bluuebunny/crossref_metadata_2025_split huggingface dataset:
إسهامات علي بن رضوان الفلسفية والمنطقية في تطور الحضارة العربية الإسلامية (ت: 453هـ/1061م)
Authors: الأستاذ الدكتورعلي عبد مشالي العكيلي  , الباحثة دعاء محمد كريم التميمي  
Published: January 2025

الخلاصة:
تهدف هذه الدراسة إلى تسليط الضوء على إسهامات علي بن رضوان الفلسفية والمنطقية التي تُعد من العلوم المهمة التي حظيت باهتمام الإنسان منذ القدم، فوجود الإنسان يمكن أن يحصر بنظرية فلسفة الخلق، فالفلسفة موجودة عند كل فرد، ولكن على درجات متفاوتة، كما تختلف موضوعاتها في المجتمعات، وقد أدرك الإنسان أهمية العلوم الحكمية منذ القدم، ومنهم عالمنا المسلم علي بن رضوان (ت: 453هـ/1061م). وقد أشرنا إلى بداية العلوم الفلسفية، وأين نشأت وطرق انتقالها، وما واجهتهُ من صعوبات وانتقادات، فضلاً عن مدى تعقيد وصعوبة فهم هذه العلوم، وهذا دليل على نباهة ابن رضوان الذي قرأ الكتب الفلسفية والمنطقية، لاسيما اليونانية بوجه خاص، إذ عاش في ظل الدولة الفاطمية الذي شجعت العلم والمعرفة. استفاد ابن رضوان من المؤسسات الثقافية، لاسيما المساجد والمكاتب الذي أنشأها الفاطميون، كما تميز ابن رضوان باستعداد فكري وتأني في طرح الأفكار، فكانت لهُ مساجلات فلسفية ومنطقية لا تخلو من المتعة والفائدة، فضلاً عن تميزهُ بمنهجية متزنة معتمداً بذلك على سعة خبرته ومعارفه الذي اكتسبها من خلال اطلاعه على المؤلفات العقلية بوجه عام، تاركاً مؤلفات غايةً في الأهمية، لاسيما في العلوم الحكمية، فضلاً عن مؤلفاته الطبية والفلكية.
Indonesian Society of Respirology Position Paper on Lung Cancer Control in Indonesia
Authors: Andarini Sita , Santoso Andintia Aisyah , Arfiansyah Mochammad Aris , Syahruddin Elisna , Zaini Jamal , Putra Andika Chandra , Kurniawan Ferry Dwi , Ermayanti Sabrina , Soeroso Noni Novisari , Munir Sri Melati , Infianto Andreas , Setijadi Ana Rima , Setyawan Ungky Agus , Wulandari Laksmi , Haryati Haryati , Jasminarti Ida Ayu , Hidayat Moulid , Santoso Arif 
Published: January 2025

Lung cancer is a major health concern in Indonesia due to its increasing prevalence, late-stage diagnosis, younger population, and high mortality. Addressing this issue requires nationwide implementation of comprehensive lung cancer control, which includes risk reduction and prevention strategies, focusing on tobacco control and air pollution mitigation. Screening with low-dose computed tomography (LDCT) and early detection in symptomatic patients, along with TB screening programs and all non-communicable diseases, is strongly recommended to enhance early case findings, treatment effectiveness, and overall patient outcomes. A multidisciplinary team (MDT) approach is important to ensure accurate diagnosis and comprehensive care. Moreover, the integration of palliative care at the early stages of advanced lung cancer is vital, focusing on symptom management and enhancing the quality of life for patients. While national guidelines are available for the diagnosis and treatment of lung cancer, significant disparities in healthcare access remain across Indonesia. Thus, it is essential to improve universal health coverage and referral systems to guarantee equal access to lung cancer care for patients at all levels through advocacy and ease of access.
Próba przeszczepienia typomorfologii Pierre’a Schaeffera do analizy wybranych słuchowisk eksperymentalnych Polskiego Radia
Authors: Łastowiecki Janusz 
Published: January 2025

Tekst próbuje skonfrontować typomorfologię stworzoną w latach 50. przez Pierre’a Schaeffera z analizą i interpretacją eksperymentalnych słuchowisk Teatru Polskiego Radia i Studia Eksperymentalnego. Za przykład służą tu te utwory, które w swojej warstwie fabularnej i dźwiękowej odwołały się do tematu kolejowego. Pociąg pojawia się również jako temat w kluczowej dla typomorfologicznych rozważań kompozycji Schaeffera Étude aux chemins de fer. Pod badawczą lupę wzięte zostały zarówno adaptacje radiowe (Siekierezada i Fabula rasa Edwarda Stachury, Wszystko płynie Wasilija Grossmana, Szalona lokomotywa Stanisława Ignacego Witkiewicza) jak i utwory oryginalne Teatru Polskiego Radia (Kaktus Grzegorza Walczaka). Obok klasycznych słuchowisk pole do eksplikacji stanowią tu utwory Studia Eksperymentalnego Polskiego Radia (Śniadanie na trawie w grocie Lascaux, Ptacy i ludzie Eugeniusza Rudnika). Ciekawym kontekstem dla prowadzonych nad audiosferą badań jest analiza eseju dźwiękowego Zuzanny Solakiewicz i Marcina Lenarczyka 15 stron świata. Próba konfrontacji języka typomorfologii z zjawiskami dźwiękowymi wybranych spektakli jest tu poszerzona o kontekst kolejowy, tak ważny dla zrozumienia kodu muzycznego Schaeffera. Odczytanie dźwięku w kategoriach masy, dynamiki i trwałości przyniesie nowe konteksty analityczne względem myślenia o artystycznych formach radiowych.
O rękopisie utworu „Polowanie” czyli „Heca albo polowanie na zająca...” ze zbiorów Księży Misjonarzy w Wilnie
Authors: Dacewicz Alicja 
Published: January 2025

Komunikat dotyczy dwóch woluminów rękopiśmiennych znajdujących się obecnie w Dziale muzycznym Litewskiej Państwowej Biblioteki im. Martinasa Mażwidasa [Lietuvos Nacionalinės Martyno Mažvydo bibliotekos Muzikos skyrius] pod sygnaturą Mkrn-11. Badaczki z Litwy Laima Budzinauskienė i Agnė Januškaitė nazwały rękopisy ,,Wileńską Księgą Seminaryjną”. Autorka komunikatu dochodzi do wniosku, że wileńskie muzyczne woluminy rękopiśmienne powstały w 1828 r. u Księży Misjonarzy św. Wincentego á Paulo na Górze Zbawiciela w Wilnie i do zamknięcia Domu Misjonarzy w Wilnie w 1844 r. były własnością seminarium internum Księży Misjonarzy św. Wincentego á Paulo na Górze Zbawiciela w Wilnie. Dopiero po 1844 r. muzykalia trafiły do Biblioteki Wileńskiego Rzymsko-Katolickiego Seminarium Diecezjalnego, znajdującego się przy kościele pokarmelitańskim św. Jerzego, gdzie przetrwały do naszych czasów. Umieszczona w zbiorze utworów religijnych kompozycja Polowanie jest zdekompletowanym egzemplarzem opery Heca albo polowanie na zająca. Anonimowa krotochwila myśliwska w jednym akcie.
Towards the computer systems design based on Zero Trust Architecture
Authors: Brazhuk A. I. , Olizarovich E. V. 
Published: January 2025

The work is devoted to theoretical and practical aspects of computer systems design based on the zero trust concept. Based on the system thinking of analyzing existing zero trust systems and theoretical models used in their design, the work describes key problems of implementing zero trust systems. Also, based on design and security patterns, the principles representation of the zero trust concept and the abstract access control model (pattern) of the Zero Trust Architecture are considered.The principles representation can be used to mine abstract design and security patterns, and the access control pattern – to create derivative patterns and architectures of computer systems based on zero trust. An advance of the access control pattern is the capacity to more fully formulate functional requirements and represent the architectures of the designed systems due to the description of access control levels (network path, session, transaction).
Utilization and Efficiency of eLearn Functionalities in a University
Authors: Redondo Rule P. , Tagarda Eloiza P. , Sumalinog Leonita C. 
Published: January 2025

This study determined the utilization, satisfaction and perceived efficiency of the eLearning portal in a university known as eLearn. It is a web-based learning management system to aid classroom instruction that fosters self-directed learning. The mixed method of research was used in this study and utilized the researcher-made questionnaire as the main instrument. This employed the quota sampling procedure. A total of 376 out of 9,130 college students were the participants of this study. The statistical tools utilized in the study consisted of Descriptive Statistics such as mean, standard deviations, frequency and percentages to describe the variables. Spearman’s rho ( ) was also utilized to determine the relationship of the variables under study. The findings revealed that the majority of the participants used eLearn, found it beneficial to their studies, were satisfied with the eLearn functionalities and perceived the functionalities as highly efficient. The students' utilization of eLearn and satisfaction with the system's functionalities were not significantly associated with their perceived efficiency of the system. This implies that mere utilization of the eLearn does not predict their perception of efficiency. The study concludes that eLearn in the university can be an effective tool in the teaching and learning processes and in the delivery of information resources. However, there is a need to encourage more teachers to maximize the utilization of this E-Learning portal. Furthermore, the study recommends that the findings be revealed to the administrators, Computing and Information Services Office, faculty and librarians so that through their combined efforts there would be more use of the eLearn.
A New Approach to Identifying Red Supergiant Stars in Metal-poor Galaxies: A Case Study of NGC 6822
Authors: Li 李 Zhi-wen 志文 , Yang 杨 Ming 明 , Jiang 姜 Biwei 碧沩 , Ren 任 Yi 逸 
Published: January 2025

Abstract
A complete sample of red supergiant (RSG) stars is important for studying their properties. Identifying RSGs in extragalactic fields first requires removing the Galactic foreground dwarfs. The color–color diagram (CCD) method, specifically using r − z/z − H and J − H/H − K, has proven successful in several studies. However, in metal-poor galaxies, faint RSGs will mix into the dwarf branch in the CCD and would be removed, leading to an incomplete RSG sample. This work attempts to improve the CCD method in combination with the Gaia astrometric measurement to remove foreground contamination in order to construct a complete RSG sample in metal-poor galaxies. The empirical regions of RSGs in both CCDs are defined and modified by fitting the locations of RSGs in galaxies with a range of metallicity. The metal-poor galaxy NGC 6822 is taken as a case study for its low metallicity ([Fe/H] ≈ −1.0) and moderate distance (about 500 kpc). In the complete sample, we identify 1184 RSG, 1559 oxygen-rich AGB (O-AGBs), 1075 carbon-rich AGB (C-AGBs), and 140 extreme AGB (x-AGBs) candidates, with a contamination rate of approximately 20.5%, 9.7%, 6.8%, and 5.0%, respectively. We also present a pure sample, containing only the sources away from the dwarf branch, which includes 843 RSG, 1519 O-AGB, 1059 C-AGB, and 140 x-AGB candidates, with a contamination rate of approximately 6.5%, 8.8%, 6.1%, and 5.0%, respectively. About 600 and 450 RSG candidates are newly identified in the complete and pure samples, respectively, compared to the previous RSG sample in NGC 6822.
Ion Charge States from a Global Time-dependent Wave-turbulence-driven Model of the Solar Wind: Comparison with in Situ Measurements
Authors: Riley Pete , Lionello Roberto , Rivera Yeimy J. 
Published: January 2025

Abstract
Solar wind charge-state measurements contain a wealth of knowledge related to the properties of the solar corona from where they originated. However, their interpretation has remained challenging because it convolves coronal temperature, density, and velocity along the particles’ trajectory through the corona before they “freeze in” and are convected outward through the solar wind. In this study, we calculate ion charge states by coupling a nonequilibrium ionization model with a global magnetohydrodynamic model of the corona and inner heliosphere. We present results for two periods characteristic of solar minimum and maximum and compare them with observations from the ACE spacecraft. We find that the model reproduces the essential features of the observations, rectifying an earlier inconsistency that was apparent in 1D calculations, and allows us to unambiguously trace the evolution of charge states from the base of the corona into the solar wind.
Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona
Authors: Sridhar Navin , Ripperda Bart , Sironi Lorenzo , Davelaar Jordy , Beloborodov Andrei M. 
Published: January 2025

Abstract
Using two-dimensional general relativistic resistive magnetohydrodynamic simulations, we investigate the properties of the sheath separating the black hole jet from the surrounding medium. We find that the electromagnetic power flowing through the jet sheath is comparable to the overall accretion power of the black hole. The sheath is an important site of energy dissipation as revealed by the copious appearance of reconnection layers and plasmoid chains. About 20% of the sheath power is dissipated between 2 and 10 gravitational radii. The plasma in the dissipative sheath moves along a nearly paraboloidal surface with transrelativistic bulk motions dominated by the radial component, whose dimensionless 4-velocity is ∼1.2 ± 0.5. In the frame moving with the mean (radially dependent) velocity, the distribution of stochastic bulk motions resembles a Maxwellian with an “effective bulk temperature” of ∼100 keV. Scaling the global simulation to Cygnus X-1 parameters gives a rough estimate of the Thomson optical depth across the jet sheath, ∼0.01–0.1, and it may increase in future magnetohydrodynamic simulations with self-consistent radiative losses. These properties suggest that the dissipative jet sheath may be a viable “coronal” region, capable of upscattering seed soft photons into a hard, nonthermal tail, as seen during the hard states of X-ray binaries and active galactic nuclei.
Angular Power Spectrum of TeV–PeV Cosmic-Ray Anisotropies
Authors: Bian Wenyi , Giacinti Gwenael , Reville Brian 
Published: January 2025

Abstract
Simulations of the cosmic-ray (CR) anisotropy down to TeV energies are presented, using turbulence parameters consistent with those inferred from observations of the interstellar medium. We compute the angular power spectra C

ℓ
of the CR anisotropy obtained from the simulations. We demonstrate that the amplitude of the large-scale gradient in the CR density profile affects only the overall normalization of the C

ℓ
values, without affecting the shape of the angular power spectrum. We show that the power spectrum depends on CR energy and that it is sensitive to the location of the observer at small ℓ. It is found to flatten at large ℓ and can be modeled by a broken power law, exhibiting a break at ℓ ≈ 4. Our computed power spectrum at ~10 TeV fits well HAWC and IceCube measurements. Moreover, we calculate all coefficients of the spherical harmonics and compute the component of the angular power spectrum projected onto the direction of the local magnetic field line. We find that deviations from gyrotropy become increasingly important at higher CR energies and larger values of ℓ.
Pulsar Scattering as a Probe for Structures in the Interstellar Medium
Authors: He Qiuyi , Shi Xun , Li Guangxing 
Published: January 2025

Abstract
Due to the inhomogeneity of electron number density, radio waves emitted by pulsars undergo scattering as they pass through the interstellar medium (ISM). However, a connection between large-scale pulsar scattering data and the structure of the Galactic ISM has yet to be established. In this paper, we explore the capability of pulsar scattering time data in discovering structures in the ISM. Using a large data set of scattering time measurements for 473 pulsars, we fit the pulsar reduced scattering intensity as a function of Galactic latitude and distance, constructing a smooth model of the Galactic pulsar scattering distribution. By comparing this smooth distribution with observational data, we identify two ISM structures responsible for pulsar scattering, one is associated with the Vela supernova remnant region within the Gum Nebula, while the other is a newly discovered structure—a distant superbubble, G38, located at a distance of 2.3 kpc with a size of ~50 pc. Analysis of the correlation coefficient of the pulsar scattering distribution shows that the correlation is dominated by structures smaller than 0.15 kpc—the closest separation approachable by the current data set. As measurements of the pulsar scattering time continue to increase in the future, they can potentially become an independent tool for exploring structures in the ISM.
Ubiquitous Small-scale Extreme-ultraviolet Upflow-like Events above Network Regions Observed by the Solar Orbiter/Extreme Ultraviolet Imager
Authors: Duan Yadan , Chen Hechao , Hou Zhenyong , Sun Zheng , Shen Yuandeng 
Published: January 2025

Abstract
Universal small-scale solar activity in the quiet region is suggested to be a potential source of solar wind and the upper solar atmosphere. Here, with the high-resolution 174 Å imaging observations from the Solar Orbiter/Extreme Ultraviolet Imager, we investigate 59 EUV upflow-like events observed in the quiet Sun. Their average apparent (plane-of-sky) velocity, lifetime, and propagation distance are measured as 62 km s−1, 68.6 s, and 3.94 Mm, respectively. These upflow-like events exhibit dynamic characteristics but lack base brightening, featuring a hot front and subsequent cold plasma ejection. A total of 39% of the EUV upflow-like events exhibit recurrent characteristics. Unprecedented high-resolution 174 Å observations reveal that some EUV upflow-like events exhibit blob-like fine structures and multistrand evolutionary features, and some upflow-like events can cause localized haze-like plasma heating ahead of their spire region during the ejection process. A subset of the EUV upflow-like events covered by the Solar Dynamics Observatory reveals that they appear at the chromospheric networks. Through emission measure analysis, we found that these upflow-like events eject hot plasma of transient region or coronal temperature (an average of ~105.5 K). We suggest that EUV upflow-like events may be EUV counterparts of chromospheric spicules and/or transition region network jets and play a role in heating the localized corona above the network regions.
Multiwavelength Emission of Gamma-Ray Burst Prompt Phase. II. Spectral Polarimetry
Authors: Li Jia-Sheng , Lan Mi-Xiang 
Published: January 2025

Abstract
Polarization spectra were predicted within the photosphere model. To seek more clues to distinguish between the models, both the time-resolved and time-integrated polarization spectra from optical band to MeV gamma-rays of the magnetic reconnection model are studied here. There are two newly found differences between the two models. First, the time-integrated polarization degree of the magnetic reconnection model would in general increase with frequency for on-axis observations, while it is not monotonous for the photosphere model. Second, the variations of both the time-integrated and the time-resolved polarization angles (PAs) with frequency of the magnetic reconnection model are not random, while the time-integrated PA varies randomly with frequency for the photosphere model. Therefore, future energy-resolved polarization analysis could distinguish between the two models. In addition, the PA rotation spectra are studied for the first time. The rotation value of PA within the burst duration will decrease with the increase of the observational energy band. Most significant PA rotation would happen for slightly off-axis observations in each energy band. The PA would rotate even for on-axis observations in the optical band. Compared with the aligned magnetic field case, the PA rotation is quite rare in the gamma-ray band for the case with a toroidal field in the radiation region.
A Systematic Review on the Effects of Short-Term Exposure to Bisphenol-A and Bisphenol-S During Embryonic Stages of Zebrafish (<em>Danio rerio</em>)
Authors: Dulanthi M. L. Y. , Rajapaksa G. 
Published: January 2025

Bisphenol-A is a highly used industrial chemical and a pervasive environmental oestrogen. Therefore, bisphenol-S was introduced as a safe alternative, yet endocrine disruption properties have been reported. Therefore, the safety of bisphenol-S as a safe substitute of bisphenol-A has become questionable. Yet, the existing published literature on comparative assessment of bisphenol effects are not conclusive. Therefore, a systematic review was carried out to comprehend the relative effects of bisphenols, by comparing the growth-related effects of early-life exposure to bisphenol-A and bisphenol-S in the model organism, Danio rerio (Zebrafish). The review analysed the published research through Preferred Reporting Items for Systematic Reviews and Meta-Analyses (PRISMA) strategy. The search was conducted in Research Gate, Pub Med, Google Scholar, and Science Direct databases for articles published from the start of database coverage until August 2021, searching for articles on survival and growth-related effects of bisphenols in embryonic stages of zebrafish. Out of 181 articles, only 7 articles became eligible for inclusion criteria of early life (embryo) short-term bisphenol exposure. In recruited articles, hatching rate, body length, locomotion, malformations and survival of zebrafish were analysed under bisphenol concentrations of 0.0001 mg/L to 100mg/L. Studies on hatching rate have reported that exposure to both types of bisphenols in the concentration range of 1-100 µg/L significantly increase the hatching rate in a comparable manner. One study has reported that bisphenol-S significantly decreases embryo survival in lower concentrations than bisphenol-A. Decreased body length under the concentration range of 0.1-100 µg/L were evident for both bisphenols in a comparable manner. Based on the systematic review, it can be concluded that acute exposure to bisphenol-A and bisphenol-S exert similar effects to zebrafish embryos. Therefore the claim on the bisphenol-S as a safe bisphenol-A substitute warrants further investigations.
A descriptive study of syphilitic uveitis in patients treated at tertiary hospitals in Johannesburg
Authors: Rawjee Kashmira , Makgotloe Mokokomadi A. 
Published: January 2025

Background: Syphilitic uveitis is a ‘great mimicker’ with a myriad of manifestations resembling other forms of inflammation in the eye. A large percentage of patients with syphilitic uveitis in South Africa have HIV co-infection and their clinical features and serological results may be confounded by the presence of HIV.Aim: This study aimed to describe the clinical features of patients treated for syphilitic uveitis at two tertiary hospitals in Johannesburg.Setting: The study was conducted at the ophthalmology departments of two tertiary hospitals in Johannesburg.Methods: A retrospective descriptive case series of patients admitted for treatment of syphilitic uveitis at Charlotte Maxeke Johannesburg Academic Hospital and Chris Hani Baragwanath Hospitals.Results: From 01 January 2015 to 30 June 2020, 25 patients (44 eyes) were admitted for syphilitic uveitis treatment. Vitritis was the most common sign in 54.5% of the patients (n = 24 eyes) and 23 of these eyes were of HIV positive patients. Anterior chamber cells were in 43.1% of the patients (n = 19 eyes), posterior synechiae in 36.3% (n = 16 eyes), optic disc swelling in 31.8% (n = 14 eyes), pigmentary retinopathy in 18.1% (n = 8 eyes) and ciliary injection in 18.1% (n = 8 eyes). Optic disc swelling was observed in 57.1% (n = 4 eyes) of HIV negative patients. There was an improvement in visual acuity (VA) in 64.3% of eyes (n = 27) and no change in VA in 35.7% (n = 15) of eyes. No deterioration in post-treatment VA was documented.Conclusion: Majority of the patients admitted for syphilitic uveitis had posterior segment signs, which should prompt a diagnosis of syphilis. The treatment of syphilitic uveitis leads to an improvement in VA.Contribution: This work contributes to our understanding of syphilitic uveitis presentation in South African hospitals.