter (DM) in DM-admixed neutron stars (DANSs) is supposed to result in either a dense dark core or an extended dark halo, subject to the DM fraction of the DANS (f

χ
) and the DM properties, such as the mass (m

χ
) and the strength of the self-interaction (y). In this paper, we perform an in-depth analysis of the formation criterion for dark cores/dark halos, and point out that the relative distribution of these two components is essentially determined by the ratio of the central enthalpy of the DM component to that of the baryonic matter component inside the DANSs. For the critical case where the radii of the DM and the baryonic matter are the same, we further derive an analytical formula to describe the dependence of

f

χ

crit

on m

χ
and y for a given DANS mass. The relative distribution of the two components in DANSs can lead to different observational effects. We here focus on the modification of the pulsar pulse profile, due to the extra light-bending effect in the case of a dark halo existence, and conduct the first investigation into the dark halo effects on the pulse profile. We find that the peak flux deviation is strongly dependent on the ratio of the halo mass to the radius of the DM component. Last, we perform Bayesian parameter estimation on the DM particle properties, based on the recent X-ray observations of PSR J0030+0451 and PSR J0740+6620 by the Neutron Star Interior Composition Explorer.
On the Impact of Relativistic Gravity on the Rate of Tidal Disruption Events
Authors: Coughlin Eric R. , Nixon C. J. 
Published: August 2022

Abstract
The tidal disruption of stars by supermassive black holes (SMBHs) probes relativistic gravity. In the coming decade, the number of observed tidal disruption events (TDEs) will grow by several orders of magnitude, allowing statistical inferences of the properties of the SMBH and stellar populations. Here we analyze the probability distribution functions of the pericenter distances of stars that encounter an SMBH in the Schwarzschild geometry, where the results are completely analytic, and the Kerr metric. From this analysis we calculate the number of observable TDEs, defined to be those that come within the tidal radius r
t but outside the direct capture radius (which is, in general, larger than the horizon radius). We find that relativistic effects result in a steep decline in the number of stars that have pericenter distances r
p ≲ 10 r
g, where r
g = GM/c
2, and that for maximally spinning SMBHs the distribution function of r
p at such distances scales as

f

r

p

∝

r

p

4

/

3

, or in terms of β ≡ r
t/r
p scales as f

β
∝ β
−10/3. We find that spin has little effect on the TDE fraction until the very-high-mass end, where instead of being identically zero the rate is small (≲1% of the expected rate in the absence of relativistic effects). Effectively independent of spin, if the progenitors of TDEs reflect the predominantly low-mass stellar population and thus have masses ≲1M
⊙, we expect a substantial reduction in the rate of TDEs above 107
M
⊙.
The Massive and Distant Clusters of WISE Survey. XI. Stellar Mass Fractions and Luminosity Functions of MaDCoWS Clusters at z ∼ 1
Authors: Decker Bandon , Brodwin Mark , Saha Ripon , Connor Thomas , Eisenhardt Peter R. M. , Gonzalez Anthony H. , Moravec Emily , Muhibullah Mustafa , Stanford S. Adam , Stern Daniel , Thongkham Khunanon , Wylezalek Dominika , Dicker Simon R. , Mason Brian , Mroczkowski Tony , Romero Charles E. , Ruppin Florian 
Published: August 2022

Abstract
We present stellar mass fractions and composite luminosity functions (LFs) for a sample of 12 clusters from the Massive and Distant Clusters of WISE Survey (MaDCoWS) in the redshift range 0.951 ≤ z ≤ 1.43. Using spectral energy distribution fitting of optical and deep mid-infrared photometry, we establish the membership of objects along the lines of sight to these clusters and calculate the stellar masses of member galaxies. This allows us to calculate the stellar mass of the clusters much more precisely than in previous works. We find stellar mass fractions for these clusters largely consistent with previous works, and an apparent negative correlation with total cluster mass. We measure a composite 3.6 μm LF down to m* + 2.5 for all 12 clusters. Fitting a Schechter function to the LF, we find a characteristic 3.6 μm magnitude of m* = 19.83 ± 0.12 and faint-end slope of α = −0.81 ± 0.10 for the full sample at a mean redshift of

z

¯

=
1.18

. We also divide the clusters into high- and low-redshift bins at

z

¯

=
1.29

and

z

¯

=
1.06

, respectively, and measure a composite LF for each bin. We see a small, but statistically significant, evolution in m* and α—consistent with passive evolution—when we study the joint fit to the two parameters, which is probing the evolution of faint cluster galaxies at z ∼ 1. This highlights the importance of deep IR data in studying the evolution of cluster galaxy populations at high redshift.
Widespread Detection of Two Components in the Hot Circumgalactic Medium of the Milky Way
Authors: Bluem Jesse , Kaaret Philip , Kuntz K. D. , Jahoda Keith M. , Koutroumpa Dimitra , Hodges-Kluck Edmund J. , Fuller Chase A. , LaRocca Daniel M. , Zajczyk Anna 
Published: August 2022

Abstract
Surrounding the Milky Way (MW) is the circumgalactic medium (CGM), an extended reservoir of hot gas that has significant implications for the evolution of the MW. We used the HaloSat all-sky survey to study the CGM’s soft X-ray emission in order to better define its distribution and structure. We extend a previous HaloSat study of the southern CGM (Galactic latitude b < −30°) to include the northern CGM (b > 30°) and find evidence that at least two hot gas model components at different temperatures are required to produce the observed emission. The cooler component has a typical temperature of kT ∼0.18 keV, while the hotter component has a typical temperature of kT ∼0.7 keV. The emission measure in both the warm and hot components has a wide range (∼0.005–0.03, and ∼0.0005–0.004 cm−6 pc, respectively), indicating that the CGM is clumpy. A patch of relatively consistent CGM was found in the north, allowing for the CGM spectrum to be studied in finer detail using a stacked spectrum. The stacked spectrum is well described with a model including two hot gas components at temperatures of kT = 0.166 ± 0.005 keV and kT =

0.69

−
0.05

+
0.04

keV. As an alternative to adding a hot component, a neon-enhanced single-temperature model of the CGM was also tested and found to have worse fit statistics and poor residuals.