bluuebunny/crossref_metadata_2025_split huggingface dataset:
The Effect of the Combination Stimulation Cutaneous and Virgin Coconut Oil on the Sleep Quality and Comfort level in People Undergoing Hemodialysis
Authors: Daryaswanti Putu Intan , Asnar Elyana , Krisnana Ilya 
Published: August 2022

Introduction: Sleep quality can be disruptive in patients with chronic illness, especially in patients with Chronic Renal Failure (CRF). In recent times, CRF was associated with poor sleep quality, about 25-36% of the normal adult population had sleep disorders. However, the prevalence of sleep disturbance in patients with uremia undergoing of hemodialysis occurs about 40-85% higher than the general population. It was reported that the majority of cases of chronic renal failure are people who lack sleep. Sleep disorders are very common in patients with chronic kidney disease. Poor sleep in hemodialysis patients has a negative impact on the physical and mental components of a person's life and leads to a decrease in their performance as well as cognitive and memory dysfunction.
Methods: A queasy-experiment with pretest-posttest control group design. The sampling method is used simple random sampling, conducted between January-February 2018. A total of 52 patients undergoing hemodialysis divided randomly into two groups. The treatment group was given cutaneous stimulation and VCO for 4 weeks and the control group was not given cutaneous stimulation and VCO.
Results: Giving cutaneous stimulation and VCO effective in improving sleep quality and comfort level. There were significant results on sleep quality seen from Mann Whitney test with p <.001 and comfort level from Mann Whitney test with p = 0.009.
Conclusion: Provision of cutaneous stimulation and VCO can be used as complementary therapy in improving quality of sleep and comfort in patients undergoing hemodialysis.
Family Experience Dealing with Relapse in People with Mental Disorders
Authors: Muryani Ni Made Sri , Putra I Gede Yudiana , Artawan I Kadek 
Published: August 2022

Introduction: Recurrence is a problem that often occurs in patients with mental disorders. Families who have family members with mental disorders, said that relapse can be caused by not taking medication regularly and when they relapse the family is afraid to face the patient, because the patient is angry and throw things. This study aims to explore in depth the meaning of family experience dealing with relapse in people with mental disorders.
Methods: This study uses a qualitative research design with an interpretative phenomenological approach. This study used purposive sampling, with total 15 participants with inclusion criteria: families who have family members with mental disorders who have experienced a relapse in the last six months and are willing to become participants by signing the participant's informed consent form. Exclusion criteria were families with family members with mental disorders who also had other illnesses. The data collection strategy used in-depth interview techniques with semi-structured interview guidelines. Researchers conducted data analysis using Interpretative Phenomenological Analysis (IPA).
Results: There are four themes in this study, namely (1) Always pay attention to prevent recurrence, (2) Families are able to recognize signs of relapse in family members with mental disorders, (3) Families use medical health services when a relapse occurs, (4) Feel emotional and fearful when the patient relapses.
Conclusion: The results of this study indicate that families feel emotional and fear when the patient experiences a relapse, and the family also knows about the signs of relapse in patients with mental disorders.
Telenursing in Health Services in the Era of the COVID-19 Pandemic: Literature Review
Authors: Mahardika I Made Rai , Wahyuningsih Luh Gde Nita Sri , Lestarini Putu Ayu 
Published: August 2022

Introduction: The development of telenursing is very rapid in various countries. The practice of telenursing supports nurses in providing care to patients without requiring nurses to meet directly with patients so as to reduce the spread of COVID-19 from nurses to patients, or vice versa. Telenursing is an alternative in providing health and long-distance services during the COVID-19 pandemic era. This literature review aims to determine the benefits of telenursing in health services in the COVID-19 pandemic era.
Methods: The method used is a literature study analyzed from several journals. related to the topic taken. Journals were searched through ProQuest, EBSCO and google scholar with keywords telenursing, COVID-19 and health services.
Results: The results of 11 articles show the benefits of telenursing in health services, including preventing the transmission of COVID-19 infection, media and health counseling, analysis costs and sustainable health services.
Conclusion: Telenursing is one of the answers in overcoming the changes that occur to meet the needs of health access in the community. The application of telenursing during the COVID-19 pandemic provides various benefits for both patients and health workers. Telenursing has positive implications in preventing the transmission of COVID-19, as a medium for counseling and health promotion, minimizing medical costs and as a continuity of care.
Nanocurcumin Innovation as an Anti-Apoptosis of Ovarian Granulosa Cells in White Rats Exposed to Lead Acetate (PbAc)
Authors: Syarifah Anis Satus 
Published: August 2022

Introduction: Exposure to Pb causes increased apoptosis of ovarian granulosa cells through oxidative stress mechanism. Curcumin has protective effects on reproductive organs, anti-apoptotic, antioxidant in normal cells. Curcumin in innovated nano form can function as an effective anti-apoptosis in ovarian granulosa cells of rats due to PbAc exposure.
Methods: Thirty female rats were divided into 3 groups, the negative control group (the rats receiving distilled water, in each 90 minutes receiving corn oil), positive control group (the rats receiving PbAc of 30 mg/kg BW, in each 90 minutes receiving corn oil), the experimental group, in which the rats receiving PbAc of 30 mg/kg BW, and in each 90 minutes receiving nanocurcumin of 200 mg/kg BW. All groups received treatment orally once a day for 30 days. On day 31 the rats to granulosa cell apoptosis examination using Tunnel method.
Results: Rate of apoptosis was in the positive control group (5.4 ± 0.8%/micro) and the lowest was in the experimental group (1.1 ± 0.5%/micro) and the negative control group (1.2 ± 0.6). The experimental group showed the same p value as the negative control group (p = .095) and different p value (p = .010) from the positive control group. These findings indicated that the innovation of curcumin in nano form at a dose of 200 mg/KgBW reduced apoptosis of rat ovarian granulosa cells due to PbAc exposure.
Conclusion: The innovation of curcumin in nano form has the potential as an effective natural anti-apoptosis in rats ovarian granulosa cells exposed to PbAc.
Personal Hygiene Skills are Not Related to Infections in School-Age Children
Authors: Yusiana Maria Anita , Kurniajati Sandy , Kristanti Erva Elli , Sari Dyah Ayu Kartika Wulan 
Published: August 2022

Introduction: The incidence of infection in school-age children can be caused by the negligence of children in carrying out personal hygiene, namely washing hands and due to contact with individuals who have been infected with pathogens. Infectious diseases that often suffer are upper respiratory infection, diarrhea, and intestinal worms with symptoms of fever. Preventive efforts that can be done by children are personal hygiene (washing hands). Prevention of infection in children is done by teaching school-age children to wash their hands properly. The objective of this study was to analyze personal hygiene skills (hand washing) with the incidence of infection in children.
Methods: The method in this study was a pre-experimental study with a pretest-posttest design. The samples were 20 respondents of school-age children. Differences in pretest-posttest personal hygiene skills (hand washing).
Results: The results are based on data collected from 20 subjects, the results of the pretest-posttest personal hygiene skills (hand washing) in the Wilcoxon test, there was a significant difference, namely (p = 0.541).
Conclusion: There was no correlation between personal hygiene (hand washing) and the incidence of infection.
Prediksi Kelulusan Mahasiswa Program Pendidikan Multi Profesi 1 Tahun dengan Metode Naïve Bayes
Authors: Dinata Suhendra Anjar , Hijrah  , Musfikar Rahmat 
Published: August 2022

Tingkat kelulusan mahasiswa program pendidikan multi profesi satu tahun El Rahma sejak tahun akademik 2014 sampai 2016 mengalami penurunan. Kondisi tersebut sehingga mendorong pihak El Rahma melakukan evaluasi serta menyusunlangkah langkah strategis terhadap permasalahan tersebut untuk meningkatkan tingkat kelulusan mahasiswa dengan cara sasaran mutu bisa tercapai. Evaluasi terhadap permsalahan program studi tersebut perlu ditingkatkan dengan membuat sebuah sistem untuk memprediksi tingkat kelulusan pada proses perkuliahan. Dengan teknik data mining khususnya dalam klasifikasi untuk prediksi dengan algoritma klasifikasi naive bayes dapat dilakukan prediksi terhadap kelulusan studi dari mahasiswa. Data training dan testing yang digunakan diambil secara random pada data master yang digunakan adalah data kelulusan tahun 2016. Algoritma naive bayes mampu menghitung perbandingan peluang antara jumlah masing-maisng kriteria nilai atribut terhadap nilai hasil prediksi kelulusan mahasiswa. Dari penelitian dengan menggunakan data mahasiswa sebanyak 229 dengan jumlah 171 mahasiswa lulus dan 58 mahasiswa tidak lulus makan dengan menerapkan algoritma Naïve bayes didapatkan hasil bahwa tingkat akurasi menunjukan 90,85 % hal ini menunjukan bahwa algoritma naïve bayes baik diterapkan dalam melakukan prediksi kelulusan mahasiswa adapun hasil dari klasifikasi algoritma naïve bayes dapat diketahui attribut yang memberikan pengaruh pada tingkat kelulusan mahasiswa program pendidikan multi profesi satu tahun El Rahma diantaranya jenis kelamin, daerah asal, status marital, asal sekolah, status kerja, SPP bulanan, umur dan gelombang
Frequency of Home Accidents of Children Between 0-6 Years and Levels of Diagnosis of Mothers’ Safety Measures
Authors: ENER Dilek , ÖZBEY Mehmet Yavuz 
Published: August 2022

Aim: Children are vulnerable to home accidents and injuries due to their inability to protect themselves developmentally, and they need the protection of their parents. In the study, it was aimed to investigate the frequency of home accidents of children aged 0-6, the most common types of accidents, and the knowledge levels of mothers on Diagnosing Safety Precautions for Home Accidents.
Material and Method: The study is a cross-sectional and descriptive study and was conducted with 380 parents who applied to the pediatric outpatient clinic in December 2021. The “Scale of Diagnosing the Safety Precautions for Home Accidents of Mothers with 0-6 Age Group Children” was used in the questionnaire form. In the analysis of the relations between the variables, independent groups t-test, the One-way Anova test, the Pearson correlation test, Chi-Square test and Logistic Regression Analyze were applied.
Results: The frequency of children who had home accidents was 11.3%. The most common type of accident is falling. The mean score of the Mothers’ Scale for Diagnosing Safety Measures for Home Accidents was 155.9±15.2. Identification of Safety Precautions scores are higher in mothers who graduated from college, those whose children had a home accident, and those who received first aid knowledge. The most important factors affecting the accident at home are the number of children and the caregiver.
Conclusion: Home accidents, one of the preventable risk factors, are critical health problems. Providing information about all home accidents, especially falls, should be among the priority health targets.
Comparison of the Reliability of the “GÖK Atlas” and the “Gilsanz-Ratib Atlas” in the Determination of Bone Age in Turkish Children
Authors: AYVAT ÖCAL Zeynep , MERAL Orhan 
Published: August 2022

Aim: In this study we aimed to evaluate which of the GÖK and GR atlases is more compatible with chronological age in Turkish children aged 5-10 years.
Material and Method: In this study, the wrist radiographs of patients aged 5-10 years who applied to İzmir Bakırçay University Çiğli Training and Research Hospital due to trauma were retrospectively analyzed. A total of 360 wrist radiographs were evaluated. Bone age estimates in both groups were compared with chronological ages.
Results: In the correlation analysis, the prediction rate with 1-difference tolerance is 88.9% in the GR atlas and 76.7% in the GÖK atlas, while both atlases predict 99% correctly with two-difference tolerance. GR Atlas 168 (46.2%) and GÖK Atlas 147 (40.8%) predicted correctly regardless of gender and age. Of the correct estimations, 53.5% in the GR atlas and 57.8% in the GÖK atlas were male cases. İn male age group at the age of 6 and 10, the GR atlas is more successful, at the age of 7, the GÖK Atlas is more successful, and at the age of 5, 8, and 9 the success of both atlases is the same. İn female age group at the age of 5,7, 8, and 10 the GR atlas is more successful, at the age of 6 and 9 the GÖK Atlas is more successful
Conclusion: The GR Atlas was more accurate than the GÖK Atlas. Both the GR Atlas and the GÖK Atlas predicted more accurately in males. Since reference values for bone age can change with environmental and genetic factors all over the world, it is beneficial for all races to create atlas models with multicenter studies in order to establish their own standards.
Idealized 2D Cloud-resolving Simulations for Tidally Locked Habitable Planets
Authors: Song Qiyu , Yang Jun , Luo Hang , Li Cheng , Fu Shizuo 
Published: August 2022

Abstract
Cloud is critical for planetary climate and habitability, but it is also one of the most challenging aspects of studying planets in and beyond the solar system. Here we use a cloud-resolving model (CRM) with high resolution (2 km) in a 2D configuration to simulate the clouds and circulation on tidally locked aquaplanets. We find that the substellar area is covered by deep convective clouds, the nightside is dominated by low-level clouds, and the two are linked by a global-scale Walker circulation. We further find that uniform surface warming causes the substellar cloud width to decrease, but a reduction in the day–night surface temperature contrast or an increase in the longwave radiative cooling rate causes the substellar cloud width to increase. These relationships can be roughly interpreted in accordance with simple thermodynamic theories. Comparing the results between the CRM and the global 3D general circulation model (GCM), we find that they are qualitatively consistent, including the Walker circulation, the substellar clouds, and the responses of the substellar ascending area and strength to changes in the surface temperature or in its zonal contrast. But large quantitative differences exist, such as the magnitude of the cloud water path, the cloud width, and their responses to external forcings. These results increase our confidence in using GCMs to model exoplanetary climates, although large quantitative uncertainties are always likely to exist. Future work is required to use 3D CRMs with realistic radiative transfer and the Coriolis force to examine the clouds and climates of tidally locked planets.
First High-resolution Observations of Interstellar Pickup Ion Mediated Shocks in the Outer Heliosphere
Authors: McComas D. J. , Shrestha B. L. , Swaczyna P. , Rankin J. S. , Weidner S. E. , Zirnstein E. J. , Elliott H. A. , Singer K. N. , Spencer J. , Stern S. A. , Weaver H. A. 
Published: August 2022

Abstract
This study reports the first high-time-resolution observations of interstellar pickup ions (PUIs) in the outer heliosphere, including the first high-resolution observations of PUIs mediating shocks collected anywhere. These new data were enabled by a clever flight software reprogramming of the Solar Wind Around Pluto (SWAP) instrument on New Horizons to provide ∼30 minutes resolution as compared to the previous ∼24 hr time resolution. This time resolution is sufficient to resolve the shock structures and quantify the particle heating across these shocks. In the ∼10 months of initial data, we observed seven relatively small shocks, including one reverse shock. We find that the PUIs are preferentially compressed and heated across the shocks, indicating compression ratios from ∼1.2–1.8, with little heating for values less than ∼1.5 and progressively more PUI heating for larger compression ratios. In contrast, core solar wind properties did not show consistent changes across the shocks, indicating that these particles (1) participate little in the large-scale fluid-like interactions of the outer heliosphere’s combined solar wind and PUI plasma and (2) cannot be used to characterize PUI-mediated shocks as prior studies sought to do. All six forward shock crossings showed gradual increases in PUI pressure over shock widths of ∼0.05–0.13 au, which is roughly three decades larger than characteristic particle scales such as the PUI gyroradii. The new high-resolution observations and results described here are important for understanding shocks in the outer heliosphere, the termination shock, and more broadly for PUI-mediated shocks across many astrophysical systems.
Magnetic Field Intermittency in the Solar Wind: Parker Solar Probe and SolO Observations Ranging from the Alfvén Region up to 1 AU
Authors: Sioulas Nikos , Huang 黄 Zesen 泽森 , Velli Marco , Chhiber Rohit , Cuesta Manuel E. , Shi 时 Chen 辰 , Matthaeus William H. , Bandyopadhyay Riddhi , Vlahos Loukas , Bowen Trevor A. , Qudsi Ramiz A. , Bale Stuart D. , Owen Christopher J. , Louarn P. , Fedorov A. , Maksimović Milan , Stevens Michael L. , Case Anthony , Kasper Justin , Larson Davin , Pulupa Marc , Livi Roberto 
Published: August 2022

Abstract
Parker Solar Probe (PSP) and SolO data are utilized to investigate magnetic field intermittency in the solar wind (SW). Small-scale intermittency (20−100 d

i
) is observed to radially strengthen when methods relying on higher-order moments are considered (SF
q
; SDK), but no clear trend is observed at larger scales. However, lower-order moment-based methods (e.g., partial variance of increments; PVI) are deemed more appropriate for examining the evolution of the bulk of coherent structures (CSs), PVI ≥ 3. Using PVI, we observe a scale-dependent evolution in the fraction of the data set occupied by CSs, f
PVI≥3. Specifically, regardless of the SW speed, a subtle increase is found in f
PVI≥3 for ℓ = 20 d

i
, in contrast to a more pronounced radial increase in CSs observed at larger scales. Intermittency is investigated in relation to plasma parameters. Though, slower SW speed intervals exhibit higher f
PVI≥6 and higher kurtosis maxima, no statistical differences are observed for f
PVI≥3. Highly Alfvénic intervals display lower levels of intermittency. The anisotropy with respect to the angle between the magnetic field and SW flow, ΘVB is investigated. Intermittency is weaker at ΘVB ≈ 0° and is strengthened at larger angles. Considering the evolution at a constant alignment angle, a weakening of intermittency is observed with increasing advection time of the SW. Our results indicate that the strengthening of intermittency in the inner heliosphere is driven by the increase in comparatively highly intermittent perpendicular intervals sampled by the probes with increasing distance, an effect related directly to the evolution of the Parker spiral.
1RXH J082623.6–505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate
Authors: Sokolovsky Kirill V. , Strader Jay , Swihart Samuel J. , Aydi Elias , Bahramian Arash , Chomiuk Laura , Heinke Craig O. , Hughes Allison K. , Li Kwan-Lok , de Oliveira Raimundo Lopes , Miller-Jones James C. A. , Mukai Koji , Sand David J. , Shishkovsky Laura , Tremou Evangelia , Voggel Karina 
Published: August 2022

Abstract
We report the discovery of 1RXH J082623.6−505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a ∼0.4 M
⊙ K-type secondary transferring mass through a low-state accretion disk to a nonmagnetic ∼0.8 M
⊙ white dwarf. The secondary is overluminous for its mass and dominates the optical spectra at all epochs and must be evolved to fill its Roche Lobe at this orbital period. The X-ray luminosity L

X
∼ 1–2 × 1032 erg s−1 derived from both new XMM-Newton and archival observations, although high compared to most CVs, still only requires a modest accretion rate onto the white dwarf of

M

̇

∼ 3 × 10−11 to 3 × 10−10
M
⊙ yr−1, lower than expected for a cataclysmic variable with an evolved secondary. No dwarf nova outbursts have yet been observed from the system, consistent with the low derived mass-transfer rate. Several other cataclysmic variables with similar orbital periods also show unexpectedly low mass-transfer rates, even though selection effects disfavor the discovery of binaries with these properties. This suggests the abundance and evolutionary state of long-period, low mass-transfer rate cataclysmic variables are worthy of additional attention.
Relativistic Magnetic Explosions
Authors: Barkov Maxim V. , Sharma Praveen , Gourgouliatos Konstantinos N. , Lyutikov Maxim 
Published: August 2022

Abstract
Many explosive astrophysical events, like magnetars’ bursts and flares, are magnetically driven. We consider dynamics of such magnetic explosions—relativistic expansion of highly magnetized and highly magnetically overpressurized clouds. The corresponding dynamics are qualitatively different from fluid explosions due to the topological constraint of the conservation of the magnetic flux. Using analytical, relativistic MHD as well as force-free calculations, we find that the creation of a relativistically expanding, causally disconnected flow obeys a threshold condition: it requires sufficiently high initial overpressure and a sufficiently quick decrease of the pressure in the external medium (the preexplosion wind). In the subcritical case the magnetic cloud just “puffs up” and quietly expands with the preflare wind. We also find a compact analytical solution to Prendergast’s problem—expansion of force-free plasma into a vacuum.
Universal Relations for the Increase in the Mass and Radius of a Rotating Neutron Star
Authors: Konstantinou Andreas , Morsink Sharon M. 
Published: August 2022

Abstract
Rotation causes an increase in a neutron star’s mass and equatorial radius. The mass and radius depend sensitively on the unknown equation of state (EOS) of cold, dense matter. However, the increases in mass and radius due to rotation are almost independent of the EOS. The EOS independence leads to the idea of neutron star universality. In this paper, we compute sequences of rotating neutron stars with constant central density. We use a collection of randomly generated EOSs to construct simple correction factors to the mass and radius computed from the equations of hydrostatic equilibrium for nonrotating neutron stars. The correction factors depend only on the nonrotating star’s mass and radius and are almost independent of the EOS. This makes it computationally inexpensive to include observations of rotating neutron stars in EOS inference codes. We also construct a mapping from the measured mass and radius of a rotating neutron star to a corresponding nonrotating star. The mapping makes it possible to construct a zero-spin mass–radius curve if the masses and radii of many neutron stars with different spins are measured. We show that the changes in polar and equatorial radii are symmetric, in that the polar radius shrinks at the same rate in which the equatorial radius grows. This symmetry is related to the observation that the equatorial compactness (the ratio of mass to radius) is almost constant on one of the constant-density sequences.