bluuebunny/crossref_metadata_2025_split huggingface dataset:
Region-Specific and Weather-Dependent Characteristics of the Relation between GNSS-Weighted Mean Temperature and Surface Temperature over China
Authors: Wang Minghua , Chen Junping , Han Jie , Zhang Yize , Fan Mengtian , Yu Miao , Sun Chengzhi , Xie Tao 
Published: March 2023

Weighted mean temperature of the atmosphere, Tm, is a key parameter for retrieving the precipitable water vapor from Global Navigation Satellite System observations. It is commonly estimated by a linear model that relates to surface temperature Ts. However, the linear relationship between Tm and Ts is associated with geographic regions and affected by the weather. To better estimate the Tm over China, we analyzed the region-specific and weather-dependent characteristics of this linear relationship using 860,054 radiosonde profiles from 88 Chinese stations between 2005 and 2018. The slope coefficients of site-specific linear models are 0.35~0.95, which generally reduce from northeast to southwest. Over southwest China, the slope coefficient changes drastically, while over the northwest, it shows little variation. We developed a Ts∼Tm linear model using the data from rainless days as well as a model using the data from rainy days for each station. At half the stations, mostly located in west and north China, the differences between the rainy-day and rainless-day Tm models are significant and larger than 0.5% (1%) in mean (maximal) relative bias. The regression precisions of the rainy-day models are higher than that of the rainless-day models averagely by 28% for the stations. Radiosonde data satisfying Tm−Ts>10 K and Ts−Tm>30 K most deviate from linear regression models. Results suggest that the former situation is related to low surface temperature (<270 K), as well as striking temperature and humidity inversions below 800 hPa, while the latter situation is related to high surface temperature (>280 K) and a distinct humidity inversion above 600 hPa.
Prescribed Performance Control-Based Semi-Active Vibration Controller for Seat Suspension Equipped with an Electromagnetic Damper
Authors: Zhao Junjie , Liu Pengfei , Leng Dingxin , Zhan Haoyu , Luan Guangrui , Ning Donghong , Yu Jianqiang 
Published: March 2023

Seat suspension plays a vital role in improving riding comfort and protecting drivers’ health. This paper develops semi-active seat suspension that equips a controllable electromagnetic damper (EMD) and proposes a prescribed performance control-based semi-active vibration controller with experimental validation. The semi-active EMD mainly consists of a permanent magnet synchronous motor, a ball screw, a three-phase rectifier, and a controllable external resistor, which can vary its damping from 90 to 800 N·s/m by tuning the controllable external resistor in real-time. The EMD is applied to seat suspension, and a semi-active controller is proposed for the EMD seat suspension. In order to control the seat suspension vibration, a prescribed performance method is applied to obtain a desired control force and then a force-tracking strategy is designed to make the EMD track the desired control force. Finally, the semi-active seat suspension with the proposed controller is tested in experiments with different vibration conditions. The semi-active seat suspension performs excellently for the bump, sine wave and random vibration. The root mean square (RMS) acceleration, the frequency-weighted RMS acceleration and the acceleration’s fourth power vibration dose value were reduced by 17.5%, 39.9%, and 25.4%, respectively, in the random vibration, compared with a passive system.
e-beam metrology of thin resist for high NA EUVL
Authors: Lorusso Gian Francesco , De Simone Danilo , Zidan Mohamed , Severi Joren , Moussa Alain , Dey Bappaditya , Halder Sandip , Goldenshtein Alex , Houchens Kevin , Santoro Gaetano , Fischer Daniel , Muellender Angelika , Mack Chris , Kondo Tsuyoshi , Shohjoh Tomoyasu , Ikota Masami , Charley Anne-Laure , De Gendt Stefan , Leray Philippe 
Published: March 2023

Abstract
One of the many constraints of high numerical aperture extreme ultraviolet lithography is related to resist thickness. A critical consequence of moving from the current 0.33 to 0.55 NA (high NA) is depth of focus reduction. The question we seek to answer in the present study is how the resist thickness reduction, required to compensate for the drop in NA, impacts the e-beam metrology needed to characterize the process. The impact of film thickness on e-beam metrology was first investigated by critical dimension scanning electron microscopy (CD SEM) using our current best-known methods (BKMs). Optimized settings minimizing such an impact were then studied using CD SEM as well as low-voltage SEM. Atomic force microscopy was used to accurately characterize the sample thickness. Our results indicate that alternative operating conditions and BKMs are sometimes needed to meet the metrology requirements. However, even in the case of materials showing a large sensitivity to resist thinning, we were able to identify e-beam imaging conditions capable of meeting metrology specifications.
Design guides for artificial photosynthetic devices consisting of voltage-matched perovskite/silicon tandem solar-cell modules and electrochemical reactor modules
Authors: Takeda Yasuhiko , Yamanaka Ken-ichi , Morikawa Takeshi , Kato Naohiko 
Published: March 2023

Abstract
We clarified the design guides for H2- and CO-producing artificial photosynthetic devices. The combination of a voltage-matched (VM) tandem solar-cell (SC) module and an electrochemical (EC) module was adopted. The parallel-connected top and bottom SC modules, in which multiple organic–inorganic hybrid perovskite (PVK) SCs with a bandgap of 1.7 eV and crystalline-silicon SCs were connected in series, respectively, powered the EC module consisting of series-connected multiple EC reactors. It was found that the design parameters of the series connection numbers must be optimized under slightly greater solar intensity and higher temperature than the average values to minimize the mismatch between the device operating voltage and SC maximal power voltage. This is in contrast to that the annual electricity production of the VM SC module coupled with a power conditioner is not sensitive to the optimization conditions. Increases in the bandgaps of the PVK SCs do not affect the annual production significantly.
High-order mode solid mounted resonators with polarity inverted multilayered GeAlN/AlN films
Authors: Sekimoto Jun , Suzuki Masashi , Kakio Shoji 
Published: March 2023

Abstract
High frequency bulk acoustic wave (BAW) resonators for beyond 5 G communications have low Q values and electromechanical coupling because of their ultra-thin piezoelectric monolayer films. Polarity inverted multilayered film BAW resonators operating in high-order mode resonance can have thicker piezoelectric layers than monolayer BAW resonators. In this paper, we fabricated and evaluated two- to four-layered polarity inverted GeAlN/AlN film solid mounted resonators (SMRs). They resonated in high-order mode. Their total film thicknesses were approximately two- to four-times thicker than that of a monolayer AlN film SMR. The polarity inverted GeAlN/AlN film SMRs had higher Q values than the monolayer SMR.
The Effect of Trauma Mechanism on the Frequency of Accompanying Vertebral Fracture in Cases with Thoracic Trauma
Authors: ÖZTOK TEKTEN Beliz , YAKŞİ Osman 
Published: March 2023

Introduction: Thoracic traumas are the third most common trauma among all trauma cases after head-neck and extremity traumas. The most common causes are motor vehicle accidents, falls from height, gunshot wounds, and stab wounds. In our study, it was aimed to investigate the mechanism of trauma and its effect on the frequency of accompanying vertebral fracture in patients who applied to the emergency department of a university hospital due to thoracic trauma.
Material – Method: Our study was planned retrospectively. The information of the patients who applied to the emergency department of our hospital between 01.01.2017 and 01.01.2021 due to thoracic trauma was examined. Demographic characteristics of the patients, mechanism of trauma, trauma-related thoracic injuries and accompanying vertebral fractures were evaluated.
Results: The data of 515 patients exposed to thoracic trauma were analyzed. The median age of the patients included in the study was 52 and 72.4% (n: 373) were male. 96.3% (n: 496) of the patients presented because of blunt trauma. The most common trauma mechanisms were in-vehicle traffic accident (46.6% n:240) and falling from height (30.9% n:159).
Pneumothorax was found in 34.7% (n: 179) of the patients, hemothorax in 40.2% (n: 207), and costal fracture in 81.9% (n: 422). The frequency of concomitant vertebral fracture was 33.98% (n: 175). Vertebral fractures were most commonly detected in the lumbar region (53.1%) and were most common in patients admitted after a non-vehicle traffic accident. A significant difference was found between the mechanism of trauma and accompanying vertebral fracture; vertebral fracture was seen in 53.8% (n:28) of the patients who applied after a non-vehicle traffic accident. (p=0.004)
Conclusion: It should be kept in mind that the trauma mechanism may increase the frequency of accompanying vertebral fracture in patients admitted to the emergency department after blunt trauma and evaluated for thoracic trauma.
Examining the Rotation Period Distribution of the 40 Myr Tucana–Horologium Association with TESS
Authors: Popinchalk Mark , Faherty Jacqueline K. , Curtis Jason L. , Gagné Jonathan , Bardalez Gagliuffi Daniella C. , Vos Johanna M. , Ayala Andrew , Gonzales Lisseth , Kiman Rocio 
Published: March 2023

Abstract
The Tucana–Horologium association (Tuc-Hor) is a 40 Myr old moving group in the southern sky. In this work, we measure the rotation periods of 313 Tuc-Hor objects with TESS light curves derived from TESS full-frame images and membership lists driven by Gaia EDR3 kinematics and known youth indicators. We recover a period for 81.4% of the sample and report 255 rotation periods for Tuc-Hor objects. From these objects we identify 11 candidate binaries based on multiple periodic signals or outlier Gaia DR2 and EDR3 renormalized unit weight error values. We also identify three new complex rotators (rapidly rotating M dwarf objects with intricate light-curve morphology) within our sample. Along with the six previously known complex rotators that belong to Tuc-Hor, we compare their light-curve morphology between TESS Cycle 1 and Cycle 3 and find that they change substantially. Furthermore, we provide context for the entire Tuc-Hor rotation sample by describing the rotation period distributions alongside other youth indicators such as Hα and Li equivalent width, as well as near-ultraviolet and X-ray flux. We find that measuring rotation periods with TESS is a fast and effective means to confirm members in young moving groups.
The First Flight of the Marshall Grazing Incidence X-Ray Spectrometer (MaGIXS)
Authors: Savage Sabrina L. , Winebarger Amy R. , Kobayashi Ken , Athiray P. S. , Beabout Dyana , Golub Leon , Walsh Robert W. , Beabout Brent , Bradshaw Stephen , Bruccoleri Alexander R. , Champey Patrick R. , Cheimets Peter , Cirtain Jonathan , DeLuca Edward E. , Del Zanna Giulio , Dudík Jaroslav , Guillory Anthony , Haight Harlan , Heilmann Ralf K. , Hertz Edward , Hogue William , Kegley Jeffery , Kolodziejczak Jeffery , Madsen Chad , Mason Helen , McKenzie David E. , Ranganathan Jagan , Reeves Katharine K. , Robertson Bryan , Schattenburg Mark L. , Scholvin Jorg , Siler Richard , Testa Paola , Vigil Genevieve D. , Warren Harry P. , Watkinson Benjamin , Weddendorf Bruce , Wright Ernest 
Published: March 2023

Abstract
The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) sounding rocket experiment launched on 2021 July 30 from the White Sands Missile Range in New Mexico. MaGIXS is a unique solar observing telescope developed to capture X-ray spectral images of coronal active regions in the 6–24 Å wavelength range. Its novel design takes advantage of recent technological advances related to fabricating and optimizing X-ray optical systems, as well as breakthroughs in inversion methodologies necessary to create spectrally pure maps from overlapping spectral images. MaGIXS is the first instrument of its kind to provide spatially resolved soft X-ray spectra across a wide field of view. The plasma diagnostics available in this spectral regime make this instrument a powerful tool for probing solar coronal heating. This paper presents details from the first MaGIXS flight, the captured observations, the data processing and inversion techniques, and the first science results.
Unified Picture of the Local Interstellar Magnetic Field from Voyager and IBEX
Authors: Rankin J. S. , McComas D. J. , Zirnstein E. J. , Burlaga L. F. , Heerikhuisen J. 
Published: March 2023

Abstract
Prior to the Voyagers’ heliopause crossings, models and the community expected the magnetic field to show major rotations across the boundary. Surprisingly, the field showed no significant change in direction from the heliospheric Parker Spiral at either Voyager location. Meanwhile, a major result from the IBEX mission is the derived magnitude and direction of the interstellar field far from the Sun (∼1000 au) beyond the influence of the heliosphere. Using a self-consistent model fit to IBEX ribbon data, Zirnstein et al. reported that this “pristine” local interstellar magnetic field has a magnitude of 0.293 nT and direction of 227° in ecliptic longitude and 34.°6 in ecliptic latitude. These values differ by 27% (51%) and 44° (12°) from what Voyager 1 (2) currently observes (as of ∼2022.75). While differences are to be expected as the field undrapes away from the heliosphere, the global structure of the draping across hundreds of astronimcal units has not been reconciled. This leads to several questions: How are these distinct sets of observations reconcilable? What is the interstellar magnetic field’s large-scale structure? How far out would a future mission need to go to sample the unperturbed field? Here, we show that if realistic errors are included for the difficult-to-calibrate radial field component, the measured transverse field is consistent with that predicted by IBEX, allowing us to answer these questions through a unified picture of the behavior of the local interstellar magnetic field from its draping around the heliopause to its unfolding into the pristine interstellar medium.
JWST Insight into a Lensed HST-dark Galaxy and Its Quiescent Companion at z = 2.58
Authors: Kokorev Vasily , Jin Shuowen , Magdis Georgios E. , Caputi Karina I. , Valentino Francesco , Dayal Pratika , Trebitsch Maxime , Brammer Gabriel , Fujimoto Seiji , Bauer Franz , Iani Edoardo , Kohno Kotaro , Sesé David Blánquez , Gómez-Guijarro Carlos , Rinaldi Pierluigi , Navarro-Carrera Rafael 
Published: March 2023

Abstract
Using the novel James Webb Space Telescope (JWST)/NIRCam observations in the A2744 field, we present a first spatially resolved overview of a Hubble Space Telescope (HST)-dark galaxy, spectroscopically confirmed at z = 2.58 with magnification μ ≈ 1.9. While being largely invisible at ∼1 μm with NIRCam, except for sparse clumpy substructures, the object is well detected and resolved in the long-wavelength bands with a spiral shape clearly visible in F277W. By combining ancillary Atacama Large Millimeter/submillimeter Array (ALMA) and Herschel data, we infer that this object is an edge-on dusty spiral with an intrinsic stellar mass log (M
*/M
⊙) ∼ 11.3 and a dust-obscured star formation rate ∼300 M
⊙ yr−1. A massive quiescent galaxy (log (M
*/M
⊙) ∼ 10.8) with tidal features lies 2.″0 away (r ∼ 9 kpc), at a consistent redshift as inferred by JWST photometry, indicating a potential major merger. The dusty spiral lies on the main sequence of star formation, and shows high dust attenuation in the optical (3 < A

V
< 4.5). In the far-infrared, its integrated dust spectral energy distribution is optically thick up to λ
0 ∼ 500 μm, further supporting the extremely dusty nature. Spatially resolved analysis of the HST-dark galaxy reveals a largely uniform A

V
∼ 4 area spanning ∼57 kpc2, which spatially matches to the ALMA 1 mm continuum emission. Accounting for the surface brightness dimming and the depths of current JWST surveys, unlensed analogs of the HST-dark galaxy at z > 4 would be only detectable in F356W and F444W in an UNCOVER-like survey, and become totally JWST-dark at z ∼ 6. This suggests that detecting highly attenuated galaxies in the Epoch of Reionization might be a challenging task for JWST.
On the Gamma-Ray Emission of the Andromeda Galaxy M31
Authors: Xing Yi , Wang Zhongxiang , Zheng Dong , Li Jie 
Published: March 2023

Abstract
Using the γ-ray data obtained with the Large Area Telescope on board the Fermi Gamma-ray Space Telescope (Fermi) for ∼14 yr, we examine the high-energy emission emanating from the center of the Andromeda galaxy M31. Different from previously reported results, which show a seemingly extended source, we instead find two individual point sources, one consistent with being at the center and one 0.°4 southeast of the center. The emission of the former is well described using a log-parabola model, similar to those of previous studies, and that of the latter can be fitted with a power law. We discuss the possible origins for the two sources. M31's central source, now consistent with being a point source, necessitates a revisit of its previously discussed originations with this new property taken into consideration, in particular those cosmic rays or dark matter scenarios involving extended source distributions. The SE source appears to have a projected distance of ∼6 kpc from M31's center, and the investigation is required as to whether it is a source locally associated with M31, or is instead a background extragalactic one.
How Teen Wolf’s transmasculine fans use online fandom to build community and representation
Authors: Page Ari 
Published: March 2023

When media are unable or unwilling to provide accurate trans representation, trans fans use online fan communities to create their own representation and invent entire worlds that transgressively diverge from the source. The transmasculine fans of Teen Wolf are exemplary of this phenomenon, revealing that the foundational work within the show offers a rich (though unsanctioned) basis for trans connection through lycanthropy, transformation, and queer masculinity. This article looks at the possibilities for projecting trans experiences onto fictionalized bodies in a way that is celebratory, euphoric, and reparative.
The Design and Implementation of a Novel Mental Health Literacy Educational Intervention Program in Gaelic Footballers
Authors: O’Keeffe Sinéad , Ní Chéilleachair Niamh , O’Hagan Anna Donnla , Campbell Mark , O’Connor Siobhán 
Published: March 2023

Context
Lack of education, stigma, and negative self-attitudes are key barriers to help-seeking in Gaelic footballers. With the prevalence of mental health issues in Gaelic footballers and the increased risk of experiencing mental health challenges after injury, mental health literacy (MHL) interventions are necessary.

Objectives
To design and implement a novel MHL educational intervention program in Gaelic footballers.

Design
Controlled laboratory study.

Setting
Online.

Patients or Other Participants
Elite and subelite Gaelic footballers divided into intervention (n = 70; age = 25.1 ± 4.5 years) and control (n = 75; age = 24.4 ± 6.0 years) groups. In the intervention group, 85 participants were recruited, but 15 dropped out after completing baseline measures.

Interventions
A novel educational intervention program, “GAA [Gaelic Athletic Association] and Mental Health—Injury and a Healthy Mind,” was designed to address the key components of MHL and was underpinned by the Theory of Planned Behavior and the Help-Seeking Model. The intervention was implemented online via a brief 25-minute presentation.

Main Outcome Measures
Measures of stigma, help-seeking attitudes, and MHL were completed by the intervention group at baseline, immediately after viewing the MHL program, and at 1 week and 1 month after the intervention. The control group completed the measures at similar time points.

Results
Stigma decreased, and attitudes toward help-seeking and MHL increased in the intervention group from baseline to after the intervention (P &lt; .05), with significant differences sustained at 1-week and 1-month follow-ups. Our results showed differences in stigma, attitudes, and MHL between groups across time points. Intervention participants provided positive feedback, and the program was appraised as informative.

Conclusions
Remote online delivery of a novel MHL educational program can effectively decrease mental health stigma, improve attitudes toward help-seeking, and increase the recognition and knowledge of mental health issues. Gaelic footballers with improved MHL may be better equipped to manage their mental health and cope with stressors, leading to improved mental health outcomes and overall mental well-being.
Sudden Hair “Felting” during Styling Procedure
Authors: Attia Enas A. S. 
Published: March 2023

ABSTRACT
Acute scalp hair “felting” is a rare acquired condition that presents with sudden severe twisting, entangling, and matting of scalp hair into a stiff tightly packed mass, in otherwise healthy individuals. In such conditions, the mechanism of hair matting is almost like the process of “felting” in wool and textile industry, where adjacent fibers are compacted together in a warm liquid medium. Herein, a case of acute hair “felting” during styling practice is discussed with the possible predisposing factors, prophylaxis, and treatment.
Impact of Acid (”Progressive Brush”) and Alkaline Straightening on the Hair Fiber
Authors: Velasco Maria Valéria Robles , de Sá-Dias Tânia Cristina , Dario Michelli Ferrera , Bedin Valcinir , Fileto Marjory Bernardes , de Oliveira Andressa Costa , Pinto Claudinéia Aparecida Sales de Oliveira , Baby André Rolim 
Published: March 2023

ABSTRACT

Background:
Glyoxylic acid has emerged as a safe alternative to formol (formaldehyde) use as a hair straightener/relaxer. However, the possible damage to the hair fiber after its application is low known and/or published in the literature.

Aims:
This work aims to characterize hair locks treated with glyoxylic acid compared to traditional alkaline straighteners such as sodium and guanidine hydroxide and ammonium thioglycolate.

Materials and Methods:
The morphology of the hair cuticles was observed by scanning electron microscopy. Protein loss was assessed by the Lowry method modified by Peterson and as mechanical properties that were expressed in terms of tensile strength.

Results:
All products (sodium and guanidine hydroxides and ammonium thioglycolate) caused protein loss of about 2.5 μg/g, except glyoxylic acid that caused the worst damage (3.5 μg/g), in relation to the untreated (virgin) hair (1.12 μg/g), indicating that the chemical treatments can cause hair damage in both cuticles and cortex. The force to break the fibers treated with traditional straighteners based on sodium hydroxide, guanidine hydroxide, and ammonium thioglycolate was statistically the same.

Conclusion:
The treatment with glyoxylic acid showed rupture tensile statistically equivalent to the alkaline straighteners. The mechanism of action of glyoxylic acid does not appear to be based on breaking and rearrangement of disulfide bridges, but altered them, that influenced the hair strength. However, it is also essential to consider other factors relevant: technical application technique, reaction time, and interval of reapplication of the product, as this can change the pattern of the results obtained.