bluuebunny/crossref_metadata_2025_split huggingface dataset:
ANALYSIS OF THE DEGREE OF RESTORATION OF CHECKING EFFICIENCY IN THE PARTIAL ABSENCE OF TEETH AFTER ORTHOPEDIC TREATMENT WITH REMOVABLE PROSTHESES
Authors: Беленова Ирина Александровна , Морозов Николай Валерьевич , Комарова Юлия Николаевна , Беленов Иван Сергеевич 
Published: July 2022

В работе приведены результаты восстановления жевательной эффективности у 60 пациентов с диагнозом частичное отсутствие зубов после протезирования различными видами ортопедических съемных протезов, включая разработанную модифицированную конструкцию комбинированного дугового протеза с эластичным полимером. Дана сравнительная характеристика применения модифицированной конструкцией комбинированного дугового протеза с эластичным полимером, съемных пластиночных протезов с кламмерной фиксацией из акриловых полимеров и ортопедических конструкций из безакриловых литьевых термопластических полимеров у трех групп пациентов с дефектами зубных рядов. Описана применяемая динамическая функциональная проба анализа жевательной эффективности, адаптированная для пациентов с частичным отсутствием зубов до и после ортопедического лечения. Данная жевательная проба, разработанная под руководством профессора В.Н. Трезубова, является экспресс-методом оценки жевательной эффективности. Приведены сравнительные результаты оценки восстановления функции жевания у пациентов всех групп на разных сроках протезирования. На основании полученных результатов были сделаны выводы о высокой функциональной ценности модифицированной конструкции комбинированного дугового протеза с эластичным полимером, применение которого в ортопедической практике позволяет повысить качество ортопедической помощи при съемном протезировании, сокращая время адаптации к протезам
The paper provides outcomes of the chewing efficiency restoration in 60 patients with partial teeth loss after prosthetics with various orthopedic removable dentures including the developed modification of a combined arc prosthesis with an elastic polymer. The study compared application of the above denture modification, removable lamellar dentures with clasp fixation made of acrylic polymers and orthopedic structures made of non-acrylic molded thermoplastic polymers in three groups of patients with dentition defects. The authors analysed chewing effectiveness before and after orthopedic treatment using an express dynamic functional test adapted for patients with partial teeth loss. The test was developed under Professor Trezubov guidance. The study compared outcomes of restoration of chewing function in patients of all groups at different terms of prosthetics. Based on the results obtained, it is concluded that the modified combined arc prosthesis with an elastic polymer has a high functional value; its application in orthopedic practice contributes to the improved quality of orthopedic care with removable prosthetics, reducing the terms of adaptation to prostheses
UPAYA MENINGKATKAN KEDISIPLINAN ANAK DALAM MEMATUHI PROTOKOL KESEHATAN PADA MASA PANDEMI COVID 19 DI TPA NURUL QURAN GUNUNG PUTRI, BOGOR
Authors: Siti Fatimah Okta Zenita 
Published: July 2022

Kasus Covid-19Â tidak hanya menyerang orang dewasa,Â namun anakÂ pun dapat menjadi korban penyakit pernafasan ini. Penyebaran covid-19 disebabkan karena kelalaian dalam memperhatikan protokol kesehatan. TPA Nurul Quran tetap memberlakukan siswanya untuk belajar dengan cara membagi menjadi beberapa kelompok (kelas) namun kondisi ini masih sangat rentan penyebaran Covid-19 jika tidak diimbangi kesadaran siswa mematuhi protokol kesehatan dengan tepat. Kegiatan pengabdian yang akan kami laksanakan adalah kegiatan penyuluhan. Media yang akan digunakan dalan penyuluhan ini adalah media audio visual yang didalamnya berisi tentangÂ berisi informasi mengenai covid 19 serta cara pencegahannya. Dengan Kegiatan pengabdian ini diharapkan masyarakat sadar akan pentingnya konsistensi protokol kesehatan dengan tepat untuk mencegah transmisi serta dapat menjadikan kegiatan penyuluhan ini sebagai salah satu program yang laksanakan secara rutin oleh TPA Nurul Quran.Hasil pengabdian masyarakat ini yaitu meningkatnya pengetahuan siswa yang membuktikan masyarakat semakin tahu kedisiplinan pada protokol kesehatan dan semakin ketat untuk cegah transmisi penyebaran virus corona.Kata kunci : peningkatan kedisiplinan, protokol kesehatan
Membangun Brand Image Melalui Digital Marketing Di Kelurahan Gedong, Kecamatan Pasar Rebo, Jakarta Timur
Authors: Hariani Danarti , Effendi Muhammad Ridwan , Panggabean Helena Louise 
Published: July 2022

Kegiatan Pengabdian Kepada MasyrakatÂ dengan Â subtema Membangun Brand Image Melalui Digital MarketingÂ merupakan salasatuÂ tema yang disampaikanÂ Â dalam kegiatan Pengabdian Kepada MasyrakatÂ Â dengan judulÂ Membangun Brand Image MelaluiÂ BahasaÂ Marketing Â bagiÂ ibu-ibu PKK Di kelurahan Gedong , Kecamatan Pasar Rebo, Jakarta Timur. Kegiatan Pengabdian Masyrakat ini merupakan kegiatanÂ yang dilaksanakan lintas prodi yaitu fakultas Keguruan dan Ilmu Pendidikan , Fakultas Ekonomi dan Bisnis, Fakultas Komputer dan Fakultas Kesehatan Universitas Mochammad Husni Thamrin danÂ Â masing masing program studiÂ menyampaikan materinya sesuai dengan kompetensinya. Â Tujuan dari kegiatan Â pengabdian Masyarakat ini Â adalah Â memberikan informasi dan pemahamanÂ kepada para ibu kader PKK kelurahan Kampung GedongÂ agar mampu membangun Brand image produk dan layanan bagiÂ usaha rumahannya guna memperoleh penghasilan tambahan untuk keluarga. SalahsatuÂ subtema yang disampaikan adalah membangun brand image melalui digital marketing.Ibu-ibu PKK di kelurahan gedong iniÂ sebagian besar adalah ibu rumah tangga yang mempunyai usaha rumahan yaitu aneka ragam kuliner yang diperjualbelikan di masyarakat sekitar. Potensi berwirausaha ibu-ibu kader PKK ini cukup besar namun minimnya pengetahuanÂ dan pemahaman terhadap kemampuan membangun Â brand image Â terhadap produkÂ usaha mereka menyebabkan bisnis rumahan mereka cenderung kurang berkembang dan terbatas. Selama ini, promosi yang dilakukan oleh Ibu â€“ Ibu PKK adalah promosi tradisional, yaitu promosi dari mulut ke mulut dan hanya disekitaran lingkungan tempat tinggal mereka. Â Di era digital saat ini, salah satu kemampuan yang perlu dimiliki oleh setiap orang,termasuk Â Ibu â€“ Ibu PKK adalah Internet. Internet merupakan sarana Digital Marketing yang dapat digunakan untuk melakukan promosi usahanya , sehingga usahanya dapat lebih dikenal oleh banyak pihak. Oleh karena itu diharapkan dengan adanya seminarÂ ini, Ibu â€“ Ibu PKK dapat memanfaatkan internet melalui Handphone mereka untuk memperkenalkan produk yang mereka buat kepada pihak luar.Pelaksanaan kegiatan dilakukanÂ melalui acara seminar pengabdian masyarakat yang dilaksanakan di Aula Kelurahan Gedong yang dihadiri oleh ibu-ibu kader PKK dengan kuota terbatas karena dilakukan pada masa PPKM Â Pandemi Covid-19.dan secara keseluruhan bisa Â berjalan dengan baik dan peserta sangat antusias dalam mengikuti selama kegiatan. Harapan peserta agar kegiatan pengabdian kepada masyarakat ini dapat dilaksanakan secara berkesinambungan oleh Universitas MH. Thamrin, karena melalui kegiatan ini dapat memberikan informasi , pengetahuan serta pemahaman Â mengenai Pemberdayaan wanita sehingga Â mampu berperan Â sebagai motor penggerak ekonomi keluarga dan masyarakat.Â Kata Kunci: Pengabdian kepada Masyarakat , Brand Image,Digital Marketing, Ibu PKK Kelurahan Gedong
SARS-CoV-2 Serology Antibody in Children with MIS-C (Multiple Inflammatory Syndrome in Children) Suspected
Authors: Yani Finny Fitry , Indra Ihsan  , Efrida  
Published: July 2022

Background: Multiple inflammatory syndromes in children (MIS-C) relate to COVID-19 severity in children. SARS-CoV-2 serology antibody is one of the diagnostic tools of MIS-C. The study aimed to describe the yield of serology antibodies of MIS-C and some characteristics found in hospitalized children with MIS-C suspects.
Methods: This research was an analytic observational study. The data were collected retrospectively from some children who were hospitalized in Dr. M. Djamil General Hospital, Padang, West Sumatra, Indonesia, from April - June 2021. The inclusion criteria were children aged 1 month to 18 years, with or without contact history with the person who probable or confirmed COVID-19 and have signs and symptoms as MIS-C base on WHO criteria.
Results: About eight out of 44 children showed positive serology antibodies and were diagnosed as MISC (18,2%). Based on demographic characteristics, children aged 11-15 years (27.3%) and boys were more affected (52.3%) as MIS-C suspected. Most of them were referred from a 2nd-level hospital outside Padang City (70.4%), but only 13.6% had a history of contact with COVID-19 confirmation patients. There was a significant difference in cardiovascular signs and symptoms between positive and negative serology antibody SARS-CoV-2 among children with MIS-C suspected (p<0.05), but not in fever, respiratory distress, gastrointestinal, neurology symptoms, either in laboratory results such as leukocytes, CRP and D-dimmer. Intravenous immunoglobulin, steroid, and PICU admitted showed no significant differences between the 2 groups, but more death prevalence in positive than negative. However, no significant differences (12.5% vs. 11.1%, p>0.05).
Conclusion: Cardiovascular signs and symptoms could be proposed to be one of the significant differences in clinical conditions to differentiated children with MIS-C suspected and MIS-C due to serology antibody results.
Business Feasibility Study Analysis on Coffee Shop Business
Authors: Ahmad Hidayat  , Uda Tonich , Windy Utami Putri  , Alexandro Rinto 
Published: July 2022

In recent years, SMEs engaged in the creative industry sector in the coffee shop business have continued to show their existence, one of which is the Meine Welt Coffee coffee shop business. This study aims to analyze the feasibility of a coffee shop business at a Meine Welt coffee shop business to find out whether the current business can provide the expected financial benefits with a qualitative approach, namely a research procedure that produces descriptive data collected through interviews, observations and documentation. Sources of data used are primary and secondary data. While the analysis technique used is qualitative analysis techniques to assess legal aspects, environmental aspects, market and marketing aspects, technical and technological aspects, management and human resources aspects and financial aspects. The results of this study indicate that based on non-financial aspects this coffee shop is feasible to run. Analysis of the financial aspects of the Meine Welt coffee shop shows the NPV value of IDR 115,505,164, the Payback Period (PP) for 3 years and 3 months, Profitability Index (PI) 1.78, Internal Rate of Return (IRR) of 36.60%, and Average Rate of Return (ARR) of 160%.
Environmental Effects in Herschel Observations of the Ionized Carbon Content of Star-forming Dwarf Galaxies in the Virgo Cluster∗
Authors: Minchin Robert , Fadda Dario , Taylor Rhys , Deshev Boris , Davies Jonathan 
Published: July 2022

Abstract
We use archival Herschel data to examine the singly ionized carbon ([C II]) content of 14 star-forming dwarf galaxies in the Virgo cluster. We use spectral energy distribution fits to far-infrared, mid-infrared, near-infrared, optical, and ultraviolet data to derive the total infrared continuum (TIR) for these galaxies. We compare the [C II]/TIR ratio for dwarf galaxies in the central part of Virgo to those in the southern part of the cluster and to galaxies with similar TIR luminosities and metallicities in the Herschel Dwarf Galaxy Survey (DGS) sample of field dwarf galaxies to look for signs of [C II] formation independent of star formation. Our analysis indicates that the sample of Virgo dwarfs in the central part of the cluster has significantly higher values of [C II]/TIR than the sample from the southern part of the cluster and the sample from the DGS, while the southern sample is consistent with the DGS. This [C II]/TIR excess implies that a significant fraction of the [C II] in the dwarf galaxies in the cluster center has an origin other than star formation and is likely to be due to environmental processes in the central part of the cluster. We also find a surprisingly strong correlation between [C II]/TIR and the local ram pressure felt by the dwarf galaxies in the cluster. In this respect, we claim that the excess [C II] we see in these galaxies is likely to be due to formation in ram-pressure shocks.
Parallel Plasma Loops and the Energization of the Solar Corona
Authors: Peter Hardi , Chitta Lakshmi Pradeep , Chen Feng , Pontin David I. , Winebarger Amy R. , Golub Leon , Savage Sabrina L. , Rachmeler Laurel A. , Kobayashi Ken , Brooks David H. , Cirtain Jonathan W. , De Pontieu Bart , McKenzie David E. , Morton Richard J. , Testa Paola , Tiwari Sanjiv K. , Walsh Robert W. , Warren Harry P. 
Published: July 2022

Abstract
The outer atmosphere of the Sun is composed of plasma heated to temperatures well in excess of the visible surface. We investigate short cool and warm (<1 MK) loops seen in the core of an active region to address the role of field-line braiding in energizing these structures. We report observations from the High-resolution Coronal imager (Hi-C) that have been acquired in a coordinated campaign with the Interface Region Imaging Spectrograph (IRIS). In the core of the active region, the 172 Å band of Hi-C and the 1400 Å channel of IRIS show plasma loops at different temperatures that run in parallel. There is a small but detectable spatial offset of less than 1″ between the loops seen in the two bands. Most importantly, we do not see observational signatures that these loops might be twisted around each other. Considering the scenario of magnetic braiding, our observations of parallel loops imply that the stresses put into the magnetic field have to relax while the braiding is applied: the magnetic field never reaches a highly braided state on these length scales comparable to the separation of the loops. This supports recent numerical 3D models of loop braiding in which the effective dissipation is sufficiently large that it keeps the magnetic field from getting highly twisted within a loop.
The Nature of Low-surface-brightness Galaxies in the Hyper Suprime-Cam Survey
Authors: Greene Jenny E. , Greco Johnny P. , Goulding Andy D. , Huang 黄 Song 崧 , Kado-Fong Erin , Danieli Shany , Li 李 Jiaxuan 嘉轩 , Kim Ji Hoon , Komiyama Yutaka , Leauthaud Alexie , MacArthur Lauren A. , Sifón Cristóbal 
Published: July 2022

Abstract
We present the statistical redshift distribution of a large sample of low-surface-brightness (LSB) galaxies identified in the first 200 deg2 of the Hyper Suprime-Cam Strategic Survey Program. Through cross-correlation with the NASA–SDSS Atlas, we find that the majority of objects lie within z < 0.15 or ∼500 Mpc, yielding a mass range of M
* ≈ 107−109
M
⊙ and a size range of r
eff,g
≈ 1−8 kpc. We find a peak in the distance distribution within 100 Mpc, corresponding mostly to ∼107
M
⊙ galaxies that fall on the known mass–size relation. There is also a tail in the redshift distribution out to z ≈ 0.15, comprising more massive (M
* = 108 − 109
M
⊙) galaxies at the larger end of our size range. We see tentative evidence that at the higher-mass end (M
* > 108
M
⊙), the LSB galaxies do not form a smooth extension of the mass–size relation of higher-surface-brightness galaxies, perhaps suggesting that the LSB galaxy population is distinct in its formation path.
Numerical Investigations of Catastrophe in Coronal Magnetic Configuration Triggered by Newly Emerging Flux
Authors: Chen Yuhao , Ye Jing , Mei Zhixing , Shen Chengcai , Roussev Ilia I. , Forbes Terry G. , Lin Jun , Ziegler Udo 
Published: July 2022

Abstract
We performed 2D magnetohydrodynamical numerical experiments to study the response of the coronal magnetic configuration to the newly emerging magnetic flux. The configuration includes an electric-current-carrying flux rope modeling the prominence floating in the corona and the background magnetic field produced by two separated magnetic dipoles embedded in the photosphere. Parameters for one dipole are fixed in space and time to model the quiet background, and those for another one are time dependent to model the new flux. These numerical experiments duplicate important results of the analytic solution but also reveal new results. Unlike previous works, the configuration here possesses no symmetry, and the flux rope could move in any direction. The non-force-free environment causes the deviation of the flux rope equilibrium in the experiments from that determined in the analytic solution. As the flux rope radius decreases, the equilibrium could be found, and it evolves quasi-statically until the flux rope reaches the critical location at which the catastrophe occurs. As the radius increases, no equilibrium exists at all. During the catastrophe, two current sheets form in different ways. One forms as the surrounding closed magnetic field is stretched by the catastrophe, and another one forms as the flux rope squeezes the magnetic field nearby. Although reconnection happens in both the current sheets, it erases the first one quickly and enhances the second simultaneously. These results indicate the occurrence of the catastrophe in asymmetric and non-force-free environment, and the non-radial motion of the flux rope following the catastrophe.
Spectra of Cosmic-Ray Sodium and Aluminum and Unexpected Aluminum Excess
Authors: Boschini M. J. , Torre S. Della , Gervasi M. , Grandi D. , Jóhannesson G. , La Vacca G. , Masi N. , Moskalenko I. V. , Pensotti S. , Porter T. A. , Quadrani L. , Rancoita P. G. , Rozza D. , Tacconi M. 
Published: July 2022

Abstract
Since its launch, the Alpha Magnetic Spectrometer-02 (AMS-02) has delivered outstanding quality measurements of the spectra of cosmic-ray (CR) species,

p

¯

, e
±, and nuclei (H–Si, Fe), which resulted in a number of breakthroughs. The most recent AMS-02 result is the measurement of the spectra of CR sodium and aluminum up to ∼2 TV. Given their low solar system abundances, a significant fraction of each element is produced in fragmentations of heavier species, predominantly Ne, Mg, and Si. In this paper, we use precise measurements of the sodium and aluminum spectra by AMS-02 together with ACE-CRIS and Voyager 1 data to test their origin. We show that the sodium spectrum agrees well with the predictions made with the GalProp-HelMod framework, while the aluminum spectrum shows a significant excess in the rigidity range from 2–7 GV. In this context, we discuss the origin of other low-energy excesses in Li, F, and Fe found earlier. The observed excesses in Li, F, and Al appear to be consistent with the local Wolf-Rayet stars hypothesis, invoked to reproduce anomalous 22Ne/20Ne, 12C/16O, and 58Fe/56Fe ratios in CRs, while excess in Fe is likely connected with a past supernova activity in the solar neighborhood. We also provide updated local interstellar spectra (LIS) of sodium and aluminum in the rigidity range from a few megavolts to ∼2 TV. Our calculations employ the self-consistent GalProp-HelMod framework, which has proved to be a reliable tool in deriving the LIS of CR

p

¯

, e
−, and nuclei Z ≤ 28.
The Independence of Oscillatory Reconnection Periodicity from the Initial Pulse
Authors: Karampelas Konstantinos , McLaughlin James A. , Botha Gert J. J. , Régnier Stéphane 
Published: July 2022

Abstract
Oscillatory reconnection can manifest through the interaction between the ubiquitous MHD waves and omnipresent null points in the solar atmosphere and is characterized by an inherent periodicity. In the current study, we focus on the relationship between the period of oscillatory reconnection and the strength of the wave pulse initially perturbing the null point, in a hot coronal plasma. We use the PLUTO code to solve the fully compressive, resistive MHD equations for a 2D magnetic X-point. Using wave pulses with a wide range of amplitudes, we perform a parameter study to obtain values for the period, considering the presence and absence of anisotropic thermal conduction separately. In both cases, we find that the resulting period is independent of the strength of the initial perturbation. The addition of anisotropic thermal conduction only leads to an increase in the mean value for the period, in agreement with our previous study. We also consider a different type of initial driver and we obtain an oscillation period matching the independent trend previously mentioned. Thus, we report for the first time on the independence between the type and strength of the initializing wave pulse and the resulting period of oscillatory reconnection in a hot coronal plasma. This makes oscillatory reconnection a promising mechanism to be used within the context of coronal seismology.
Global Kinetic Modeling of the Intrabinary Shock in Spider Pulsars
Authors: Cortés Jorge , Sironi Lorenzo 
Published: July 2022

Abstract
Spider pulsars are compact binary systems composed of a millisecond pulsar and a low-mass companion. The relativistic magnetically dominated pulsar wind impacts onto the companion, ablating it and slowly consuming its atmosphere. The interaction forms an intrabinary shock, a proposed site of particle acceleration. We perform global fully kinetic particle-in-cell simulations of the intrabinary shock, assuming that the pulsar wind consists of plane-parallel stripes of alternating polarity and that the shock wraps around the companion. We find that particles are efficiently accelerated via shock-driven reconnection. We extract first-principles synchrotron spectra and light curves, which are in good agreement with X-ray observations: (1) the synchrotron spectrum is nearly flat, F

ν
∝ const; (2) when the pulsar spin axis is nearly aligned with the orbital angular momentum, the light curve displays two peaks, just before and after the pulsar eclipse (pulsar superior conjunction), separated in phase by ∼0.8 rad; (3) the peak flux exceeds the one at the inferior conjunction by a factor of 10.
Properties of Dense Molecular Gas along the Major Axis of M82
Authors: Li Fei , Zhang Zhi-Yu , Wang Junzhi , Gao Feng , Li Shanghuo , Zhou Jing , Sun Yichen , Guo Ziyi , Liu Shu 
Published: July 2022

Abstract
Dense gas is important for galaxy evolution and star formation. Optically thin dense-gas tracers, such as isotopologues of HCN, HCO+, etc., are very helpful in diagnosing the excitation conditions of dense molecular gas. However, previous studies of optically thin dense-gas tracers mostly focused on the average properties of galaxies as a whole, due to limited sensitivity and angular resolution. M82, a nearby prototype starburst galaxy, offers a unique case for spatially resolved studies with single-dish telescopes. With the IRAM 30 m telescope, we observed the J = 1 → 0 transition of H13CN, HC15N, H13CO+, HN13C, H15NC, and SiO J = 2 → 1, HC3N J = 10 → 9, and H2CO J = 2 → 1 toward five positions along the major axis of M82. The intensity ratios of I(HCN)/I(H13CN) and I(HCO+)/I(H13CO+) show a significant spatial variation along the major axis, with lower values in the central region than those on the disk, indicating higher optical depths in the central region. The optical depths of HCO+ lines are found to be systematically higher than those of HCN lines at all positions. Furthermore, we find that the 14N/15N ratios have an increasing gradient from the center to the outer disk.