bluuebunny/crossref_metadata_2025 huggingface dataset:
The Effects of Nested Dynamos in the Gas Giants
Authors: Wulff Paula , Cao Hao , Aurnou Jonathan
Published: July 2024

Gravity measurements of the gas giants, as well as ring seismology in the case of Saturn, have led to increasingly complex structure models for both planets. The latest interior models for Jupiter and Saturn include a dilute, diffuse, or fuzzy core at their centres (e.g., Mankovich & Fuller 2021; Militzer et al. 2022). However, the dynamical nature of this central region and its effects on the dynamo process are not well constrained. Some hypothesise that the deep interior takes the form of a fully stably stratified dilute core while others argue for a convecting (inner) dilute core and a stably stratified transitional envelope atop. Either of these models will act to alter the geometry of the convective dynamo region considerably, especially in combination with likely additional stably stratified layers at mid-depths, due to helium rain.Here we use 3D numerical MHD simulations to explore the effect of a dilute-core dynamo. As a first step, we adopt an imposed axial dipole with varying strength as a proxy for a deep dilute-core dynamo. We investigate its effects on the dynamical flows and magnetic field generation process in the convective metallic hydrogen layer above. In addition, a stably stratified transitional layer between the dilute-core dynamo and the convective metallic hydrogen layer has been implemented in our numerical models. With these numerical simulations, we aim to elucidate 1) which type of structures models leads to Jupiter-like or Saturn-like surface magnetic fields, and 2) if the deep dilute-core dynamo will leave observable imprints in the spatial or temporal pattern of the magnetic field. 
Development of an Antenna Emulator Device for the JuventasRadar Experiment on the HERA Mission
Authors: Laabs Martin , Pfohl Thomas , Plettemeier Dirk , Herique Alain
Published: July 2024

The Juventas Radar (JuRa), a monostatic radar system designed to probe Didymos binarysystem internal structure using a BPSK coded signal. A key component in ensuring the effectiveoperation of the JuRa system is the accurate matching of the dipole antenna impedance to thepower amplifier and receiver. In the transmitting path, the power amplifier performance is sensitiveto the loading impedance. For high efficient power amplifier this is a non-linear effect which ischallenging to model and simulate, especially for modulated signals. Calibration data obtained in astandard 50-ohm environment would be therfore inaccurate.Traditional deployment of antennas in an anechoic chamber for testing is not feasible due to the lowcenter frequency of 60 MHz as coupling with close objects and multiple reflections changeits frequency response. To address this challenge, we developed an antenna emulator device.The antenna emulator device is engineered to present an equivalent antenna-like impedancetowards the transmitter, mimicking the behavior of the actual antennas used in the JuRa systemwhen deployed in space. This device is crucial for testing and calibration because deploying actualantennas is impractical. Thus, the emulator provides a realistic impedance environment, ensuringthat the power amplifier operates under conditions that closely resemble those it will encounter inspace.Additionally, the emulator is equipped with input/output interfaces for monitoring TX signals andsignal injection for RX testing. However, these interfaces exhibit a inadvertently non-flat frequencyresponse, necessitating the development of a mathematical model to correct for these discrepanciesthrough post- and pre-processing techniques. The mathematical model developed for the emulator'sinput/output interfaces involves linear pre-and post-processing techniques, based on combination ofmultiple measurement of the antenna emulator device and instrument.The publication will detail the design process of the antenna emulator, including the theoreticalconsiderations and practical challenges (e.g. strong coupling with the solar panels) addressed duringits development. To facilitate testing during the assembly and integration (AIT) phases, wedeveloped a modified version of the emulator that can be used with non-deployed antennas. Thisversion allows for testing during the AIT without risking damaging the power amplifier by largevoltage standing wave ratio.Finally the principles and techniques developed for the Juventas Radar antenna emulator can beapplied to other missions with low-frequency antennas facing similar testing challenges. Byproviding a practical solution to the problem of testing low-frequency antennas withoutenvironmental interference, our approach offers a valuable tool for future planetary andinterplanetary space missions.
Seismic wave detectability on Venus using ground deformation sensors, infrasound sensors on balloons and airglow imagers
Authors: Garcia Raphael F. , van Zelst Iris , Kawamura Taichi , Näsholm Sven Peter , Horleston Anna , Klaasen Sara , Lefèvre Maxence , Solberg Celine Marie , Smolinski Krystyna T. , Plesa Ana-Catalina , Brissaud Quentin , Maia Julia S. , Stähler Simon C. , Lognonné Philippe , Panning Mark , Gülcher Anna , Ghail Richard , De Toffoli Barbara
Published: July 2024

The relatively unconstrained internal structure of Venus is a missing piece in our understanding of the Solar System formation and evolution. To determine the seismic structure of Venus' interior, the detection of seismic waves generated by venusquakes is crucial, as recently shown by the new seismic and geodetic constraints on Mars' interior obtained by the InSight mission.  In the next decades multiple missions will fly to Venus to explore its tectonic and volcanic activity, but they will not be able to conclusively report on seismicity or detect actual seismic waves. Looking towards the next fleet of Venus missions in the future, various concepts to measure seismic waves have already been explored in the past decades. These detection methods include typical geophysical ground sensors already deployed on Earth, the Moon, and Mars; pressure sensors on balloons; and airglow imagers on orbiters to detect ground motion, the infrasound signals generated by seismic waves, and the corresponding airglow variations in the upper atmosphere.Here, we provide a first comparison between the detection capabilities of these different measurement techniques and recent estimates of Venus' seismic activity.In addition, we discuss the performance requirements and measurement durations required to detect seismic waves with the various detection methods. As such, our study clearly presents the advantages and limitations of the different seismic wave detection techniques and can be used to drive the design of future mission concepts aiming to study the seismicity of Venus.
PISCES: Plumes and Ices Simulation Chamber for Enceladus and icy moonS
Authors: Bourgeois Yael , Cazaux Stephanie
Published: July 2024

Vast subsurface oceans buried under kilometers of ice crust have been discovered in our Solar System's icy moons and have sparked worldwide interests in ascertaining their potential habitability. The tell-tale signs that betray their presence on their hosts are mostly related to density and gravitational field measurements. In the case of Saturn’s moon Enceladus however, the Cassini space probe has observed supersonic plumes of water vapour and ice particles spewing from a fractured area of the South Polar Terrain called the "tiger Stripes", with later analysis of their composition confirming the presence of liquid water below the surface. While the plumes mechanisms are now well-understood as a whole, some areas remain unclear such as the link between icy particles nuclei composition and their origin and evolution from the subsurface ocean. As future missions will renew contact with Enceladus and explore its mysteries in the coming decades, we need experimental studies to best prepare for those. These studies will help with mission planning, instruments choice and tests and making sure we will harvest the best scientific return from the observations made.  In this paper we present a new experimental setup called the Plumes and Ices Simulation Chamber for Enceladus and icy moonS, or PISCES for short. It is designed to emulate the environmental conditions (pressure, temperature) at the surface and interior of icy moons to experimentally study the processes that occur there using a wide range of sensors and instruments. We first describe the vacuum chamber setup and the range of sensors and instruments it can interface with. To showcase the setup's capabilities, we will then proceed to detail some of the plumes experiments we've run. Using 3D-printed cylindrical channels of various shapes and profiles and mounting them atop a liquid water reservoir placed in the vacuum chamber, we can investigate a wide range of plumes and link the plumes behaviour (vent velocity, temperature or particle size) to subsurface characteristics e.g. wall temperature, width, length or expansion ratio. By steadily increasing the complexity of the models used, we aim to experimentally replicate the icy plumes of Enceladus under analogous conditions using the PISCES setup will be a pioneering achievement this new area of research.
Update on ESAs Planetary Defence missions under study and in planning
Authors: Moissl Richard , Conversi Luca , Cano Juan-Luis , Walker Roger , Skrypnyk Ilja , Martino Paolo
Published: July 2024

ESA is currently studying three Planetary Defence related missions in the framework of the Space Safety (S2P) Programme:- NEOMIR (Near Earth Mission in the Infra Red): A space based IR telescope to be stationed at the Earth-Sun Lagrange point (L1), which will be scanning the inner solar system for Asteroids with solar elongations not readily accessible from groundbased observations.- RAMSES (Rapid Apophis Mission for SEcurity and Safety): Rendezvous mission to asteroid (99942)Apophis (based on maximum re-use of components from the Hera spacecraft) with the objective to arrive at the NEO prior to its close encounter with Earth (ECA) on Friday 13th of April 2029 and to perform a full pre-ECA characterisation of the Object. This data will be highly valuable in combination with the data acquired by the NASA OSIRIS-APEx mission post-ECA.- Satis: A lightweight Cubesat (12U-XL baseline) mission which is intended to demonstrate a low-cost asteroid inspection concept for Fast Asteroid Reconnaissance (FAR) of Near Earth Objects with a minimum payload configuration needed for the assessment of basic physical parameters necessary for Planetary Defence purposes. In this presentation we will provide a programmatic update on these three mission studies and present plans for upcoming mission concepts. 
SPH Simulations of Boulder Disruptions: from Laboratory Scale Impacts to Asteroids
Authors: Della Moglie Paolo , Raducan Sabina D. , Jutzi Martin , Ballouz Ronald L. , Cline Christopher J. , Cintala Mark J.
Published: July 2024

The detailed observations of the boulder populations on rubble-pile asteroid surfaces such as Ryugu, Bennu or Dimorphos provide insights into their physical properties and the evolution of their host asteroids [1]. Asteroid surfaces evolve through impacts and thermal processing – both mechanisms that may lead to boulder fragmentation (Figure 1). Figure 1: a) - c) Images acquired by the DART spacecraft approaching the surface of Dimorphos. Boulders which may have originated as a result of an impact event on the asteroid surface are highlighted in red (NASA/Johns Hopkins APL). Here, we present numerical simulations using the Bern SPH code [2] to study the impact fragmentation of boulders on asteroid surfaces. Before applying our models to asteroid scales, we successfully validated them by comparing the results with boulder disruptions observed in laboratory impact experiments [3].In scenarios of impacts on rubble-pile asteroids, our Bern SPH simulations include the displacement and late-stage evolution of the boulder fragments, using a recently developed approach [4,5]. This allows us to determine their final position on the asteroid surface or if they are ejected from the asteroid. Our initial results suggest that only for boulders with a relatively low bulk tensile strength (
Amplitude estimation of the Moon’s spheroidal excitation induced by a gravitational wave
Authors: Majstorović Josipa , Vidal Léon , Lognonné Philippe
Published: July 2024

Gravitational waves from astrophysical sources interact with elastic bodies and their interaction can be presented in terms of the normal mode excitations. In this regards, the GWs are described as forces driving these oscillations. In the community, two theories emerged on how the GW metric perturbation couples with the elastic body. One theory relates to Dyson’s paper (Dyson, 1969), where the GW force is coupled with the elastic body through the gradient of the shear modulus. The second one is related to Weber’s paper (Weber, 1960), where the GW is coupled with the elastic body through a Newtonian tidal forcing.  Here, we present analytical displacement solutions to both of these theories by using the Green tensor formalism, where the induced displacement is calculated as a double integral of the convolution between the impulse response of the elastic body and the GW force term. Eventually, we examine what are the key ingredients to obtain the GW response of the Moon. It has been shown that Moon is extremely seismically quiet with an upper limit on the background noise that is lower than the Earth one by at least 3 orders of magnitude. This is one of the main driving reasons why the Moon is considered as a unique environment for a gravitational astronomy. Therefore, to conduct our study, we introduce several approximations:  firstly, GWs are monochromatic waves defined by a scalar metric value, a polarization tensor and a propagating vector; secondly, we consider non-rotating anelastic Moon; thirdly, the derivation is obtained in the Moon’s reference system.  We study, what are the main differences of the induced responses from the two theories, and what are the levels of the excitation amplitudes for a published lunar model. Next, we also scrutinise how the estimated excitation amplitude depends on the regolith structure by altering the initial lunar model and using different regolith models. We discuss what are the prospect of detecting these signals with future GW detectors build on the Moon. Dyson, F. J. (1969). Seismic response of the earth to a gravitational wave in the 1-Hz band. Astrophysical Journal, vol. 156, p. 529, 156, 529. Weber, J. (1960). Detection and generation of gravitational waves. Physical Review, 117(1), 306.
Molecular Complexity in forming Solar-like Planetary Systems 
Authors: Ceccarelli Cecilia , Bianchi Eleonora
Published: July 2024

Our is the only planet known with such complex chemistry that give rise to life. Numerous evidence suggests that molecular complexity had already begun and developed when the Solar System was an embryo inside a cold molecular cloud. In this presentation, I will present the major advances in our comprehension of chemistry during those ancient eons, based on what we observe in the young solar-like planetary systems forming in the Sun’s vicinity today and our ability to understand them. I will also give an overview of the many challenges that remain to be overcome.
Multi-wavelength phase curves of asteroids
Authors: Alvarez-Candal Alvaro
Published: July 2024

The arrival of extensive multi-wavelength photometric surveys opens a window into exploring aspects of astrophysics in ways that were not possible before. In particular, studying scores of small bodies observed serendipitously at different orbital locations in different epochs allows us to understand the phase-angledependence of their photometric properties while obtaining their absolute magnitudes.In this work, I present recent results showing that the surfaces of small bodies do not follow a unique color trend with phase angle (the so-called "phase reddening") but instead have a dual behavior with a change at a critical angle of about α = 5 deg. On the other hand, the large number of results opens for a critical revision of long-standing relations involving phase coefficients and observables, such as taxa and albedo, which may not hold.The main results of this work can be summarized as follows: (1) Using observations at a single epoch may bias the results, (2) long-used observational relations may not survive the increase in the number of data, and (3) small bodies' reflectance properties do not behave as suspected.
Analysis of Jupiter's atmosphere using Juno's radio occultations
Authors: Smirnova Maria , Galanti Eli , Caruso Andrea , Buccino Dustin , Gomez Casajus Luis Antonio , Gramigna Edoardo , Zannoni Marco , Parisi Marzia , Hubbard Bill , Steffes Paul , Levin Steven , Bolton Scott , Tortora Paolo , Kaspi Yohai
Published: July 2024

The shallow layers of the Jovian atmosphere, the only regions accessible to direct investigation through in situ sampling and remote sensing experiments, are the looking glass through which the unknowns of Jupiter's structure are revealed. Radio occultation experiments have proved to offer invaluable opportunities to investigate the atmospheric dynamics of Jupiter, akin to descending a probe into its upper layers, offering unique insights into the thermal structure and composition.
Since July 2023, Juno's extended mission has presented a multitude of such opportunities, with each passing month bringing forth a new experiment, a first since the Voyager missions. In these experiments, as the Juno spacecraft orbits Jupiter, it is obscured by the planet along its trajectory. As the electromagnetic signal from the spacecraft travels towards Earth, it traverses through Jupiter's atmosphere, resulting in refraction on the signal. This refraction is recorded on the ground station as a frequency shift, known as the Doppler shift, compared to its expected frequency in a vacuum environment. Radio occultation experiments capitalize on these refraction effects to investigate and decipher the atmospheric vertical properties of the planetary atmosphere up to 0.5 bar.
The Juno radio occultations of Jupiter operated in a coherent two-way mode, utilizing multi-frequency link signals. Consequently, this study necessitated the use of an optimization method employing ray tracing techniques to track both the uplink and downlink signal through the neutral atmosphere in X- and Ka-band, enabling the extraction of vertical profiles of atmospheric parameters. The analyzed atmospheric pressure-temperature profiles highlight the potential of Juno's radio occultation experiments in elucidating the relatively unknown neutral atmosphere of Jupiter. In this presentation we present initial results from Juno's first year of radio occultations, analyse the measurement sensitivity concerning density and temperature, investigate the vertical temperature profiles at different latitudes and discuss their implications regarding the dynamics of Jupiter.
Investigating Uranus' formation through the D/H ratio
Authors: Benest Couzinou Tom , Mousis Olivier
Published: July 2024

The formation mechanisms of the ice giants Uranus and Neptune, as well as the origin of their elemental and isotopic compositions, have been long-standing subjects of debate. Several puzzling observations have challenged our understanding of these planets' formation processes. Spectroscopic observations have revealed that both Uranus and Neptune are highly enriched in carbon and perhaps deficient in nitrogen, an elemental composition that deviates from predictions based on our current understanding of planet formation. Also, the ices from which Uranus and Neptune originally formed might have had deuterium-to-hydrogen (D/H) ratios lower than the predicted cometary value, a characteristic that has not been envisaged in any other planets in our solar system.Resolving these puzzles is crucial for advancing our understanding of the formation mechanisms and evolutionary processes that shaped these enigmatic ice giants. One key piece of observational data that can shed light on this mystery is the measurement of the D/H ratio in Uranus, provided by the Herschel space telescope. This measurement is vital for understanding the current planetary composition of Uranus.The aim of this study is to investigate whether the CO/H2O ratio of Uranus, inferred from the D/H measurement, is consistent with the composition in the protosolar nebula during its evolution. To achieve this, the following approach has been employed:Interior Models. Using interior models and assuming a cometary D/H value in the primitive ices of Uranus, the contemporary D/H measurement from Herschel can be related to the bulk CO/H2O ratio of Uranus.
Protoplanetary Disk Evolution Model. A protoplanetary disk evolution model that includes solid and gaseous phases, as well as clathrates, has been utilized to simulate the evolution of the CO/H2O ratio in the protosolar nebula over time.
Comparison of Ratios. The preliminary results compare the inferred CO/H2O ratio of Uranus with the local CO/H2O ratio in the protosolar nebula at different epochs, providing insights into the local conditions present during the formation of Uranus.
By combining observational data, interior models, and protoplanetary disk simulations, this study aims to shed light on the connection between the composition of Uranus and the conditions in the PSN during the planet's formation process.
DIPSY: A New Disc Instability Population Synthesis
Authors: Schib Oliver , Mordasini Christoph , Helled Ravit , Emsenhuber Alexandre
Published: July 2024

Disc instability remains the leading formation pathway for some of the observed giant planets. In particular, this model can more naturally explain giant planets at large separation, giant planets around M stars, and very young giant planets. However, there are still many open questions regarding this formation mechanism, and the expected population of planets is currently unknown.We present the results of a new disc instability population synthesis (DIPSY) that addresses many of these questions and makes predictions about the expected population of planets that can be tested observationally.Our model describes the formation of a star-and-disc system and its evolution until the disappearance of the disc and beyond. It includes a large number of physical effects: gravitational interaction between forming companions, self-consistent gas-accretion, migration and many more.We find that, while fragmentation (the formation of bound clumps of gas in the disc, a necessary condition for planet formation in the disc instability model) may only happen in a minority of systems, it typically leads to the formation of at least one companion when it does.The inferred population of companions spans a large range of masses, from the planetary to the stellar regime.We present and discuss this population, as well as the influence of a number of assumptions.The figure shows the result of the baseline run: the mass-distance diagram for 100’000 systems after 100 Myr. The final host star mass is given as colour code.The results of the population synthesis will provide hints both for the theoretical study of planet formation (e.g. hydrodynamic simulations) and future observational surveys of companions.DIPSY contributes to our understanding of planet formation irrespective of the formation model.
Venus as an Exoplanet: Effect of varying stellar, orbital, planetary andatmospheric properties upon composition, habitability and detectability
Authors: Grenfell John Lee , Helbert Joern , Arnold Gabriele , Herbst Konstantin , Sinnhuber Miriam , Rauer Heike
Published: July 2024

The newly selected Venus missions EnVISION and VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy) offer new opportunities for studying Venus but will also contribute to furthering our knowledge of Venus as an exoplanet. Hot rocky planets are favored targets due to generally more frequent transits than cooler Earth-like objects. In this work we simulate Venus as an exoplanet varying stellar, orbital, planetary and atmospheric parameters and study the effect upon atmospheric composition, climate and spectral detectability.
Observations of negatively-charged particle populations near Enceladus and its plume
Authors: Jones Geraint , Coates Andrew
Published: July 2024

We provide an overview of observations near Enceladus obtained by the Cassini Plasma Spectrometer's Electron Spectrometer, CAPS-ELS (Young et al. 2004). The instrument was designed to observe electrons between 0.6 eV/e and 28.8 keV/e in energy per charge, though, as we report here, other negatively-charged particles are also detectable by the instrument. A major hindrance to the comparison of particle data between Cassini’s Enceladus encounters has been the differing flyby geometries, speeds, and instrument pointing parameters. To help remove some of these complicating factors, we present the encounters grouped according to encounter geometry. We take stock of the CAPS-ELS data obtained near Enceladus, with reference to earlier studies by ourselves and others of nanograins, negative ions, and magnetic field-aligned electron beams. We also highlight features not yet published, some of which are only revealed when data from the 14 encounters are analysed collectively. These include electron dropouts and spikes in and near the plume, the effects on the spacecraft and plume material when in the optical shadow of Enceladus, and curious electron pulsations. 
Imprensa, Revolução do Porto e os ecos políticos no Rio de Janeiro (1820-1821)
Authors: Meirelles Juliana
Published: July 2024

This article discusses the implications of the 1820 Porto Revolution in the Luso-Brazilian press of the period amid the crisis of the Portuguese Ancien Regime. Within the perspective of the Social History of Written Culture, with a particular focus on the circulation of ideas on both sides of the Atlantic, we address how the news of this political event were apprehended by the joanine society living in Rio de Janeiro and its developments for the transformation of the press order in the city in the year 1821.
Sobre as dinâmicas de cooperação e/ou competição na Eurorregião Galiza-Norte de Portugal
Authors: Cancela Outeda Celso , González Cacheda Bruno
Published: July 2024

At present, relations between Galicia and Portugal seem to be characterised by a certain paradox. On the one hand, since the 1990s, the EU has promoted territorial cooperation through financial contributions (INTERREG) for the implementation of joint projects. Later, it provided a legal-institutional framework through the regulation of European Groupings of Territorial Cooperation (EGTC). This cooperation, especially crossborder cooperation, is conceived as a useful tool for improving the competitiveness of certain local and regional areas (barrier effect) and for bringing citizens closer together. At the same time, in the context of globalisation and the internationalisation of markets, states are practising a “best place policy”. They try to create the most suitable conditions within their borders for attracting investment and capital appreciation. In this way, competitive dynamics are generated between territories. This article aim to carry out an analysis of the dynamics of competition and cooperation that can be detected in the Galicia-North Portugal Euroregion. To this end, we will analyse the discourse of the main actors and agents involved in the productive processes in the Euroregion: politicians, business leaders and trade unions.
Aplikasi Perawatan Kesehatan Yang Digunakan Untuk Perawatan Total Di Rumah: Tinjauan Pustaka
Authors: Tyas Prastyanto F X Bobby
Published: July 2024

Aplikasi perawatan kesehatan yang dapat digunakan untuk perawatan total di rumah telah menjadi topik yang semakin relevan dan mendesak. Peningkatan jumlah pasien yang memilih perawatan di rumah mereka sendiri menuntut solusi teknologi inovatif yang dapat meningkatkan kualitas layanan dan pengalaman pasien. Oleh karena itu, latar belakang penelitian ini bertujuan untuk menyajikan tinjauan literatur yang komprehensif mengenai aplikasi perawatan kesehatan yang telah diterapkan atau dikembangkan untuk mendukung perawatan total di rumah. Metode penelitian menggunakan literature review. Penulis menggunakan beberapa database, yaitu, ProQuest, Sage Journals, JSTOR, Clinicalkey Nursing. Kriteria inklusi, meliputi artikel yang membahas tentang pene-rapan “health care application”, “total care Application”, “health care appli-cation AND total care at home”. Hasil pencarian menghasilkan ± 218 artikel. Artikel yang didiskusikan, yaitu penerapan aplikasi layanan kesehatan berbasis smartphone pada pasien yang membutuhkan total care. Hasil literature review dari beberapa jurnal memberikan informasi terkait keterlibatan berbagai sektor dalam pengembangan teknologi dan harapan pada aspek privasi, sehingga dapat mengembangkan program yang efektif dan memberikan layanan yang tepat pada pasien yang menjalani perawatan total care
Analisis Kepuasan Pelayanan Kesehatan Pasien Infeksi Saluran Pernafasan Akut Anak Balita Di Poli KIA Puskesmas Tahun 2024
Authors: Kurniati Kurniati , Chairil Zaman  , Arie Wahyudi
Published: July 2024

Latar belakang infeksi saluran pernafasan akut menyumbang hampir 15% dari seluruh kematian anak  di Asia dan anak-anak yang ada di pedesaan mempunyai risiko lebih tinggi karena tidak dapat diaksesnya fasilitas kesehatan. Kasus ISPA yang terjadi pada anak-anak akan menimbulkan gambaran klinis yang lebih parah dibandingkan pada orang dewasa.  Metode penelitian dengan desain penelitian kuantitatif dengan pendekatan crossectional.  Populasi penelitian ini adalah oran tua anak balita tahun 2024. Sampel dalam penelitian ini berjumlah 90 orang. Cara pengambilan sampel menggunakan purposive sampling. Penelitian ini telah di laksanakan pada tanggal  7 sampai dengan 29 februari 2024. Pengumpulan data dengan menggunakan kuisioner. Analisis data bivariat menggunakan uji chi-square dan multivariate regresi logistik. Hasil penelitian menunjukan ada hubungan tangible  (pValue = 0,002) , reliability (pValue = 0,039) responsiveness (pValue = 0,00)  dan  assurance (pValue = 0,007) terhadap kepuasan pasien infeksi saluran pernafasan akut anak balita tahun 2024.  Tidak ada hubungan umur (pValue 0,37), pendidikan (pValue 0,57) dan pengetahuan (pValue 0,10) terhadap kepuasan pasien infeksi saluran pernafasan akut anak balita tahun 2024. Faktor yang paling dominan yang berhubungan dengan kepuasan pasien infeksi saluran pernafasan akut anak balita tahun 2024, yaitu responsiveness (pValue = 0,000), (OR = 0,28). Kesimpulan  ada hubungan tangible, reliability,  responsiveness dan  assurance terhadap kepuasan pasien infeksi saluran pernafasan akut anak balita tahun 2024.
Pengetahuan Ibu Dan Dukungan Keluarga Terhadap Pemberian Asi Ekslusif Pada Bayi
Authors: Siska Delvia  , Muhammad Hasan Azhari
Published: July 2024

ASI Ekslusif merupakan pemberian ASI kepada bayi tanpa makanan dan minuman pendamping (termasuk air jeruk, madu, air gula). Tindakan tersebut dapat dimulai sejak bayi baru lahir sampai dengan usia 6 bulan. Asi merupakan sumber gizi yang sangat ideal dengan komposisi yang seimbang dan di sesuaikan dengan kebutuhan pertumbuhan bayi. Asi adalah makanan yang sempurna baik secara kualiatas maupun kuantitasnya dengan tatalaksana menyusui yang benar Hipotesis dalam penelitian ini ada hubungan antara pengetahuan ibu dan dukungan keluarga terhadap pemberian Asi. Jenis penelitian yang digunakan adalah survey Analitik dengan pendekatan Cross Sectional dengan menggunakan uji Chi Square dikatakan terdapat hubungan jika p value <0,05 dengan Variabel penelitian yaitu variable Independen (pengetahuan ibu dan dukungan keluarga) dan Variabel Dependen (Pemberian Asi Ekslusif) dimana data yang dikumpulkan dalam waktu bersamaan. Pengambilan sampel pada penelitian ini dilakukan dengan metode total sampling dengan sampel dalam penelitian ini adalah 80 orang yang di ambil dari data kunjungan posyandu balita usia >6-24 bulan diPMB Ririn Sevda Korini SKM., S.keb dari bulan Januari 2022 sampai Juni 2023. Tempat Penelitian dilaksanakan di PMB Ririn Sevda Korini SKM.,S.keb Kabupaten Ogan Komering Ulu. Waktu pengumpulan data dalam penelitian ini pada Bulan Agustus - Oktober2023. Hasil penelitian ini didapatkan nilai p-value = 0,000 antara pengetahuan ibu dan dukungan keluarga dengan pemberian Asi eksklusif. Kesimpulannya terdapat hubungan yang signifikan antara pengetahuan dan dukungan keluarga dengan pemberian Asi eksklusif.
Implementation of E-Health Based Technology to Improve the Health Status of the Elderly: A Literature Review
Authors: Filipus Y. Boibalan  , Sukihananto
Published: July 2024

The number of elderly from year to year continues to increase, this has a significant impact on health services. The significant addition of the elderly and the worsening of the situation including decreased health, altered emotional status, inability to do activities independently make some people consider the elderly a burden. Objective: Providing ideas and ideas from the results of literature review on the implementation of E-health-based technology to improve the health status of the elderly, using smartphones to measure elderly activities, security and safety of the elderly. The method used in this research is literature review with keywords namely "technology", "elderly", and "degree of health". Searching for academic journals through Online Databases including: Science Direct, Google Scholar, ProQuest and clinical key from 2015-2022. The results of the review of 10 journals that discuss the technology of monitoring the elderly remotely via smartphones can be concluded if the development of technology to monitor the development of the elderly remotely is very satisfying because it can help caregivers and health workers in monitoring activities, the state of the elderly, and minimizing adverse events. It is hoped that future researchers can examine the ability of users to apply technology and user preparedness and costs in using this technology.
Aplikasi Taklid dan Talfîq dalam Implementasi Hukum Keluarga di Indonesia
Authors: Dzurriyyatus Sa'adah Isqi , Saepullah Usep
Published: July 2024

Tulisan bertujuan memaparkan bagaimana konsepsi ijthad dalam kurun waktu yang berkelanjutkan dimulai dari periode Imam Mujtahid sampai dengan ulama kontemporer dan terkodifikasi menjadi hukum Nasional mampu mempengaruhi setiap aspek hukum yang berkaitan langsung baik dalam segi ibadah ataupun muamalat. Kompilasi Hukum Islam dalam hal ini memiliki pertalian erat sebagai sebuah aktualisasi hukum taklid dan talfîq dalam sistem hukum keluarga Islam yang lebih konkret. Hasil penelitian menunjukan bahwa keadaan zaman yang terus mengalami perkembangan seolah memaksa hukum fikih untuk terus berjalan elastis beriringan dan realistis untuk dipergunakan semua elemen masyarakat. Polemik yang muncul berkaitan dengan keberadaan taklid dan talfîq tidak serta merta dapat dipisahkan berkenaan hukum menyangkut banyak aspek melahirkan dikotomi antara fikih klasik dan modern yang tidak bisa dielakan menyangkut kemampuan penalaran dalam menafsirkan suatu permasalahan dengan menggali hukum syariat yang sama-sama mengejar pada satu tujuan kemaslahatan yang secara aplikatif tertuang dalam setiap butir KHI sebagai pedoman bagi terlaksananya hukum keluarga di Indonesia baik secara personal ataupun rujukan di Pengadilan Agama.
Efektifitas Lotion Anti Nyamuk Ekstrak Etanol Daun Kenikir (Cosmos caudatus)
Authors: Suprianto  , Hendri Faisal  , Endang Subekti
Published: July 2024

Mosquitoes are one of those insects with an often annoying presence. Saponins, polyphenols, and essential oils are found in the Kenikir plant (Cosmos caudatus). Experimental research was conducted with tests covering: organoleptic, homogeneity, pH, and effectiveness. Organoleptic lotions at concentrations of 5%, 10% and 15% have a dark green colour with a distinctive odour of Kenikir. Lotions with a concentration of 5% are homogeneous, while at concentrations of 10% and 15% are not homogeneous. Organolepticrequirements and homogeneity as lotions are met. The results obtained showed that the Kenikir leaf extract was effective at repelling mosquitoes.
Potential Antioxidant Activity of Dry and Fresh Ethanol Extract of Mahkota Dewa Leaves (Phaleria macrocarpa)
Authors: Herlina  , Lasmaryna Sirumapea  , Hilma  , Yulia Azelya Salsabela
Published: July 2024

Senyawa yang berfungsi sebagai penangkal radikal bebas dikenal sebagai antioksidan, yang menghambat proses oksidasi reaksi kimia dan bekerja dengan cara mengambil sebuah elektron pada suatu molekul sehingga dapat mengurangi pengaruh negatif akibat adanya radikal bebas tersebut. Tanaman mahkota dewa (Phaleria macrocarpa) dari famili Thymelacaccae diketahui memiliki potensi sebagai antioksidan alami. Pengaruh perbedaan perlakuan sebelum proses ekstraksi daun mahkota dewa terhadap nilai aktivitas antioksidan telah diamati. Sebagian daun dikeringkan dengan cara kering-angin dan sebagian lagi diekstraksi dari daun segar, sebelum kedua kelompok daun tersebut diekstraksi secara maserasi. Ditentukan persentasi rendemen, uji fitokimia dan hasil pengujian antioksidan menggunakan DPPH (1,1-difenil2-pikrihidrakzil) dan asam galat sebagai pembanding. Hasil pengujian menunjukan, nilai rendemen adalah sebesar 13,6 % b/b (ekstrak hasil pengeringan) dan 9% b/b (daun segar). Senyawa metabolit sekunder aktif yang terdapat pada daun mahkota dewa adalah alkaloid, fenolik dan flavonoid. Nilai aktivitas antioksidan (IC50) didapatkan sebesar 108,05 ppm (daun kering); 90,97 ppm (daun segar) dan 4,04 ppm (senyawa pembanding). Ekstrak sampel daun mahkota dewa segar memiliki nilai aktivitas antioksidan yang lebih baik dibanding ekstrak sampel daun mahkota dewa kering.
Anti-Inflammatory Potential of Ethanol Extract of Sawo Kecik Leaves (Manilkara kauki L.)
Authors: Aminah Syarifuddin  , Debi Dinha Octora  , Cucu Arum Dwi Cahya
Published: July 2024

Background: Inflammation often occurs in the community in the joints, its prevalence in the world is around 11.9 million. The prevalence in high-income countries is around 1.3 million, while in low-income countries it reaches 5.9 million, Southeast Asia has 4.4 million. Objective: The study was directed to test the anti-inflation effect of EDSK. Method: The method causes oedema of the soles of the test animals through carrageenan induction. The EDSK test as an anti-inflammatory was used by 25 animals distributed in 5 groups; one positive and one negative control, and 3 treatments each of SND, CMC, SEDSK1, SEDSK2, SEDSK3. Results: The percentage of inflammation in the five groups decreased continuously starting from the first hour to the 6th hour after carrageenan induction. The largest percentage of inflammation occurred at the 2nd hour in CMC, followed by SEDSK1, SEDSK2, SEDSK3 and SND. The greatest percent inhibition was SND, followed by SEDSK3, SEDSK2, and SEDSK1. The best inhibition was on SEDSK3 after SND, followed by SEDSK2, and SEDSK1.Conclusion: Research provides information that the SEDSK1, SEDSK2, and SEDSK3 groups have potential anti-inflammatory agents.
Reflexões sobre o Serviço Social Brasileiro e a Decolonialidade: Uma Pesquisa Bibliográfica
Authors: Fernandes Nidia Gizelli de Oliveira , Silveira Carlos Roberto da , Mascia Marcia Aparecida Amador
Published: July 2024

Este trabalho objetivou refletir sobre as relações entre o Serviço Social brasileiro e a decolonialidade. A pesquisabibliográfica foi a metodologia adotada e realizada a partir de buscas no Scielo, Google Acadêmico e Periódicos Capes. Verificou-se que o debate decolonial é incipiente no Serviço Social, que ele não compõe a formação profissional. Noentanto, há um movimento inicial em direção à abordagem decolonial, conforme indicado pelos estudos levantados, especialmente na análise da Questão Colonial e da Questão Social. Estes aspectos ressaltam a urgência de realizarinvestigações mais detalhadas sobre esses temas, visando contribuir para um novo paradigma profissional.
Perancangan Sistem Informasi Ticketing Jaringan Pada Dinas Komunikasi, Informatika dan Statistik Provinsi DKI Jakarta
Authors: Sururi Dede Miftah , Susanti Melan
Published: July 2024

The rapid development of technology affects all aspects of life, especially information systems. With the development of this technology, speed and accuracy are needed to send information so that it can be received by the recipient. For the process of sending data, a communication network is needed as a means of transportation. In the process, it doesn't always go well; sometimes network interference problems occur. To overcome this problem, a system is needed that can record network disturbances so that problems can be resolved and analyzed immediately. The process of recording network disturbances at the DKI Jakarta Province Communication, Informatics, and Statistics Office is currently still using conventional or manual methods, which often creates problems. So it is necessary to have a system that can record these disturbances. The design of this system is made to make it easier for companies to record network disturbances and facilitate analysis if there are repeated disturbances. By using the waterfall method, existing problems can be examined so that the designed system can perform as expected. So that this system makes it easier for network managers to document reported network disturbance data, which results in not requiring a long time to search for or collect manual records. Therefore, this system will make the work system more effective and efficient in terms of time, effort, and cost.Keywords : network, ticketing, waterfall
ЭТИОЛОГИЧЕСКИЕ АСПЕКТЫ КАРИЕСА ЗУБОВ И ВЛИЯНИЕ ФТОРИДОВ НА ИХ ЗАБОЛЕВАЕМОСТЬ
Authors: Акунов Нурсултан
Published: July 2024

Кариес зубов издавна известное заболевание человечеству, и по сей день продолжает оставаться серьезной проблемой в современном обществе, где значительная часть населения страдает от него. Согласно отчетам некоторых исследователей, наблюдается увеличение заболеваемости кариесом зубов в различных возрастных группах. Эта тенденция прослеживается преимущественно в городских районах и в условиях сложного климата и географии, где уровень распространения кариеса среди определенных групп населения достигает 98,2%. Высокая частота кариеса, особенно среди детей, в значительной мере связана с нарушением баланса между внутренними и внешними факторами. Особое внимание уделяется неправильному питанию, социально-бытовым аспектам, а также недостаточному содержанию микроэлементов и минеральных солей как в питьевой воде, так и в общем рационе питания. Целью исследования является изучение этиологии кариеса и влияние фторидов на заболеваемость.
THE REPRESENTATION OF HISTORICAL TRAUMA IN THE EDUCATIONAL DISCOURSE OF HIGHER EDUCATION: A SOCIO-PHILOSOPHICAL ANALYSIS
Authors: Naumov Dmitry , Savitsky Konstantin , Desjukevich Igor
Published: July 2024

The paper examines the problems of constructing and representing historical trauma in the educational discourse of the Belarusian higher school in the context of constructing a historical picture of national statehood. The theoretical and methodological basis of this study is the theory of historical trauma, which allows us to identify the specifics of the formation of historical consciousness and civil and political identity of students. The study revealed that the representation of trauma in educational discourse not only provides legitimization of modern Belarusian political institutions and the political system as a whole, but also sets a teleological focus for consideration and evaluation of political genesis.
СӨӨК КОЮУ САЛТЫ (ФЕРГАНА ӨРӨӨНҮНҮН ТҮШТҮК-БАТЫШЫНДАГЫ КЫРГЫЗДАРДЫН МИСАЛЫНДА)
Authors: Сапиева Нурия
Published: July 2024

Бул макалада Фергана өрөөнүнүн түштүк батышындагы кыргыздардын сөөк коюу салтынын пайдалануу чөйрөсү жөнүндө жазылды. Автор кыргыздардын сөөк көюу салтындагы жөрөлгөлөр жай турмуштагы жашоодо зор маани-маңызга ээ экендигин аныктаганга аракет жасады. Сөөк коюу жана эскерүү ырым-жырымдары кыргыздардын салттуу маданиятынын жана диний ишенимдеринин маанилүү бөлүгү болуп саналат. Көптөгөн диндик жаңыланууга карабастан сөөк коюудагы анимисттик ишенимдер руханий чөйрөдө өзүнүн маанисин сактап калууда. Ошондуктан, сөөк коюу салты этникалык маданиятын изилдөөдө актуалдуу тема бойдон калат. Сөөк коюу салтындагы ырым-жырымдар кыргыздардын жашоо турмушунда байыртадан келе жаткан бирден бир маанилүү салт экендиги бизге белгилүү болду. Методдор: Сөөк коюу салтын изилдөө учурунда негизинен теориялык жана эмпирикалык изилдөө методдору колдонулду. Жыйынтык: Кыргыздардын сөөк коюу салтындагы ырым жырымдардын пайдалалануу чөйрөсү аркылуу алардын этномаданиятындагы өзгөчөлүктөр аныкталды.
АКТУАЛЬНЫЕ ПРОБЛЕМЫ ИСПОЛЬЗОВАНИЯ НЕЙРОСЕТЕЙ В ОБУЧЕНИИ СТУДЕНТОВ ДИСЦИПЛИНАМ «РУССКИЙ И АНГЛИЙСКИЙ ЯЗЫКИ» (НА ПРИМЕРЕ ТЕХНОЛОГИИ TEXTTOSPEACH.RU)
Authors: Кочконбаева Сонаим , Cадыкова Айгуль , Дуйшоева Бактыгул
Published: July 2024

Развитие цифровых технологий дает новый импульс для проведения педагогических исследований, в том числе связанных теорией и методикой преподавания русского и иностранных языков. В статье проанализированы возможности технологии texttospeeach.ru и особенности использования в педагогических целях инструмент D-ID. Делается вывод о расширении возможностей мультимедиа посредством искусственного интеллекта.
МОНИТОРИНГ УПОТРЕБЛЕНИЯ ОВЦАМИ СОЛОНОВАТОЙ ВОДЫ ОЗЕРА В СЕВЕРО-ЗАПАДНОМ ПРИИССЫККУЛЬЕ
Authors: Турдубаева Айнура
Published: July 2024

Цель исследования – мониторинг употребления овцами солоноватой воды озера в Северо-Западном Прииссыккулье. Исследования были проведены в Тамчынском айылном аймаке Иссык-Кульского района Иссык-Кульской области Кыргызской Республики. Объектами исследования были фермерские и личные хозяйства айылного аймака. Методом исследования было выборочный опрос (методом случайного отбора) владельцев животных. Результаты проведенного выборочного опроса, методом случайного отбора владельцев животных в Северо-Западном регионе Прииссыккулья показали, что: в Северо-Западном регионе Прииссыккулье выделяются приозёрный и предгорно-горный экотопы; абсолютное большинство сельскохозяйственных животных приозёрного экотопа употребляют для питья солоноватую воду озера Иссык-Куль.
ВЛИЯНИЕ ГЕНОТИПА ВАЛУШКОВ НА ПОТРЕБЛЕНИЕ КОРМОВ, ПИТАТЕЛЬНЫХ ВЕЩЕСТВ, ЭНЕРГИИ И ДИНАМИКУ ЖИВОЙ МАССЫ
Authors: Косилов Владимир , Старцева Наталья , Рахимжанова Ильмира , Губайдуллин Наиль , Газеев Игорь , Галиева Зульфия
Published: July 2024

В статье приводятся результаты изучения влияния генотипа валушков романовской породы (I гр.) и её помесей с эдильбаевской породой первого поколения (½ эдильбай × ½ романовская – II гр.) и второго поколения (¾ эдильбай × ¼ романовская – III гр.) на потребление питательных веществ, энергии кормов рациона и изменение живой массы в возрастном аспекте. Установлено, что валушки I гр. уступали помесным сверстникам II и III групп по потреблению кормовых единиц соответственно на 80,52 кг и 93,55 кг, ЭКЕ – на 86,34 и 89,90, переваримого протеина – на 8,14 кг и 9,50 кг, сухого вещества – на 96,62 кг и 101,13 кг. Генотипические особенности и неодинаковое потребление питательных веществ и энергии кормов рациона обусловили межгрупповые различия по живой массе во все возрастные периоды. В конце выращивания в 10-месячном возрасте помесные валушки II и III гр. превосходили чистопородных сверстников I гр. по живой массе на 11,66 кг (31,31 %) и 13,69 кг (36,76 %). При этом валушки II гр. уступали помесям III гр. по массе тела в 10 мес. на 2,03 кг (4,15 %).
ВОЗДЕЙСТВИЕ ПРЕПАРАТОВ СЕЛЕНА НА МОЛОЧНУЮ ПРОДУКТИВНОСТЬ КОРОВ
Authors: Мустафин Рамис , Мустафина Александра , Миронова Ирина , Хабибуллин Ильмир , Хабибуллин Рузель
Published: July 2024

В работе доказана актуальность поставленной темы, изучена молочная продуктивность лактирующих коров. Авторы приводят краткую характеристику методики зоотехнического опыта. Дана характеристика продуктивности подопытных коров в различные периоды лактации в результате действия изучаемых препаратов Е-селен и Бутофан, применяемых в хозяйстве. Сделаны обоснованные выводы.