bluuebunny/crossref_metadata_2025_split huggingface dataset:
La esfera religiosa de la mujer romana: espacio público vs privado
Authors: Molina Torres María Pilar 
Published: June 2018

En estas páginas se da una visión general de cómo el espacio público y privado influyó en las formas de religiosidad de las mujeres romanas. Aunque las diferencias no son todo lo claras que nos gustarían, no hay que olvidar que una devota debía ser capaz de hacer todo lo necesario para conseguir la estabilidad religiosa oficial y doméstica. Las fuentes literarias, epigráficas y especialmente las arqueológicas de Pompeya, nos acercan a las prácticas rituales donde la presencia femenina aparece simbolizada iconográficamente. Asimismo, sus actuaciones religiosas en la esfera pública se reservaron a organizaciones matronales que tuvieron un papel decisivo en determinadas festividades del calendario romano.
Yaşlıların Mekân ve Mobilya Kullanımında Karşılaştıkları Sorunlar ve Çözüm Önerileri Analizi
Authors: ÖZTÜRK Ahmet Mustafa , ÇINAR Hamza , İŞLER Erhan 
Published: June 2018

Bilim ve teknolojik
gelişmeler sonucunda insan yaşamı uzamakta ve toplumda yaşlı nüfusu
artmaktadır. Ülkemizde yaşlı nüfusun hızla artması ve yaşam
sürecinin uzaması, yaşlı insanların
kendi yaşam mekânlarındaki şartların incelenerek iyileştirilmesi beklentisini
de arttırmaktadır. Bu görüşten yola çıkılarak bu çalışmada yaşlıların mekân ve
mobilya kullanımında karşılaştıkları sorunların belirlenmesi amaçlanmıştır.
Yaşlıların yaşadıkları mekânlarda ve kullandıkları mobilyalarda karşılaştıkları
problemleri tespit edilmesine yönelik hazırlanan anket, Giresun ilinde yaşları
65 ve üzerinde olan 73 kişiye uygulanmıştır. Çalışmadan elde edilen bulgular
yaşlıların mutfak, yatak odası, salon, çalışma odası, antre gibi iç mekan
alanlarında çok zorluk yaşamadıklarını banyo, tuvalet gibi alanlarda sıkıntı
yaşadıklarını göstermiştir. Ayrıca yaşlı bireylerin sosyal faaliyetleri
gerçekleştirirken büyük oranda zorlandığı gözlemlenmiştir. Çalışma sonucunda
yaşlıların yaşam alanlarını düzenlerken gerekli tedbirlerin alınması, evlerde
yaşlı bireylere yönelik iç mekân tasarımının yapılması, sosyal alanlarda yaşlı
bireylerin kolaylıkla kullanılabileceği tasarımlar geliştirilerek önlemler
alınması önerilmektedir.
Papatyadan (Matricaria chamomilla L.) Lipaz Enziminin Saflaştırılması ve Çeşitli Taşıyıcılara İmmobilize Edilmesi
Authors: Bilgin Sökmen Bahar , Sarı Burçak , Azap Tuğba 
Published: June 2018

Bu çalışmada, Giresun İli ve çevresinde bol miktarda
yetişen papatyadan (Matricaria chamomilla
L.) lipaz enzimi ilk defa
saflaştırıldı ve kinetik özellikleri incelendi. Lipaz
esteraz aktivitesi gösteren homojenizatın % 70’lik (NH4)2SO4
kesiti elde edildi. Dializden sonra bu kesit DEAE-selüloz kolonlara uygulanarak
lipaz enzimi 26 kat saflaştırıldı. Saflaştırma işlemlerinde protein miktarı
Lowry ve E280/E260 Warburg yöntemlerine göre, lipaz
esteraz aktivitesi ise Erlanson yöntemine göre tayin edildi. SDS-PAGE
elektroforezi ile elde edilen saflaştırılmış enzimin molekül ağırlığının 30 kDa
olduğu bulundu. Optimum pH ve sıcaklık değerleri belirlendi. Papatyadan
saflaştırılan lipazın optimum pH’sının 9, optimum sıcaklığının 50 °C olduğu
bulundu. Enzimin çeşitli substratlara karşı ilgisi incelendiğinde, lipazın
ilgisinin en çok p-nitrofenil palmitatta olduğu ve bu substrata karşı Km
ve Vmax değerlerinin sırasıyla 0,2899 mM ve 144,93 Ünite olduğu
saptandı.Ayrıca, papatyadan saflaştırılan lipaz enzimi çeşitli
taşıyıcılar üzerine
adsorpsiyon, kovalent ve iyonik bağlama yöntemleri ile immobilize edildi. İmmobilize
edilmiş papatya lipazının optimum pH, optimum sıcaklık gibi kinetik özellikleri
de incelendi.
The First Record of Two Moths (Lepidoptera) in Hatay Province of Turkey and External and Genital Morphology of The Species
Authors: ATAY Erol , HÜSEYİNOĞLU Yusuf , SLAMKA Frantisek , TATLI Mahmut 
Published: June 2018

This study was conducted in field and laboratory. Nemophora fascielle (Fabricius, 1775) (Adelidae) and Endothenia sororiana (Herrich-Schaffer, 1851) (Tortricidae) were caught with insect net, mercury vapour light trap and white screen, at different altitudes, with various vegetation in Hatay. In the field studies, N. fascielle totally 3 male and 2 female, and E. sororiana totally 5 male and 1 female were collected. Specimens were dissected in the laboratory and prepared male genitalia and wings slides. We described the external and male genital morphology of N. fascielle and E. sororiana in detail and also diagnostical morphological features. As a result of the study, N. fascielle and E. sororiana are first record for Hatay.
PATCHWORK: A Multipatch Infrastructure for Multiphysics/Multiscale/Multiframe Fluid Simulations
Authors: Shiokawa Hotaka , Cheng Roseanne M. , Noble Scott C. , Krolik Julian H. 
Published: June 2018

Abstract
We present a “multipatch” infrastructure for the numerical simulation of fluid problems in which subregions require different grid scales, different grid geometries, different physical equations, or different reference frames. Its key element is a sophisticated client–router–server framework for efficiently linking processors supporting different regions (“patches”) that must exchange boundary data. This infrastructure may be used with a wide variety of fluid dynamics codes; the only requirement is that their primary dependent variables be the same in all patches, e.g., fluid mass density, internal energy density, and velocity. Its structure can accommodate either Newtonian or relativistic dynamics. The overhead imposed by this system is both problem and computer cluster architecture dependent. Compared to a conventional simulation using the same number of cells and processors employed on a problem not requiring multipatch methods, the cell update per processor rate decreases by an amount that can range from negligible to a factor of a few; however, even in these problems, the infrastructure can permit substantial decreases in the total number of cell updates required.
Heliosheath Magnetic Field and Plasma Observed by Voyager 2 during 2015 Near Solar Maximum
Authors: Burlaga L. F. , Ness N. F. , Richardson J. D. 
Published: June 2018

Abstract
We discuss magnetic field and plasma observations of the heliosheath made by Voyager 2 (V2) during 2015, when V2 was observing the effects of near-maximum solar activity during solar cycle 24 following the solar minimum in 2009. The average magnetic field strength B was relatively high, 0.126 nT, as expected for solar maximum. A sector structure was observed with nearly equal maximum values of the distribution of directions of daily averages at approximately 90° and 180°, consistent with the Parker spiral magnetic field directions in the heliosheath. This structure indicates that the heliospheric current sheet (HCS) extended to high latitudes above V2 throughout most of 2015. The analysis of one sector boundary confirmed that the HCS was highly inclined (47°) with respect to the equatorial plane. The small-scale increments in B can be described by a

-Gaussian distribution with q = 1.60 ± 0.17 for daily averages and q = 1.66 ± 0.03 for hourly averages. The magnetic flux BV

R

R increased at V2, indicating that there was no significant loss of magnetic energy during 2015. Two merged interaction regions and a global merged interaction region (GMIR) were observed. The flow speed increased as the GMIR moved past V2, indicating that the GMIR was still being compressed by the flow. The GMIR caused a major decrease in the >70 MeV/nuc cosmic-ray intensity. It is likely that the GMIR is causally related to a shock-like disturbance observed by Voyager 1 in the draped interstellar magnetic field beyond the heliopause.
Excessive Shift of the CMB Acoustic Peaks of the Cold Spot Area
Authors: Chiang Lung-Yih 
Published: June 2018

Abstract
Measurement of the acoustic peaks of the cosmic microwave background (CMB) temperature anisotropies has been instrumental in deciding the geometry and content of the universe. Acoustic peak positions vary in different parts of the sky owing to statistical fluctuation. We present the statistics of the peak positions of small patches from ESA Planck data. We found that the peak positions have significantly high variance compared to the 100 CMB simulations with the best-fit ΛCDM model with lensing and Doppler boosting effects included. Examining individual patches, we found that the one containing the mysterious “Cold Spot,” an area near the Eridanus constellation where the temperature is significantly lower than Gaussian theory predicts, displays large synchronous shifts of peak positions toward smaller multipole numbers with significance lower than 1.11 × 10−4. The combination of large synchronous shifts in acoustic peaks and lower-than-usual temperature at the Cold Spot area results in a 4.73σ detection (significance p = 1.11 × 10−6) against the ΛCDM model. And it was already reported in Finelli et al. that in the WISE-2MASS galaxy catalog at z < 0.3 the Cold Spot region is surrounded by surprisingly large underdense regions around 15° in radius, which are found to be in the same square patch. Thus, we propose that there is some extra localized unknown energy to stretch out the space in the transverse direction around the Cold Spot area to simultaneously account for the Cold Spot, the excessive shift of the acoustic peaks, and the large underdense regions.
ALMA 26 Arcmin2 Survey of GOODS-S at One Millimeter (ASAGAO): Average Morphology of High-z Dusty Star-forming Galaxies in an Exponential Disk (n ≃ 1)
Authors: Fujimoto Seiji , Ouchi Masami , Kohno Kotaro , Yamaguchi Yuki , Hatsukade Bunyo , Ueda Yoshihiro , Shibuya Takatoshi , Inoue Shigeki , Oogi Taira , Toft Sune , Gómez-Guijarro Carlos , Wang Tao , Espada Daniel , Nagao Tohru , Tanaka Ichi , Ao Yiping , Umehata Hideki , Taniguchi Yoshiaki , Nakanishi Kouichiro , Rujopakarn Wiphu , Ivison R. J. , Wang Wei-hao , Lee Minju M. , Tadaki Ken-ichi , Tamura Yoichi , Dunlop J. S. 
Published: June 2018

Abstract
We present morphological properties of dusty star-forming galaxies at z = 1–3 determined with the high-resolution (FWHM ∼ 0.″19) Atacama Large Milllimeter/submillimeter Array (ALMA) 1 mm map of our ASAGAO survey covering a 26 arcmin2 area in GOODS-S. In conjunction with the ALMA archival data, our sample consists of 45 ALMA sources with infrared luminosity (L
IR) range of ∼1011–1013
L
⊙. To obtain an average rest-frame far-infrared (FIR) profile, we perform individual measurements and careful stacking of the ALMA sources using the uv-visibility method that includes positional-uncertainty and smoothing-effect evaluations through Monte Carlo simulations. We find that our sample has an average FIR-wavelength Sérsic index and effective radius of n
FIR = 1.2 ± 0.2 and R
e,FIR = 1.0–1.3 kpc, respectively, additionally with a point-source component at the center, indicative of the existence of active galactic nuclei. The average FIR profile agrees with a morphology of an exponential disk clearly distinguished from a de Vaucouleurs spheroidal profile (Sérsic index of 4). We also examine the rest-frame optical Sérsic index n
opt and effective radius R
e,opt with deep Hubble Space
Telescope (HST) images. Interestingly, we obtain n
opt = 0.9 ± 0.3 (≃n
FIR) and R
e,opt = 3.2 ± 0.6 kpc (>R
e,FIR), suggesting that the dusty disk-like structure is embedded within a larger stellar disk. The rest-frame UV and FIR data of HST and ALMA provide us with a radial profile of the total star formation rate (SFR), where the infrared SFR dominates over the UV SFR at the center. Under the assumption of a constant SFR, a compact stellar distribution in z ∼ 1–2 compact quiescent galaxies (cQGs) is well reproduced, while a spheroidal stellar morphology of cQGs (n
opt = 4) is not, suggestive of other important mechanism(s) such as dynamical dissipation.
The Mouse Pulsar Wind Nebula
Authors: Klingler Noel , Kargaltsev Oleg , Pavlov George G. , Ng C.-Y. , Beniamini Paz , Volkov Igor 
Published: June 2018

Abstract
The young energetic pulsar J1747–2958 (τ = 26 kyr,

erg s−1) powers the Mouse pulsar wind nebula (PWN), famous for its spectacular tail spanning 45″ in X-rays and 12′ in radio (d ∼ 5 kpc). We present the results of Chandra observations of the PWN and the analysis of archival lower-frequency data. The Chandra HRC image reveals a point-like source at the pulsar position, ≈1′ behind the bow shock apex of the PWN. The flattened appearance of the compact nebula is consistent with an equatorial outflow deformed by the ram pressure, implying that the angle between the pulsar’s spin axis and line of sight is ∼70° (in agreement with the radio and γ-ray pulse profiles). The spatially resolved spectroscopy with Chandra ACIS shows that the power-law (PL) spectrum steepens from Γ = 1.65 ± 0.02 to 3.0 ± 0.1 over the 45′ extent of the X-ray tail. However, the tail’s X-ray spectrum integrated over its 45″ length fits a single absorbed PL with Γ = 2.09 ± 0.03. We also found the Mouse PWN in 150 MHz GMRT data and a possible counterpart in 24 μm Spitzer data. The multiwavelength data suggest that, at low frequencies, the spectrum of the X-ray-emitting tail region can be described by a broken PL with at least one turnover between radio and X-rays. This is consistent with synchrotron cooling of electrons injected at the termination shock (with a spectral energy distribution slope of 2.2) with an equipartition magnetic field B ∼ 200 μG and a bulk flow speed v ∼ 4000 km s−1.
Le contrôle des circulations maritimes et des produits exportés dans l’espace baltique à l’époque moderne : l’exemple de Riga au xviii e  siècle
Authors: Pourchasse Pierrick 
Published: June 2018

À l’époque moderne, le Nord se spécialise dans la fourniture de matières premières vers l’Europe occidentale et développe son réseau portuaire. Sur la côte sud de la mer Baltique, les contraintes géographiques favorisent quelques ensembles portuaires situés aux débouchés des grands fleuves qui collectent les matières premières de leur arrière-pays pour l’exportation. Dans la plupart d’entre eux (Dantzig, Königsberg, Riga, Memel), les pouvoirs municipaux conservent leurs privilèges, datant du Moyen Âge, pour organiser leur commerce en établissant des règlements très stricts pour favoriser les bourgeois de la ville mais aussi pour faciliter la circulation des marchandises et garantir la qualité de ses produits sur les marchés de l’Europe occidentale. La ville de Riga, fondée en 1192, bénéficie d’une situation géographique exceptionnelle qui lui permet de collecter les marchandises d’un immense arrière-pays et de mettre en relation une grande partie de l’Europe de l’Est avec la Baltique. C’est aussi un centre nodal qui redistribue produits et matières premières du Nord vers l’ensemble du marché européen grâce à une communauté marchande bien structurée. Le port livonien bénéficie de tous les atouts nécessaires à un grand développement : une localisation idéale à l’embouchure de la Dvina (Daugava), fleuve d’environ 1000 km de longueur, un arrière-pays qui s’étend de la Livonie à l’Ukraine et un contexte institutionnel qui favorise les échanges internationaux. Le système de la ville-étape, tel qu’il fonctionne à Riga, est un moyen pour faire fonctionner ces outils stratégiques que sont les ports, leviers indispensables au développement économique et social mais aussi au rayonnement politique d’une région ou d’un pays.
Vices et malheurs de la charité : les détournements du réalisme
Authors: Pierre Chantal 
Published: June 2018

Pour le roman réaliste-naturaliste qui s’inscrit dans une période critique remettant en question l’économie et la morale de charité, celle-ci constitue à la fois un fait social à caractériser dans le cadre d’une étude de mœurs (la charité est à l’ordre du jour des agendas mondains) et un récit préétabli (comme la visite au pauvre prescrite et détaillée par les manuels de charité du dix-neuvième siècle, tel Gérando) avec des protagonistes, un déroulement, une tonalité (le pathétique) qu’il s’agit de dérégler et de déprogrammer. Il en résulte des scènes de charité mondaine, obscène et prostitutionnelle, des scènes d’aumônes détournées en scènes érotiques et des catastrophes (morts, viols, vols…) en guise de dénouement au scénario caritatif. L’ultime dommage réaliste infligé à l’économie de la charité consiste en la suppression de l’échange sentimental qui est censé l’accompagner : reconnaissance et attendrissement n’ont plus cours.
Comparison of &lt;i&gt;H&lt;/i&gt; component geomagnetic field time series obtained at different sites over South America
Authors: Bolzan Maurício J. A. , Denardini Clezio M. , Tardelli Alexandre 
Published: June 2018

Abstract. The
geomagnetic field in the Brazilian sector is influenced by the South American
Magnetic Anomaly (SAMA) that causes a decrease in the magnitude of the local
geomagnetic field when compared to other regions in the world. Thus, the
magnetometer network and data set of space weather over Brazil led by Embrace
are important tools for promoting the understanding of geomagnetic fields
over Brazil. In this sense, in this work we used the H component of
geomagnetic fields obtained at different sites in South America in order to
compare results from the phase coherence obtained from wavelet transform
(WT). Results from comparison between Cachoeira Paulista (CXP) and
Eusébio (EUS), and Cachoeira Paulista and São Luis (SLZ), indicated
that there exist some phenomena that occur simultaneously in both locations,
putting them in the same phase coherence. However, there are other phenomena
putting both locations in a strong phase difference as observed between CXP
and Rio Grande, Argentina (RGA). This study was done for a specific moderate
geomagnetic storm that occurred in March 2003. The results are explained in
terms of nonlinear interaction between physical phenomena acting in distinct
geographic locations and at different times and scales. Keywords. Geomagnetism and paleomagnetism (time variations – diurnal to secular)
Early Twentieth-Century Religio-Racial Movements and the Radical Reconfiguration of Memory, Experience, and Imagination
Authors: Sesay Chernoh M. 
Published: June 2018

Abstract
This review highlights how Judith Weisenfeld's concept of “religio-racial” consciousness reveals the comparative and contrasting ways that Ethiopian Hebrews, the Moorish Science Temple, the Nation of Islam, and the Peace Mission refigured perspectives of time and space. Weisenfeld's analysis also underscores the limits of Protestantism for understanding twentieth-century racial communities.
In-Service Music Teachers’ Self-Perceived Sources of Pedagogical Content Knowledge
Authors: Haston Warren 
Published: June 2018

Abstract
The purpose of this multiple case study was to examine the perceived sources of identifiable pedagogical content knowledge (PCK) used by 5 in-service secondary band teachers. Participants agreed to plan, teach, and video-record a 30-minute band rehearsal early in the second semester of the school year. I viewed each video and created a log of applications of PCK based on previous models. An independent researcher confirmed the identified instances of applied PCK. Without exception, participants confirmed the researcher-identified applications of PCK. The responses from the participants varied: 1 participant reported apprenticeship of observation as the primary source of PCK; 1 reported apprenticeship of observation and methods courses equally; another reported intuition and peers equally; 1 reported peers; and another reported cooperating teacher. Participants recognized the positive impacts this type of metacognition had on their teaching and expressed eagerness to reflect about their PCK in the future.
Fifty Years in Folklore
Authors: Teske Robert T. 
Published: June 2018

Abstract
Much like Tim Lloyd, Robert Teske stumbled into folklore in the undergraduate classroom. He soon found himself a member of the first class of undergraduate folklore majors at Harvard University. Teske went on to complete a PhD in Folklore and Folklife at the University of Pennsylvania and embarked on an academic career teaching first at Wayne State and then at Western Kentucky University. Prepared for a lifetime of scholarly endeavor, Teske made a career U-turn when the opportunity arose to work at the National Endowment for the Arts, Folk Arts Program, under the leadership of Bess Lomax Hawes. He later returned to his home state of Wisconsin for a career working in arts and historical agencies. “Fifty Years in Folklore” is a revised version of a keynote address given by Teske in March 2017 at a symposium honoring the 50-year anniversary of the establishment of the Committee on Degrees in Folklore and Mythology at Harvard. As with the Lloyd interview included in this issue, it provides a personal and close look at a career trajectory of a folklorist active in our field’s past half-century.
Dwight Diller’s Documentation of the West Virginia Hammons Family
Authors: Stern Lewis M. 
Published: June 2018

Abstract
While many individuals discovered folklore in the undergraduate classroom, others entered the field through the portal of music (though, of course, the two groups are not mutually exclusive). Although the relationship between the folk revival and the professional field of folklore has often been noted, typically it is with a broad brush, looking at national trends rather than specific instances. In this essay, Lewis Stern examines in detail a narrow slice of this history. His is the story of a remarkable West Virginia family, the excitement they generated among a group of musicians (several of them nascent folklorists), and the relationships that developed between amateur and professional documentarians of folklife. The ensuing collaborations were both productive, resulting in recordings that are still influential in old-time music and chaotic in their archival results. With the patience of a detective, Stern teases out the many manifestations of Dwight Diller’s original recordings of the Hammons family and discusses the ultimate fate of the recordings.
Mapping Appalachia’s Boundaries: Historiographic Overview and Digital Collection
Authors: Scales Stewart , Satterwhite Emily , August Abigail 
Published: June 2018

Abstract
In this article, we offer a historiographical overview of major scholarly and political delineations of Appalachia from 1895 to the present alongside an online component that allows for an extensive virtual collection of historical maps as well as greater dynamism for user exploration.
A new genus of Tetracampidae (Hymenoptera) from South Africa
Authors: Gumovsky Alex 
Published: June 2018

Afrocampe gen. nov. is described for its only species, A. prinslooi gen. et sp. nov., from Eastern and Western Cape, South Africa. This new genus is recognized as a member of the subfamily Tetracampinae Förster, 1856 of Tetracampidae Förster, 1856 based on the possession of 5-segmented tarsi in females and 4-segmented tarsi in males, the short straight calcar, the mesoscutum with distinct notauli, the mesoscutellum with two pairs of setae, the reduced mesopleural suture and the short stigmal and long postmarginal veins of the fore wing. Afrocampe gen. nov. is characterized by a large mesosoma, a non-convex first gastral tergite, an evenly acute calcar, a 5-segmented antennal funicle, a head lacking occipital carina and facial grooves and a long fore wing with distinctly delimited speculum, a bare admarginal area with a distinct admarginal row of setae on the underside and with 3 setal tracks (hair rows) radiating from the apex of the stigmal vein. The combination of these characters suggests a special status of the new genus within the subfamily Tetracampinae. Moreover, Afrocampe gen. nov. bears some resemblance to the Australian tetracampine genus Niticampe Bouček, 1988. The position of the latter in Tetracampinae, as well as habitus features of the former, are discussed.