bluuebunny/crossref_metadata_2025_split huggingface dataset:
PENERAPAN HEALTH BELIEF MODEL SEBAGAI UPAYA PENCEGAHAN INFEKSI MENULAR SEKSUAL PADA IBU RUMAH TANGGA
Authors: Agustina Silvia Ari , Murti Bhisma , Demartoto Argyo 
Published: March 2018

Latar Belakang. Masalah kesehatan seksual dan reproduksi semakin menjadi perhatian di seluruh dunia antara lain berkaitan dengan kebersihan genetalia. Perawatan genital masih sangat tabu untuk dibicarakan dikalangan masyarakat Indonesia. Higiene Genital yang buruk dapat meningkatkan risiko mengalami IMS. Persepsi dalam Health Belief Model (HBM) diyakini dapat menentukan kemungkinan individu melakukan perilaku kesehatan.
Objective: Penelitian ini untuk menganalisis penerapan Health Belief Model dengan higiene genital Ibu Rumah Tangga
Metode. Objek penelitian ini adalah Ibu Rumah Tangga, dengan total sampel 101, termasuk 2 Ibu Rumah Tangga, 2 Suami, petugas Puskesmas yang melayani penapisan Infeksi Menular Seksual dan 1 Lembaga Swadaya Masyarakat. Teknik sampling menggunakan quota sampling. Jenis penelitian ini mixed methodology dengan strategi eksplanatoris sekuensial dan menggunakan pendekatan cross sectional study.Teknik pengambilan data kuantitatif dengan menggunaan kuesioner tertutup dan untuk data kualitatif dengan wawancara mendalam. Analisis yang digunakan adalah regresi linier ganda. Validitas dan reliabilitas data kualitatif menggunakan triangulasi sumber dan metode.
Hasil: Higiene Genital dengan beberapa variabel independen yang diteliti mempunyai hubungan yang positif dengan persepsi kerentanan (b:0,97; CI 95%: 0,87 hingga 1,06; p<0,01), efikasi diri (b: 0,02; CI 95%: 0,00 hingga 0,05; p<0,05), dan cues to action higiene genital (b:0,16; CI 95%: 0,08 hingga 0,23; p<0,01). Terdapat hubungan negatif antara higiene genital dengan persepsi hambatan higiene (b:-0,13; CI 95%: -0,18 hingga -0,09; p<0,01). Secara bersama-sama seluruh variabel independen di dalam model regresi linier ganda ini mampu menjelaskan higiene genital sebesar 84,5%. Ibu Rumah Tangga menyatakan bahwa higiene genital penting, tetapi dalam menjaga kesehatan alat kelaminnya masih kurang tepat, yaitu seperti sering menggunakan pembersih kewanitaan, celana dalam yang ketat, dan saat keputihan sering menggunakan pentyliner.
Kesimpulan. Terdapat 4 komponen Health Belief Model berhubungan dengan higiene genital.
HUBUNGAN POLA ASUH DENGAN POLA PERKEMBANGAN SEKSUAL SEKUNDER PADA SISWA SMP
Authors: Mayang Sari Uci , Musvita Ayu Suci 
Published: March 2018

Background: Adolescence is a transition period from childhood to adulthood, both physically and psychologically. Parents are generally considered as primary teachers for their children, therefore parents play important roles in children development. Parenting style is one of the factors associated with the pattern of secondary sexual development.
Objective: This study aimed to examine the relationship between parenting style and the pattern of secondary sexual development in junior high school students.
Methods: This research was an observational analytic study, using cross sectional approach. The study population was all male students at SMP 1 Berbah Yogyakarta (188 students). Samples were selected using purposive sampling, involving 143 respondents. Data were analyzed with Chi square test.
Result: There was a correlation between parenting style and the pattern of secondary sexual development (p= 0.000 <0.05), with PR value of 4,975, CI 95 % of 1,831-13,516.
Conclusion: There was a relationship between parenting style and the pattern of secondary sexual development in junior high school students.
Keywords: Adolescence, Parenting, Patterns of Sexual Secondary Students
GAMBARAN KARAKTERISTIK WANITA YANG MENGALAMI KANKER SERVIKS DI RUMAH SAKIT UMUM DAERAH (RSUD) PANEMBAHAN SENOPATI BANTUL YOGYAKARTA
Authors: Anggraeni Fatimah Dewi , Rahayu Retno 
Published: March 2018

Background : Cervical cancer is still becoming the most prevalent diseases in Indonesia. Health Department of Indonesia in 2012 recorded that the predicted incidence and mortality rate which caused by cervical cancer were 13.2 million of lifes. Factors that affecting cervical cancer are age, education, job, parity, and hormonal contracepcy. This statement is supported by the Hospital Information System (HIS) data in the year of 2013 which showed that there were 130 cases of cervical cancer in Yogyakarta (DIY). The opreliminary study obtained that in 2015 there were 50 persons of cervical cancer sufferer in Panembahan Senopati Public Hospital, which were consist of 40 outpatient cases and 10 inpatient cases.
Aim : This study aimed to know the characteristics of mothers who encounter cervical cancer.
Research Methods : This research was a descriptive quantitative research. The sampling technique used in this research was total sampling technique. The samples were 50 respondents with frequency distribution that obtained by using secondary data and checklist methods.
Results : Most of mothers who encounter cervical cancer in Panembahan Senopati public hospital Bantul Yogyakarta that aged >35 years old were as many as 34 respondents (68.0%), as many as 26 respondents (52.0%) were high school educated or graduated, as many as 18 repondents (36.05) were statused as a farmer, as many as 18 repondents (36.0%) were primiparas and grandemulti parity, and as many as 29 respondents (58.0%) were using hormonal contracepcy.
Conclusion : Mothers who encounter cervical cancer in Panembahan Senopati public hospital Bantul Yogyakarta that aged >35 years old were: high school educated or graduated, farmers, primiparas and grandmultiparas, and using hormonal contracepcy.
Keywords : Characteristic, Cervical cancer
A PERILAKU MENCUCI TANGAN PENGUNJUNG RUMAH SAKIT DI RUMAH SAKIT SWASTA YOGYAKARTA
Authors: Theresia Siwi Ikaristi Maria 
Published: March 2018

Background: Visitors take part in the occurrence of nosocomial infections. Their hands are a reservoir for microorganisms that can be transmitted to patients as individuals susceptible for secondary infections. Hand washing before and after visiting patients is the easiest way to remove colonies of microorganisms in the hands. The alcohol-based hand rub is available for visitors in the hospital’s rooms but there are no evaluation by hospital managemen.
Objective: This study aims to evaluate hand-washing behavior of visitors at a private hospital in Yogyakarta.
Methods: Research method used descriptive quantitative survey. Sample was taken by accidental sampling from 2015 - 2017 and got 229 respondents. Data collection by observation in the room includes ICU, ICCU, surgical ward and post partum ward.
Results: The result showed that percentage visitors who did not wash their hands before and after entering in the ICU was 50% and 83.33%, in the medical ward was 80% and 81.82%, in the ICCU was 81,73% and 70,19% and in the post partum ward was 57,5% and 30%.
Conclusion: The high percentage of respondents who did not wash their hands before and after visiting patients is an important concern because they will carry microorganisms that can be transmitted to others. Suggestions for hospital are to campaign, make banners and leaflets for health promotion of the importance washing hands before and after visiting patients in the hospital for public.
Key words: hand washing, visitors, nosocomial infection.
Four Weekly Ayahuasca Sessions Lead to Increases in “Acceptance” Capacities: A Comparison Study With a Standard 8-Week Mindfulness Training Program
Authors: Soler Joaquim , Elices Matilde , Dominguez-Clavé Elisabeth , Pascual Juan C. , Feilding Amanda , Navarro-Gil Mayte , García-Campayo Javier , Riba Jordi 
Published: March 2018

Background: The therapeutic effects of the Amazonian plant tea ayahuasca may relate to its ability to enhance mindfulness capacities. Ayahuasca induces a modified state of awareness through the combined action of its active principles: the psychedelic N,N-dimethyltryptamine (DMT) and a series of centrally acting β-carbolines, mainly harmine and tetrahydroharmine. To better understand the therapeutic potential of ayahuasca, here we compared the impact on mindfulness capacities induced by two independent interventions: (a) participation in four ayahuasca sessions without any specific purpose related to improving mindfulness capacities; and (b) participation in a standard mindfulness training course: 8 weeks mindfulness-based stress reduction (MBSR), with the specific goal of improving these skills.Methods: Participants of two independent groups completed two self-report instruments: The Five Facet Mindfulness Questionnaire (FFMQ) and the Experiences Questionnaire (EQ). The MINDSENS Composite Index was also calculated, including those EQ and FFMQ items that have proven to be the most sensitive to meditation practice. Group A (n = 10) was assessed before and after the last of four closely spaced consecutive ayahuasca sessions. Group B (n = 10) was assessed before and after completion of a standard 8-week MBSR course.Results: MBSR training led to greater increases in overall mindfulness scores after the 8-week period. MBSR but not ayahuasca led to increases in the MINDSENS Composite Index. However, the ayahuasca sessions induced comparable increases in the Non-Judging subscale of the FFMQ, specifically measuring “acceptance.” Improving this capacity allows for a more detached and less judgmental stance toward potentially distressing thoughts and emotions.Results: The present findings suggest that a small number of ayahuasca sessions can be as effective at improving acceptance as more lengthy and costly interventions. Future studies should address the benefits of combining ayahuasca administration with mindfulness-based interventions. This will allow us to investigate if ayahuasca will improve the outcome of psychotherapeutic interventions.
Robo-AO Kepler Survey. IV. The Effect of Nearby Stars on 3857 Planetary Candidate Systems
Authors: Ziegler Carl , Law Nicholas M. , Baranec Christoph , Riddle Reed , Duev Dmitry A. , Howard Ward , Jensen-Clem Rebecca , Kulkarni S. R. , Morton Tim , Salama Maïssa 
Published: March 2018

Abstract
We present the overall statistical results from the Robo-AO Kepler planetary candidate survey, comprising of 3857 high-angular resolution observations of planetary candidate systems with Robo-AO, an automated laser adaptive optics system. These observations reveal previously unknown nearby stars blended with the planetary candidate host stars that alter the derived planetary radii or may be the source of an astrophysical false positive transit signal. In the first three papers in the survey, we detected 440 nearby stars around 3313 planetary candidate host stars. In this paper, we present observations of 532 planetary candidate host stars, detecting 94 companions around 88 stars; 84 of these companions have not previously been observed in high resolution. We also report 50 more-widely separated companions near 715 targets previously observed by Robo-AO. We derive corrected planetary radius estimates for the 814 planetary candidates in systems with a detected nearby star. If planetary candidates are equally likely to orbit the primary or secondary star, the radius estimates for planetary candidates in systems with likely bound nearby stars increase by a factor of 1.54, on average. We find that 35 previously believed rocky planet candidates are likely not rocky due to the presence of nearby stars. From the combined data sets from the complete Robo-AO KOI survey, we find that 14.5 ± 0.5% of planetary candidate hosts have a nearby star with 4″, while 1.2% have two nearby stars, and 0.08% have three. We find that 16% of Earth-sized, 13% of Neptune-sized, 14% of Saturn-sized, and 19% of Jupiter-sized planet candidates have detected nearby stars.
High Spectral Resolution SOFIA/EXES Observations of C2H2 toward Orion IRc2
Authors: Rangwala Naseem , Colgan Sean W. J. , Gal Romane Le , Acharyya Kinsuk , Huang Xinchuan , Lee Timothy J. , Herbst Eric , deWitt Curtis , Richter Matt , Boogert Adwin , McKelvey Mark 
Published: March 2018

Abstract
We present high spectral resolution observations from 12.96 to 13.33 microns toward Orion IRc2 using the mid-infrared spectrograph, Echelon-Cross-Echelle Spectrograph (EXES), at Stratospheric Observatory for Infrared Astronomy (SOFIA). These observations probe the physical and chemical conditions of the Orion hot core, which is sampled by a bright, compact, mid-infrared background continuum source in the region, IRc2. All 10 of the rovibrational C2H2 transitions expected in our spectral coverage are detected with high signal-to-noise ratios (S/Ns), yielding continuous coverage of the R-branch lines from J = 9–8 to J = 18–17, including both ortho and para species. Eight of these rovibrational transitions are newly reported detections. The isotopologue, 13CCH2, is clearly detected with a high S/N. This enabled a direct measurement of the 12C/13C isotopic ratio for the Orion hot core of 14 ± 1 and an estimated maximum value of 21. We also detected several HCN rovibrational lines. The ortho and para C2H2 ladders are clearly separate, and tracing two different temperatures, 226 K and 164 K, respectively, with a non-equilibrium ortho to para ratio (OPR) of 1.7 ± 0.1. Additionally, the ortho and para V
LSR values differ by about 1.8 ± 0.2 km s−1, while the mean line widths differ by 0.7 ± 0.2 km s−1, suggesting that these species are not uniformly mixed along the line of sight to IRc2. We propose that the abnormally low C2H2 OPR could be a remnant from an earlier, colder phase, before the density enhancement (now the hot core) was impacted by shocks generated from an explosive event 500 years ago.
Deep Learning Based Solar Flare Forecasting Model. I. Results for Line-of-sight Magnetograms
Authors: Huang Xin , Wang Huaning , Xu Long , Liu Jinfu , Li Rong , Dai Xinghua 
Published: March 2018

Abstract
Solar flares originate from the release of the energy stored in the magnetic field of solar active regions, the triggering mechanism for these flares, however, remains unknown. For this reason, the conventional solar flare forecast is essentially based on the statistic relationship between solar flares and measures extracted from observational data. In the current work, the deep learning method is applied to set up the solar flare forecasting model, in which forecasting patterns can be learned from line-of-sight magnetograms of solar active regions. In order to obtain a large amount of observational data to train the forecasting model and test its performance, a data set is created from line-of-sight magnetogarms of active regions observed by SOHO/MDI and SDO/HMI from 1996 April to 2015 October and corresponding soft X-ray solar flares observed by GOES. The testing results of the forecasting model indicate that (1) the forecasting patterns can be automatically reached with the MDI data and they can also be applied to the HMI data; furthermore, these forecasting patterns are robust to the noise in the observational data; (2) the performance of the deep learning forecasting model is not sensitive to the given forecasting periods (6, 12, 24, or 48 hr); (3) the performance of the proposed forecasting model is comparable to that of the state-of-the-art flare forecasting models, even if the duration of the total magnetograms continuously spans 19.5 years. Case analyses demonstrate that the deep learning based solar flare forecasting model pays attention to areas with the magnetic polarity-inversion line or the strong magnetic field in magnetograms of active regions.
A 100 au Wide Bipolar Rotating Shell Emanating from the HH 212 Protostellar Disk: A Disk Wind?
Authors: Lee Chin-Fei , Li Zhi-Yun , Codella Claudio , Ho Paul T. P. , Podio Linda , Hirano Naomi , Shang Hsien , Turner Neal J. , Zhang Qizhou 
Published: March 2018

Abstract
HH 212 is a Class 0 protostellar system found to host a “hamburger”-shaped dusty disk with a rotating disk atmosphere and a collimated SiO jet at a distance of ∼400 pc. Recently, a compact rotating outflow has been detected in SO and SO2 toward the center along the jet axis at ∼52 au (0.″13) resolution. Here we resolve the compact outflow into a small-scale wide-opening rotating outflow shell and a collimated jet, with the observations in the same S-bearing molecules at ∼16 au (0.″04) resolution. The collimated jet is aligned with the SiO jet, tracing the shock interactions in the jet. The wide-opening outflow shell is seen extending out from the inner disk around the SiO jet and has a width of ∼100 au. It is not only expanding away from the center, but also rotating around the jet axis. The specific angular momentum of the outflow shell is ∼40 au km s−1. Simple modeling of the observed kinematics suggests that the rotating outflow shell can trace either a disk wind or disk material pushed away by an unseen wind from the inner disk or protostar. We also resolve the disk atmosphere in the same S-bearing molecules, confirming the Keplerian rotation there.
The Mass and Absorption Columns of Galactic Gaseous Halos
Authors: Qu Zhijie , Bregman Joel N. 
Published: March 2018

Abstract
The galactic gaseous halo is a gas reservoir for the interstellar medium in the galaxy disk, supplying materials for star formation. We developed a gaseous halo model connecting the galaxy disk and the gaseous halo by assuming that the star formation rate on the disk is balanced by the radiative cooling rate of the gaseous halo, including stellar feedback. In addition to a single-temperature gaseous halo in collisional ionization equilibrium, we also consider the photoionization effect and a steady-state cooling model. Photoionization is important for modifying the ion distribution in low-mass galaxies and in the outskirts of massive galaxies due to the low densities. The multiphase cooling model dominates the region within the cooling radius, where t
cooling = t
Hubble. Our model reproduces most of the observed high ionization state ions for a wide range of galaxy masses (i.e., O vi, O vii, Ne viii, Mg x, and O viii). We find that the O vi column density has a narrow range around ≈1014 cm−2 for halo masses from M
⋆ ≈ 3 × 1010
M
⊙ to 6 × 1012
M
⊙, which is consistent with some but not all observational studies. For galaxies with halo masses ≲3 × 1011
M
⊙, photoionization produces most of the O vi, while for more massive galaxies, the O vi is from the medium that is cooling from higher temperatures. Fitting the Galactic (Milky-Way) O vii and O viii suggests a gaseous halo model where the metallicity is ≈0.55 Z
⊙ and the gaseous halo has a maximum temperature of ≈1.9 × 106 K. This gaseous halo model does not close the census of baryonic material within R
200.
Magnetorotational Instability in Eccentric Disks
Authors: Chan Chi-Ho , Krolik Julian H. , Piran Tsvi 
Published: March 2018

Abstract
Eccentric disks arise in such astrophysical contexts as tidal disruption events, but it is unknown whether the magnetorotational instability (MRI), which powers accretion in circular disks, operates in eccentric disks as well. We examine the linear evolution of unstratified, incompressible MRI in an eccentric disk orbiting a point mass. We consider vertical modes of wavenumber k on a background flow with uniform eccentricity e and vertical Alfvén speed

along an orbit with mean motion n. We find two mode families, one with dominant magnetic components, the other with dominant velocity components. The former is unstable at

, where

, and the latter at e ≳ 0.8. For f
2 ≲ 3, MRI behaves much like in circular disks, but the growth per orbit declines slowly with increasing e; for f
2 ≳ 3, modes grow by parametric amplification, which is resonant for 0 < e ≪ 1. MRI growth and the attendant angular momentum and energy transport happen chiefly near pericenter, where orbital shear dominates magnetic tension.
The MASSIVE Survey. IX. Photometric Analysis of 35 High-mass Early-type Galaxies with HST WFC3/IR*
Authors: Goullaud Charles F. , Jensen Joseph B. , Blakeslee John P. , Ma Chung-Pei , Greene Jenny E. , Thomas Jens 
Published: March 2018

Abstract
We present near-infrared observations of 35 of the most massive early-type galaxies in the local universe. The observations were made using the infrared channel of the Hubble Space Telescope Wide Field Camera 3 (WFC3) in the F110W (1.1 μm) filter. We measured surface brightness profiles and elliptical isophotal fit parameters from the nuclear regions out to a radius of ∼10 kpc in most cases. We find that 37% (13) of the galaxies in our sample have isophotal position-angle rotations greater than 20° over the radial range imaged by WFC3/IR, which is often due to the presence of neighbors or multiple nuclei. Most galaxies in our sample are significantly rounder near the center than in the outer regions. This sample contains 6 fast rotators and 28 slow rotators. We find that all fast rotators are either disky or show no measurable deviation from purely elliptical isophotes. Among slow rotators, significantly disky and boxy galaxies occur with nearly equal frequency. The galaxies in our sample often exhibit changing isophotal shapes, sometimes showing both significantly disky and boxy isophotes at different radii. The fact that parameters vary widely between galaxies and within individual galaxies is evidence that these massive galaxies have complicated formation histories, and some of them have experienced recent mergers and have not fully relaxed. These data demonstrate the value of IR imaging of galaxies at high spatial resolution and provide measurements necessary for determining stellar masses, dynamics, and black hole masses in high-mass galaxies.
Not All Stars Are the Sun: Empirical Calibration of the Mixing Length for Metal-poor Stars Using One-dimensional Stellar Evolution Models
Authors: Joyce M. , Chaboyer B. 
Published: March 2018

Abstract
Theoretical stellar evolution models are constructed and tailored to the best known, observationally derived characteristics of metal-poor ([Fe/H] ∼ −2.3) stars representing a range of evolutionary phases: subgiant HD 140283, globular cluster M92, and four single, main sequence stars with well-determined parallaxes: HIP 46120, HIP 54639, HIP 106924, and WOLF 1137. It is found that the use of a solar-calibrated value of the mixing length parameter α
MLT in models of these objects is ineffective at reproducing their observed properties. Empirically calibrated values of α
MLT are presented for each object, accounting for uncertainties in the input physics employed in the models. It is advocated that the implementation of an adaptive mixing length is necessary in order for stellar evolution models to maintain fidelity in the era of high-precision observations.
Le grand bond en avant du procès de la justice climatique, « Juliana » contre l´administration Trump
Authors: Mougeolle Paul 
Published: March 2018

Dans l´affaire Juliana et al. v. USA, vingt et un plaignants issus de la nouvelle génération de citoyens invoquent une violation de leurs droits fondamentaux à la vie et à la propriété afin de contraindre l´administration Trump à agir contre le changement climatique. Alors que le tribunal de première instance avait déjà reconnu à plusieurs reprises la recevabilité de la requête des demandeurs, le gouvernement avait finalement réussi à interjeter un appel exceptionnel à cet égard. Cette requête a néanmoins été rejetée et un procès sur le fond de l´affaire devient désormais hautement probable.