bluuebunny/crossref_metadata_2025_split huggingface dataset:
The Limitations and Solutions in Chinese Legislation about Sexual Harassment in Workplace Based on Analysis and Case Studies
Authors: Li Yujiao 
Published: August 2024

In light of the burgeoning feminist movement in China, the issue of sexual harassment in the workplace has garnered significant attention both from the public and legislative bodies. This article sheds light on the shortcomings of current Chinese legislation concerning workplace sexual harassment, proposing viable solutions supported by case studies and survey data. It reveals a lack of precision in existing legal provisions and the absence of specific laws or regulations in this domain. Moreover, the detrimental aftermath experienced by victims underlines the urgency of addressing these deficiencies. The article advocates for a bilateral approach, focusing on actions to be taken by both individuals and employers. Empowering victims through heightened awareness is highlighted as a fusion for reporting and pursuing legal recourse. Concurrently, it stresses the significance for employers to make robust anti-harassment policies, furnish employee training, and institute transparent procedures for addressing complaints. Collaboration between these two fronts emerges as pivotal in effectively combating sexual harassment within the workplace.
Tinjauan Penggunaan Komputer Terkait Gejala Computer Vision Syndrome (CVS) Pada Petugas Rekam Medis Di Rumah Sakit X kediri tahun 2023
Authors: Zuliana Nimatu , Wardhani Christabella Nafthalia , Jayanto Deni , Jayanti Krisnita , Laksono Adi 
Published: August 2024

Teknologi informasi saat ini berkembang sangat pesat. Perkembangan teknologi tersebut dibuktikan dengan penggunaan komputer pada Rekam Medis Eletronik. Penggunaan komputer dapat memberikan dampak positif dan negatif bagi penggunanya. Salah satu dampak negatifnya adalah Computer Vision Syndrome. Desain penelitian ini yaitu penelitian kuantitatif dengan metode deskriptif. Populasi penelitian berjumlah 24 petugas rekam medis yang menggunakan komputer dengan teknik pengambilan sampel yaitu purposive sampling, sampel berjumlah 6 petugas yang telah memenuhi kriteria inklusi. Pengumpulan data dilakukan dengan lembar wawancara dan observasi. Hasil dari penelitian ini didapatkan jumlah petugas rekam medis di Rumah Sakit X Kota Kediri yang lebih beresiko mengalami gejala Computer Vision Syndrome adalah 6 petugas dengan usia ≤45 tahun, masa kerja 4 petugas ≤5 tahun dan 2 petugas >5 tahun, lama menatap monitor komputer dari 6 petugas termasuk dalam kategori waktu >2 jam, jarak monitor komputer dengan mata dari 3 petugas berjarak 45-60 cm dan 3 petugas lainnya berjarak <45->60 cm. Sebaiknya petugas dapat melakukan kedipan mata secara berkala, mengatur kecerahan monitor komputer, melakukan pengecekan ketajaman penglihatan (visual), melakukan istirahat mata secara teratur dengan aturan 20-20-20 dan menggunakan teknik zoom in atau zoom out untuk menyesuaikan tulisan pada layar komputer.
Evaluasi Kegiatan Pelayanan Pendaftaran Pasien di RS X Malang
Authors: Alvionita Chyntia Vicky , Marselina Elystia Vidia 
Published: August 2024

Pelayanan pendaftaran merupakan pelayanan pertama dan secara langsung berinteraksi dengan pasien dan tempat dimana akan mendaftar ke poliklinik yang akan dituju. Berdasarkan hasil observasi diketahui bahwa kegiatan pada pelayanan pendaftaran pasien masih terkendala beberapa hal, antara lain jaringan dan pada SIMRS. Salah satu upaya yang dilakukan untuk menyelesaikan permasalahan tersebut yaitu melakukan evaluasi kegiatan pada pelayanan pendaftaran pasien. Tujuan dari penelitian ini adalah untuk melakukan evaluasi kegiatan pada pelayanan pendafataran pasien. Instrumen yang digunakan adalah lembar wawancara. Jenis penelitian menggunakan analisis deskriptif kualitatif untuk menggambarkan hasil evaluasi pada pelayanan pendafataran pasien. Hasil penelitian menunjukkan bahwa pelayanan pendaftaran di RSI Unisma Malang berjalan dengan baik, namun masih ada beberapa permasalahan yang terjadi. Koneksi internet yang lambat dan tidak stabil sering kali menjadi kendala dalam melakukan pendaftaran pasien. Gangguan pada SIMRS juga kerap terjadi dan beresiko terjadinya perlambatan dalam proses pendaftaran. Selain itu tracer masih manual, sehingga menyebabkan resiko petugas pendaftaran lupa untuk menuliskan data rekam medis pasien. Masalah lainnya yang terjadi adalah SIMRS yang belum bridging dengan BPJS menyebabkan pendaftaran pasien BPJS lebih lama karena melalui banyak tahap.
Bone Metastasis Evaluation Using Bone Scintigraphy
Authors: Yousef Mohamed , Algethami Shmoukh , Alfarra Raghda , Abdullah Bayan , Alahmadi Remaz , Jastaniah Saddig 
Published: August 2024

Background: Diagnosing bone metastasis in patients with a history of cancer remains challenging. Diagnostic evaluation may be prolonged owing to difficulties in distinguishing between bone metastasis and common orthopedic diseases.
Objectives: This study aimed to evaluate bone metastasis using scintigraphy
Materials and Methods: A retrospective study was carried out at Batterjee Medical College, Radiologic Sciences program, and King Abdulaziz University Hospital. It included 200 consecutive patients with a history of malignant disease (60% Females and 40% Males) referred for bone scintigraphy. Using a database of the King Abdulaziz University Hospital, the prevalence of bone metastasis from each type of primary cancer was noted.
Results: The results showed that most participants were above 50 years old, with Primary cancer sites including Breast cancer (88 (44%) cases), Prostate cancer (15%), Lung and colon (11%), and Bone metastasis locations including spine (186), Ribs (n= 136), pelvis (n= 133), Lower Extremities (n= 108), and Skull (n= 59), respectively.
Conclusions: The most common malignancy is breast cancer, followed by prostate carcinoma, and most bone metastasis locations include the spine, Ribs, and pelvis.
Association between celiac disease and fibromyalgia and their severity: a cross-sectional study
Authors: Kılıçoğlu Mehmet Serkan , Sayılır Safiye , Yurdakul Ozan Volkan , Aydin Teoman , Koçhan Koray , Basaranoglu Metin , Kucukakkas Okan 
Published: August 2024

Background
Fibromyalgia (FMS) is a common musculoskeletal disorder with many causes. People with fibromyalgia often have the same symptoms as people with celiac disease (CD). Demonstration of the coordination and frequency of FMS and CD is important for effective treatment.

Methods
This is a single center cross-sectional clinical study. The study included 60 patients who were diagnosed with CD by the Gastroenterology Clinic based on American College of Gastroenterology (ACG) criteria. Patients were also asked to complete the Widespread Pain Index (WPI), Symptom Severity Scale (SSS), and Fibromyalgia Impact Questionnaire (FIQ) to diagnose fibromyalgia and assess its severity. The results were used to analyze the frequency of concomitance and relationship between the two diseases.

Results
The relationship between the clinical types of CD and the presence of fibromyalgia was insignificant. Analysis of the relationship between the pathologic typing of biopsy and fibromyalgia frequency was insignificant. Those with antibodies more frequently met criteria for fibromyalgia (P = 0.04, P = 0.04, respectively).

Conclusions
Presence of clinical extraintestinal manifestations in patients with CD should lead clinicians to consider FMS as a possible diagnosis. This points to the importance for clinicians in all subspecialties to be aware of the various symptoms and diseases associated with FMS.
Influence of Different Organic Manures and Inorganic Fertilizers on Growth Attributes and Flower Yield of Marigold (Tagetes erecta L.) under Foot Hills of Himalaya
Authors: Singh Satendra Kumar 
Published: August 2024

The experiment was conducted at farmer’s field, Deoria, Uttar Pradesh during 2021-22 and 2022-23.The experiment consisted of 11 treatments which were replicated thrice in Randomized complete blocks design (RCBD). The result showed significant effect on plant height (66.40 cm), girth of stem (1.43 cm), number of branches plant-1 (17.10), plant spread along the row (38.30 cm), plant spread across the row (38.32 cm), days to start flowering (68.10 days), flowering duration (24.40 days), number of flower plant-1 (23.50), circumferences of flower (24.20 cm), fresh weight of flower (12.25 g) and fresh yield plant-1 (264.08 g) was observed in T10 i.e. 2.5 tonne poultry manure ha-1 with 50% Recommended Dose of Fertilizers (RDF) followed by T4,T7 and T3.
Constraints on the evolution of crustal flow beneath Northern Tibet
Authors: Le Pape Florian , Jones Alan G. , Unsworth Martyn J. , Vozar Jan , Wei Wenbo , Jin Sheng , Ye Gaofeng , Jing Jianen , Dong Hao , Zhang Letian , Xie Chengliang 
Published: November 2015

AbstractCrustal flow is an important tectonic process active in continent‐continent collisions and which may be significant in the development of convergent plate boundaries. In this study, the results from multidimensional electrical conductivity modeling have been combined with laboratory studies of the rheology of partially molten rocks to characterize the rheological behavior of the middle‐to‐lower crust of both the Songpan‐Ganzi and Kunlun terranes in the northern Tibetan Plateau. Two different methods are adopted to develop constraints on melt fraction, temperature, and crustal flow velocity in the study area. The estimates of these parameters are then used to evaluate whether crustal flow can occur on the northern margin of the Tibetan plateau. In the Songpan‐Ganzi crust, all conditions are satisfied for topography‐driven channel flow to be dominant, with partial melt not being required for flow at temperature above 1000°C. Further north, the Kunlun fault defines the southern boundary of a transition zone between the Tibetan plateau and the Qaidam basin. Constrained by the estimated melt fractions, it is shown that channel injection across the fault requires temperatures close to 900°C. The composition of igneous rocks found at the surface confirm those conditions are met for the southern Kunlun ranges. To the north, the Qaidam basin is characterized by colder crust that may reflect an earlier stage in the channel injection process. In the study area, at least 10% of the eastward directed Tibetan crustal flow could be deflected northward across the Kunlun Fault and injected into the transition zone defining the northern margin of the Tibetan plateau.
Anisotropic low‐velocity lower crust beneath the northeastern margin ofTibetanPlateau: Evidence for crustal channel flow
Authors: Shen Xuzhang , Yuan Xiaohui , Ren Junsheng 
Published: November 2015

AbstractDetailed seismic structure in the crust beneath the northeastern margin of Tibetan Plateau was revealed by receiver functions of a regional permanent seismic network. At most stations, negative P‐to‐S converted phases can be detected in the radial receiver functions, prior to the Moho phases, indicating low velocities in the midlower crust. Prominent azimuthal variations in the transverse receiver functions with polarity reversal suggest azimuthal anisotropy in the crust. We used time variations of the P‐to‐S converted phases at the Moho in the radial receiver functions and the azimuth‐weighted stacking of transverse receiver functions to determine the fast direction and magnitude of anisotropy. The low‐velocity midlower crust with the coherent azimuthal anisotropy in the northeastern margin of Tibetan Plateau is consistent with the lower crustal channel flow model.
A hot flow anomaly at Mars
Authors: Collinson Glyn , Halekas Jasper , Grebowsky Joseph , Connerney Jack , Mitchell David , Espley Jared , DiBraccio Gina , Mazelle Christian , Sauvaud Jean‐André , Fedorov Andrei , Jakosky Bruce 
Published: November 2015

AbstractOne of the most important modes of planet/solar wind interaction are “foreshock transients” such as hot flow anomalies (HFAs). Here we present early observations by the NASA Mars Atmosphere and Volatile EvolutioN spacecraft, confirming their presence at Mars and for the first time at an unmagnetized planet revealing the underlying ion perturbations that drive the phenomenon, finding them to be weaker than at magnetized planets. Analysis revealed the HFA to be virtually microscopic: the smallest on record at ∼2200 km across and commensurate with the local proton gyroradius, resulting in a much stronger perturbation in solar wind protons than alpha particles. As at Venus, despite being physically diminutive, the HFA is still large (0.66 RM) when compared to the relative size of the induced magnetosphere. Given the associated order of magnitude decrease in solar wind dynamic pressure (411 pPa
70 pPa), we find that HFAs at Mars have the potential to directly impact the topside ionosphere. We thus hypothesize that the loss of a planetary magnetic dynamo left Mars far more vulnerable to the pressure pulses resulting from HFAs and related foreshock transients.
Electric Mars: The first direct measurement of an upper limit for the Martian “polar wind” electric potential
Authors: Collinson Glyn , Mitchell David , Glocer Alex , Grebowsky Joseph , Peterson W. K. , Connerney Jack , Andersson Laila , Espley Jared , Mazelle Christian , Sauvaud Jean‐André , Fedorov Andrei , Ma Yingjuan , Bougher Steven , Lillis Robert , Ergun Robert , Jakosky Bruce 
Published: November 2015

AbstractAn important mechanism in the generation of polar wind outflow is the ambipolar electric potential which assists ions in overcoming gravity and is a key mechanism for Terrestrial ionospheric escape. At Mars, open field lines are not confined to the poles, and outflow of ionospheric electrons is observed far into the tail. It has thus been hypothesized that a similar electric potential may be present at Mars, contributing to global ionospheric loss. However, no direct measurements of this potential have been made. In this pilot study, we examine photoelectron spectra measured by the Solar Wind Electron Analyzer instrument on the NASA Mars Atmosphere and Volatile EvolutioN (MAVEN) Mars Scout to put an initial upper bound on the total potential drop in the ionosphere of Mars of
, with the possibility of a further
4.5 V potential drop above this in the magnetotail. If the total potential drop was close to the upper limit, then strong outflows of major ionospheric species (H+, O+, and
) would be expected. However, if most of the potential drop is confined below the spacecraft, as expected by current theory, then such a potential would not be sufficient on its own to accelerate
to escape velocities, but would be sufficient for lighter ions. However, any potential would contribute to atmospheric loss through the enhancement of Jeans escape.
Magnetotail dynamics at Mars: Initial MAVEN observations
Authors: DiBraccio Gina A. , Espley Jared. R. , Gruesbeck Jacob R. , Connerney John E. P. , Brain David A. , Halekas Jasper S. , Mitchell David L. , McFadden James P. , Harada Yuki , Livi Roberto , Collinson Glyn , Hara Takuya , Mazelle Christian , Jakosky Bruce M. 
Published: November 2015

AbstractWe report on the complex nature of the induced Martian magnetotail using simultaneous magnetic field and plasma measurements from the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft. Two case studies are analyzed from which we identify (1) repetitive loading and unloading of tail magnetic flux as the field magnitude changes dramatically, exhibiting signatures similar to substorm activity within intrinsic magnetospheres; (2) multiple current sheet crossings indicative of plasma sheet flapping; (3) tailward flowing high‐energy planetary ions (O+ and O2+), confined exclusively to the cross‐tail current sheet, contributing to atmospheric escape; and (4) signatures of magnetic flux ropes, suggesting the occurrence of tail reconnection. These events illustrate the complexity of the Martian magnetotail as MAVEN provides key observations relevant to the unanswered questions of induced magnetosphere dynamics.
Three‐dimensional structure in the Mars H corona revealed by IUVS on MAVEN
Authors: Chaffin M. S. , Chaufray J. Y. , Deighan J. , Schneider N. M. , McClintock W. E. , Stewart A. I. F. , Thiemann E. , Clarke J. T. , Holsclaw G. M. , Jain S. K. , Crismani M. M. J. , Stiepen A. , Montmessin F. , Eparvier F. G. , Chamberlain P. C. , Jakosky B. M. 
Published: November 2015

AbstractLoss of water to space via neutral hydrogen escape has been an important process throughout Martian history. Contemporary loss rates can be constrained through observations of the extended neutral hydrogen atmosphere of Mars in scattered sunlight at 121.6 nm. Historically, such observations have been interpreted with coupled density and radiative transfer models, inferring escape fluxes from brightness profiles gathered by flybys, orbiters, and telescope observations. Here we demonstrate that the spherical symmetry assumed by prior analyses cannot reproduce observations by the Imaging Ultraviolet Spectrograph (IUVS) on the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. We present unique observations of the Mars H corona to large radial distances and mapping results from initial MAVEN science at Mars. These observations represent the first detection of three‐dimensional structure in the H corona of Mars, with implications for understanding the atmosphere today and the loss of H to space throughout Martian history.
Response of Mars O+ pickup ions to the 8 March 2015 ICME: Inferences from MAVEN data‐based models
Authors: Curry S. M. , Luhmann J. G. , Ma Y. J. , Dong C. F. , Brain D. , Leblanc F. , Modolo R. , Dong Y. , McFadden J. , Halekas J. , Connerney J. , Espley J. , Hara T. , Harada Y. , Lee C. , Fang X. , Jakosky B. 
Published: November 2015

AbstractWe simulate and compare three phases of the Mars‐solar wind interaction with the 8 March interplanetary coronal mass ejection (ICME) event using Mars Atmosphere and Volatile EvolutioN (MAVEN) mission observations in order to derive heavy ion precipitation and escape rates. The MAVEN observations provide the initial conditions for three steady state MHD model cases, which reproduce the observed features in the solar wind density, velocity, and magnetic field seen along the MAVEN orbit. Applying the MHD results to a kinetic test particle model, we simulate global precipitation and escape maps of O+ during the (1) pre‐ICME phase, (2) sheath phase, and (3) ejecta phase. We find that the Case 1 had the lowest precipitation and escape rates of 9.5 × 1025 and 4.1 × 1025 s−1, Case 2 had the highest rates of 9.5 × 1025 and 4.1 × 1025 s−1, and Case 3 had rates of 3.2 × 1025 and 1.3 × 1025 s−1, respectively. Additionally, Case 2 produced a high‐energy escaping plume >10 keV, which mirrored corresponding STATIC observations.
Water and water ions in the Martian thermosphere/ionosphere
Authors: Fox Jane L. , Benna M. , Mahaffy P. R. , Jakosky B. M. 
Published: November 2015

AbstractFirst results from the Neutral Gas and Ion Mass Spectrometer instrument on the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft reveal density profiles of protonated species that are mostly in good qualitative agreement with recent models of the Martian thermosphere/ionosphere. We present here the first photochemical model in which the density profiles of water and water ions in the ionosphere/thermosphere are predicted. We find that the computed peak densities of OH+, H2O+, and H3O+ are in fairly good agreement with the measured values. The computed column density of water is predicted to be about 1010 cm−2, and the mixing ratio at 80 km is 0.4 ppb. The actual water densities must be small enough so that HCO+ is not destroyed by proton transfer to water during the daytime and large enough so that H3O+ dominates the ionosphere at low altitudes just beyond the terminator. The calculations also show that the mass‐2 ion is almost certainly H
.
First measurements of composition and dynamics of the Martian ionosphere by MAVEN's Neutral Gas and Ion Mass Spectrometer
Authors: Benna M. , Mahaffy P. R. , Grebowsky J. M. , Fox J. L. , Yelle R. V. , Jakosky B. M. 
Published: November 2015

AbstractWe report the results of the observations of the ionosphere of Mars by the Neutral Gas and Ion Mass Spectrometer. These observations were conducted during the first 8 months of the Mars Atmosphere and Volatile EvolutioN mission (MAVEN). These observations revealed the spatial and temporal structures in the density distributions of 22 ions: H2+, H3+, He+, O2+, C+, CH+, N+, NH+, O+, OH+, H2O+, H3O+, N2+/CO+, HCO+/HOC+/N2H+, NO+, HNO+, O2+, HO2+, Ar+, ArH+, CO2+, and OCOH+. Dusk/dawn and day/night asymmetries in the density distributions were observed for nearly all ion species. Additionally, high‐density fluctuations were detected on the nightside and may reflect the effect of the partial screening of the atmosphere of Mars by the weak intrinsic magnetic field of the planet. The two first MAVEN “deep dip” campaigns were used to investigate the location of the primary ion peak. This peak was detected at 190 km near the terminator but was below the spacecraft altitude of 130 km near the subsolar point.
Dissolved inorganic carbon budgets in the eastern subpolar North Atlantic in the 2000s from in situ data
Authors: Zunino Patricia , Lherminier Pascale , Mercier Herlé , Padín Xose A. , Ríos Aida F. , Pérez Fiz F. 
Published: November 2015

AbstractThe subpolar North Atlantic (SPNA) is important in the global carbon cycle because of the deep water ventilation processes that lead to both high uptake of atmospheric CO2 and large inventories of anthropogenic CO2 (Cant). Thus, it is crucial to understand its response to increasing anthropogenic pressures. In this work, the budgets of dissolved inorganic carbon (DIC), Cant and natural DIC (DICnat) in the eastern SPNA in the 2000s, are jointly analyzed using in situ data. The DICnat budget is found to be in steady state, confirming a long‐standing hypothesis from in situ data for the first time. The biological activity is driving the uptake of natural CO2 from the atmosphere. The Cant increase in the ocean is solely responsible of the DIC storage rate which is explained by advection of Cant from the subtropics (65%) and Cant air‐sea flux (35%). These results demonstrate that the Cant is accumulating in the SPNA without affecting the natural carbon cycle.
Nonmigrating tides in the Martian atmosphere as observed by MAVEN IUVS
Authors: Lo Daniel Y. , Yelle Roger V. , Schneider Nicholas M. , Jain Sonal K. , Stewart A. Ian F. , England Scott L. , Deighan Justin I. , Stiepen Arnaud , Evans J. Scott , Stevens Michael H. , Chaffin Michael S. , Crismani Matteo M. J. , McClintock William E. , Clarke John T. , Holsclaw Gregory M. , Lefèvre Franck , Jakosky Bruce M. 
Published: November 2015

AbstractUsing the Mars Atmospheric and Volatile EvolutioN mission (MAVEN) Imaging Ultraviolet Spectrograph (IUVS), we found periodic longitudinal variations in CO2 density in the Martian atmosphere. These density variations are derived from observations of the
(
) emission from limb scans in the 100–190 km altitude range. The variations exhibit significant structure with longitudinal wave numbers 1, 2, and 3 in an effectively constant local solar time frame, and we attribute this structure to nonmigrating tides. The wave‐2 component is dominated by the diurnal eastward moving DE1 tide at the equator and the semidiurnal stationary S0 tide at the midlatitudes. Wave‐3 is dominated by the diurnal eastward moving DE2 tide, with possibly the semidiurnal eastward moving SE1 tide causing an amplitude increase at the midlatitudes. Structure in the wave‐1 component can be explained by the semidiurnal westward moving SW1 tide.