bluuebunny/crossref_metadata_2025_split huggingface dataset:
Natural language processing in-and-for design research
Authors: Siddharth L. , Blessing Lucienne , Luo Jianxi 
Published: August 2022

AbstractWe review the scholarly contributions that utilise natural language processing (NLP) techniques to support the design process. Using a heuristic approach, we gathered 223 articles that are published in 32 journals within the period 1991–present. We present state-of-the-art NLP in-and-for design research by reviewing these articles according to the type of natural language text sources: internal reports, design concepts, discourse transcripts, technical publications, consumer opinions and others. Upon summarising and identifying the gaps in these contributions, we utilise an existing design innovation framework to identify the applications that are currently being supported by NLP. We then propose a few methodological and theoretical directions for future NLP in-and-for design research.
Using ground-based thermal imagery to estimate debris thickness over glacial ice: fieldwork considerations to improve the effectiveness
Authors: Aubry-Wake Caroline , Lamontagne-Hallé Pierrick , Baraër Michel , McKenzie Jeffrey M. , Pomeroy John W. 
Published: August 2022

AbstractDebris-covered glaciers are an important component of the mountain cryosphere and influence the hydrological contribution of glacierized basins to downstream rivers. This study examines the potential to make estimates of debris thickness, a critical variable to calculate the sub-debris melt, using ground-based thermal infrared radiometry (TIR) images. Over four days in August 2019, a ground-based, time-lapse TIR digital imaging radiometer recorded sequential thermal imagery of a debris-covered region of Peyto Glacier, Canadian Rockies, in conjunction with 44 manual excavations of debris thickness ranging from 10 to 110 cm, and concurrent meteorological observations. Inferring the correlation between measured debris thickness and TIR surface temperature as a base, the effectiveness of linear and exponential regression models for debris thickness estimation from surface temperature was explored. Optimal model performance (R2 of 0.7, RMSE of 10.3 cm) was obtained with a linear model applied to measurements taken on clear nights just before sunrise, but strong model performances were also obtained under complete cloud cover during daytime or nighttime with an exponential model. This work presents insights into the use of surface temperature and TIR observations to estimate debris thickness and gain knowledge of the state of debris-covered glacial ice and its potential hydrological contribution.
Participation and Objectivity
Authors: Koskinen Inkeri 
Published: August 2022

AbstractMany philosophers of science have recently argued that extra-academic participation in scientific knowledge production does not threaten scientific objectivity. Quite the contrary: Citizen science, participatory projects, transdisciplinary research, and other similar endeavours can even increase the objectivity of the research conducted. Simultaneously, researchers working in fields in which such participation is common have expressed worries about various ways in which it can result in biases. In this article I clarify how these arguments and worries can be compared, and how extra-academic participation can both increase and threaten the objectivity of the research conducted.
Validity and reliability of the Turkish version of the Sustainable and Healthy Eating Behaviors Scale
Authors: Köksal Eda , Bilici Saniye , Çıtar Dazıroğlu Merve Esra , Erdoğan Gövez Nazlıcan 
Published: August 2022

AbstractThis study was conducted to determine the validity and reliability of the Turkish version of the Sustainable and Healthy Eating (SHE) Behaviors Scale. The original scale included eight factors and thirty-four items related to the SHE behaviors of adults. The research was carried out in three stages with a total of 586 participants aged 19 to 50 years. The Cronbach alpha coefficient was used to evaluate internal consistency reliability and the test–retest method was applied. Exploratory factor analysis (EFA) was performed to determine the factor structure. The model obtained with EFA was evaluated with confirmatory factor analysis (CFA). The Cronbachαcoefficient of the scale was found to be excellent at 0·912, and the intra-class correlation coefficient was found to be good at 0·832 using the test–retest method. Considering the suitability of the data for factor analysis, the Kaiser–Meier–Olkin coefficient was 0·859, and the significance level of the Bartlett test of sphericity was less than 0·05 (χ2=3·803,25; P < 0·05). As a result of EFA, the items of the scale were found to be distributed in seven factor dimensions. The factor loadings of the items were between 0·516 and 0·890, and the factors explained 67 % of the variance. Considering the fit indices obtained as a result of the analysis of this model with CFA, it was seen that the model had an acceptable fit (χ2/sd = 2·593, comparative fit index = 0·915, Tucker–Lewis index=0·902, standardised root mean square error = 0·0754 and root mean square error of approximation = 0·067). In conclusion, the Turkish version of the SHE Behaviors Scale has credible reliability and construct validity to assess the sustainable and healthy eating behaviours of the Turkish adult population.
Lessons for International Small and Medium-Sized Enterprises from Counterfeiting Civil Litigations in China
Authors: Cai Chuanzi 
Published: August 2022

AbstractThis study aims to assess the effect of the 2013 trademark law revision (2013 law revision) on judicial remedies in China. The 2013 law revision increased the remedies Chinese courts can grant to plaintiffs, including small and medium enterprise (SME) plaintiffs, thus leading to higher remedies granted to plaintiffs compared to the past years in prevailing cases. This study finds that right after the law revision, the average amount of judicial remedies granted to plaintiffs increased temporarily. Meanwhile, the detailed judicial reasonings, foreign plaintiffs, and company defendants have stronger positive effects than product types and the year of decisions on the amount of monetary relief. These findings suggest that certain factors in cases may increase the remedies in trademark civil litigation. Therefore, SME plaintiffs should pay attention to core factors for litigation strategies, including preliminary injunctions, choice of defendant, choice of venue, and evidence in remedy collection.
The Role of Water Vapor in the Response of the Extratropical Circulation of Earth‐Like Planets to Obliquity Changes
Authors: Lobo Ana H. , Bordoni Simona 
Published: August 2022

AbstractIn this study, we use idealized aquaplanet simulations of Earth‐like planets to explore the large‐scale atmospheric circulation’s response to changes in shortwave radiation, through changes in the planet obliquity, and in longwave radiation, through changes in the prescribed optical depth. We primarily focus on the extratropical circulation and the counterintuitive weakening of extratropical eddy activity, and associated precipitating storm tracks, with increased obliquity. We show that on high‐obliquity planets with a small surface thermal inertia, net energy deficit during the winter months is primarily balanced by the latent energy component of the atmospheric heat capacity, which buffers any significant atmospheric cooling. As temperatures finally start to decrease, condensational latent heat release of atmospheric moisture further slows down the cooling and keeps the winter pole warmer than the midlatitudes until after the winter solstice. This prevents vigorous baroclinic eddy activity, which lives off the potential energy stored in the sloping isopycnals, as well as the development of a Ferrel cell and storm track. For planets with larger surface heat capacity, we see a similar suppression, with the energy storage in the ocean surface, rather than atmospheric latent energy storage, primarily balancing the net energy loss during the winter months. These results suggest that, regardless of surface thermal inertia, water‐covered high‐obliquity Earth‐like planets would not experience significant extratropical storm activity and highlight the need for a proper characterization of polar properties in planetary modeling and observational investigations.
Spectral Diversity of Rocks and Soils in Mastcam Observations Along the Curiosity Rover's Traverse in Gale Crater, Mars
Authors: Rice Melissa S. , Seeger Christina , Bell Jim , Calef Fred , St. Clair Michael , Eng Alivia , Fraeman Abigail A. , Hughes Cory , Horgan Briony , Jacob Samantha , Johnson Jeff , Kerner Hannah , Kinch Kjartan , Lemmon Mark , Million Chase , Starr Mason , Wellington Danika 
Published: August 2022

AbstractThe Mars Science Laboratory Curiosity rover has explored over 400 m of vertical stratigraphy within Gale crater to date. These fluvio‐deltaic, lacustrine, and aeolian strata have been well‐documented by Curiosity's in situ and remote science instruments, including the Mast Camera (Mastcam) pair of multispectral imagers. Mastcam visible to near‐infrared spectra can broadly distinguish between iron phases and oxidation states, and in combination with chemical data from other instruments, Mastcam spectra can help constrain mineralogy, depositional origin, and diagenesis. However, no traverse‐scale analysis of Mastcam multispectral data has yet been performed. We compiled a database of Mastcam spectra from >600 multispectral observations and quantified spectral variations across Curiosity's traverse through Vera Rubin ridge (sols 0–2302). From principal component analysis and an examination of spectral parameters, we identified nine rock spectral classes and five soil spectral classes. Rock classes are dominated by spectral differences attributed to hematite and other oxides (due to variations in grain size, composition, and abundance) and are mostly confined to specific stratigraphic members. Soil classes fall along a mixing line between soil spectra dominated by fine‐grained Fe‐oxides and those dominated by olivine‐bearing sands. By comparing trends in soil versus rock spectra, we find that locally derived sediments are not significantly contributing to the spectra of soils. Rather, varying contributions of dark, mafic sands from the active Bagnold Dune field is the primary spectral characteristic of soils. These spectral classes and their trends with stratigraphy provide a basis for comparison in Curiosity's ongoing exploration of Gale crater.
Stability Analysis of Submerged Vegetation Patterns in Rivers
Authors: Calvani G. , Carbonari C. , Solari L. 
Published: August 2022

AbstractAquatic vegetation in fluvial systems is often characterized by spatial patterning of the plant patches. To investigate the conditions for the formation of vegetation patches, we explore the stability of a uniform flow over a non‐erodible bed with a uniform vegetation cover of submerged plants. The flow model consists of the two‐dimensional shallow water and continuity equations. The hydrodynamic equations are coupled firstly to the classic formulation for vegetation dynamics, and secondly to a modified version of the equation. The revised relationship for vegetation dynamics accounts for the influence of removal, transport, and resettlement of propagules on the growth rate of aquatic vegetation. Linear stability analysis of the eco‐hydrodynamic problem is performed by enforcing the quasi‐steady approximation. We obtain a dispersion relation disclosing the growth rate and the migration rate of the perturbations of vegetation density as a function of the wavenumber and the relevant flow and vegetation parameters. The present theory predicts the onset of vegetation patterns and includes an adequate wavelength selection mechanism. While uprooting initially reduces plant density, the analysis demonstrates that resettled propagules after removal are fundamental for further plant population increases and the development of vegetation patterns. The proposed framework is then validated against data available in the literature. Additionally, the presence of an upper threshold in terms of vegetation density, above which uniform vegetation cover is stable, might explain the absence of any spatial pattern and thus the extremely dense vegetation cover induced by climate change and invasive species in altered ecosystems.
Simulation of Latent Heating Rate From the Microphysical Process Associated With Mesoscale Convective System Over Korean Peninsula
Authors: Madhulatha A. , Dudhia Jimy , Park Rae‐Seol , Rajeevan M. 
Published: August 2022

AbstractTo investigate the structure of latent heating rate during different stages of mesoscale convective system (MCS) over the Korean Peninsula, a four nested domain Weather Research and Forecasting (WRF) model simulation with two‐way nesting method has performed. Advanced physics options from the Korean Integrated model physics are considered for simulation. Latent heating rate associated with condensation, evaporation, deposition, sublimation, freezing and melting process is computed based on different microphysical process using WRF double moment (WDM6) microphysics scheme. During the development/mature stage of the convective system, the warming associated with latent heat release by condensation is dominant below 400 hPa, and deposition above 500 hPa. The maximum contribution of warming processes from condensation, cloud nucleation, graupel accretion, and ice, snow deposition is evident. Cooling processes from rain, cloud evaporation followed by graupel, and snow melting are also noticed. Major updrafts associated with ascent of air parcel and large hydrometeor distribution is apparent along with downdrafts in the lower levels. In the dissipating stage, the cooling due to latent heat absorption by evaporation below 600 hPa and melting around 600 hPa are dominant. Contribution from cooling processes is dominant with major downdraft motion in the lower levels corresponding to the hydrometeor fall velocity. Dominant positive (negative) total latent heating provided (restrained) the energy for convection during developing and dissipating stages of system. Varied distribution of total cloud hydrometeors in different stages is apparent. Consistency between cloud hydrometeors, net heating rates, major upward (downward) motion and corresponding rainfall in developing (dissipating) stages of MCS is noticed. Model simulated latent heating (WDM6) profiles are consistent with computed moisture source and sink terms (ERA5).
Traveling Ionospheric Disturbances in the Vicinity of Storm‐Enhanced Density at Midlatitudes
Authors: Zhang Shun‐Rong , Nishimura Yukitoshi , Erickson Philip J. , Aa Ercha , Kil Hyosub , Deng Yue , Thomas Evan G. , Rideout William , Coster Anthea J. , Kerr Robert , Vierinen Juha 
Published: August 2022

AbstractThis study provides first storm time observations of the westward‐propagating medium‐scale traveling ionospheric disturbances (MSTIDs), particularly, associated with characteristic subauroral storm time features, storm‐enhanced density (SED), subauroral polarization stream (SAPS), and enhanced thermospheric westward winds over the continental US. In the four recent (2017–2019) geomagnetic storm cases examined in this study (i.e., 2018‐08‐25/26, 2017‐09‐07/08, 2017‐05‐27/28, and 2016‐02‐02/03 with minimum SYM‐H index −206, −146, −142, and −58 nT, respectively), MSTIDs were observed from dusk‐to‐midnight local times predominately during the intervals of interplanetary magnetic field (IMF) Bz stably southward. Multiple wavefronts of the TIDs were elongated NW‐SE, 2°–3° longitude apart, and southwestward propagated at a range of zonal phase speeds between 100 and 300 m/s. These TIDs initiated in the northeastern US and intensified or developed in the central US with either the coincident SED structure (especially the SED basis region) or concurrent small electron density patches adjacent to the SED. Observations also indicate coincident intense storm time electric fields associated with the magnetosphere–ionosphere–thermosphere coupling electrodynamics at subauroral latitudes (such as SAPS) as well as enhanced thermospheric westward winds. We speculate that these electric fields trigger plasma instability (with large growth rates) and MSTIDs. These electrified MSTIDs propagated westward along with the background westward ion flow which resulted from the disturbance westward wind dynamo and/or SAPS.
Plasmoids in the Jovian Magnetotail: Statistical Survey of Ion Acceleration Using Juno Observations
Authors: Blöcker A. , Kronberg E. A. , Grigorenko E. E. , Clark G. , Vogt M. F. , Roussos E. 
Published: August 2022

AbstractTransient magnetic reconnection plays an important role in energetic particle acceleration in planetary magnetospheres. Jupiter's magnetosphere provides a unique natural laboratory to study processes of energy transport and transformation. Strong electric fields in spatially confined structures such as plasmoids can be responsible for ion acceleration to high energies. In this study we focus on the effectiveness of ion energization and acceleration in plasmoids. Therefore, we present a statistical study of plasmoid structures in the predawn magnetotail, which were identified in the magnetometer data of the Juno spacecraft from 2016 to 2018. We additionally use the energetic particle observations from the Jupiter Energetic Particle Detector Instrument which discriminates between different ion species. We are particularly interested in the analysis of the acceleration and energization of oxygen, sulfur, helium, and hydrogen ions. We investigate how the event properties, such as the radial distance and the local time of the observed plasmoids in the magnetotail, affect the ion intensities close to the current sheet center. Furthermore, we analyze if ion acceleration is influenced by magnetic field turbulence inside the plasmoids. We find significant heavy ion acceleration in plasmoids close to the current sheet center which is in line with the previous statistical results based on Galileo observations conducted by Kronberg et al. (2019, https://doi.org/10.1029/2019JA026553). The observed effectiveness of the acceleration is dependent on the position of Juno in the magnetotail during the plasmoid event observation. Our results show no correlation between magnetic field turbulence and nonadiabatic acceleration for heavy ions during plasmoids.
Desilicification Rims of Zircon Xenocrysts Record the Timing of Kimberlite Emplacement
Authors: Melnik Aleksey E. , Li Qiu‐Li , Korolev Nester M. , Li Jiao , Ling Xiao‐Xiao , Liu Yu , Tang Guo‐Qiang , Zinger Tatiana F. , Mao Qian , Wu Shi‐Tou , Xu Jing‐Yao , Li Xian‐Hua 
Published: August 2022

AbstractKimberlites are deep and relatively rare mantle‐derived igneous rocks, which provide key insights into the lithospheric mantle composition beneath continents (i.e., from the entrained mantle materials) at the time of magma emplacement. In addition, the temporal distribution of kimberlites throughout Earth's history may reveal secular changes in global geodynamics. However, alteration and abundant exotic material (i.e., xenoliths and xenocrysts) of different ages, both typical of kimberlites, often hinder reliable dating of these rocks. In this study, we investigated zircon xenocrysts and their replacement by desilicification reaction rims (DSRs), which consist mainly of baddeleyite, in the metamorphosed Kimozero kimberlites from the Karelian Craton, Russia. Similar DSRs have been identified previously on mantle‐derived zircons in numerous kimberlites, but the precise timing and location of formation of these rims remain unclear. U–Pb isotope dating of mantle zircon xenocrysts in the Kimozero kimberlites indicates that these rocks were emplaced at ca. 1.97 Ga. DSRs with similar textures and baddeleyite chemistry occur on both the 1.97 Ga mantle and 2.70–2.38 Ga crustal zircon xenocrysts in these kimberlites. Pb–Pb isotope dating of the DSRs yields the same age (i.e., ca. 1.97 Ga) as the mantle zircons. The data constrain the formation of DSRs to crustal levels and, more importantly, indicate that these rims record the timing of kimberlite emplacement. Therefore, we suggest that such baddeleyite reaction rims are a new and promising material for kimberlite geochronology.
Precursory Signals in the Stratospheric Meridional Mass Circulation for Mid‐Latitude Cold Air Outbreak Events of High and Low Sub‐Seasonal Predictability
Authors: Yu Yueyue , Liu Bowen , Ren Rongcai , Guan Zhaoyong , Yang Qinlan , Hu Muxin 
Published: August 2022

AbstractUsing the NCEP reforecast data (1999–2010) and NCEP's CFSv2 real‐time forecast data (2012–2019) from the S2S (Sub‐seasonal to Seasonal) project, we evaluated the sub‐seasonal skill by the CFSv2 model with respect to mid‐latitude cold air outbreak events (CAOs) in winter (November–February) and investigated the distinct features of the anomalies of surface temperature, stratospheric mass circulation, and wave activities between the top 11 “high‐skill” CAO events and the top 10 “low‐skill” events. Results show that the predictability limit tends to be longer for wide‐impact and long‐lasting CAOs occurred in Eurasia or both continents, but such tendency is not very robust. The model possesses a better sub‐seasonal skill when there is generally stronger and longer‐lasting equatorward cold air branch of isentropic meridional mass circulation, which is coupled with a stronger stratospheric poleward warm branch in the 3 weeks prior to the peak time of “high‐skill” CAOs. The largest contrast between “high‐skill” and “low‐skill” CAOs lies in the wavenumber‐1 component of stratospheric poleward warm branch. Both the amplitude in the middle stratosphere and vertically westward‐tilting of wavenumber‐1 waves in the lower stratosphere tend to be stronger (weaker) prior to “high‐skill” (“low‐skill”) CAOs, collaboratively contributing to the stronger (weaker) stratospheric poleward warm branch. The temporal evolution of intensity of stratospheric poleward warm branch, wave amplitude, and westward‐tilting are better captured by CFSv2 model at sub‐seasonal scale in the month before “high‐skill” CAOs. These results reveal the important role of stratosphere–troposphere connection in determining the windows of opportunity for skillful sub‐seasonal forecasts of CAOs.
Emulator For Eroded Beach And Dune Profiles Due To Storms
Authors: Gharagozlou A. , Anderson D. L. , Gorski J. F. , Dietrich J. C. 
Published: August 2022

AbstractDunes and beaches are vulnerable to erosion during storm events. Numerical models can predict beach response to storms with fidelity, but their computational costs, the domain‐specific knowledge necessary to use them, and the wide range of potential future storm and beach conditions can hinder their use in forecasting storm erosion for short‐ and long‐term horizons. We develop an emulator, which is an efficient predictive model that behaves like a numerical model, to predict the morphologic response of the subaerial beach to storms. Specific emphasis is placed on providing antecedent beach states as an input to the emulator and predicting the post‐storm profile shape. Training data include beach profiles at multiple stages in a nourishment life cycle to assess if such a framework can be applied in locations that nourish as a coastal defense policy. Development and application of the emulator is focused on Nags Head, North Carolina, which nourishes its beaches to mitigate hazards of storm waves, flooding, and erosion. A high‐fidelity, process‐based morphodynamic model is used to train the emulator with 1250 scenarios of sea‐storms and beach profiles. The post‐storm beach state is emulated with a parameterized power‐law function fit to the eroded portion of the subaerial profile. When the emulator was tested for a sequence of real storms from 2019, the eroded beach profiles were predicted with a skill score of 0.66. This emulator is promising for future efforts to predict storm‐induced beach erosion in hazard warnings or adaptation studies.