cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Neoperla magisterchoui Du 2000
Creators: name: Li, Weihai
name: Li, Shan
name: Feng, Guangwei
name: Wang, Yunbing
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperla
Neoperla magisterchoui

description: Neoperla magisterchoui Du, 2000
 Neoperla magisterchoui Du, 2000. In Zhang, Y. L. Systematic and Faunistic Research on Chinese Insects. Proceedings of the 5th National Congress of Insect Taxonomy: 1. Type locality: Shaanxi (Ningshan County, Xunyangba); Li et al., 2011. Zootaxa. 2735: 57.
 Material examined. 1 male (HIST), Henan Province, Song County, Baiyuanshan, 2002. VII.19, light trap, Hongliang Wang.
 Distribution. China (Henan and Shaanxi provinces) (Du 2000; Li et al. 2011).
description: Published as part of Li, Weihai, Li, Shan, Feng, Guangwei & Wang, Yunbing, 2014, Species of Neoperla (Plecoptera: Perlidae) from Henan Province, China, pp. 174-182 in Zootaxa 3838 (2) on page 178, DOI: 10.11646/zootaxa.3838.2.2, http://zenodo.org/record/226918
Topological entropy of transitive dendrite maps
Creators: name: Špitalský, Vladimír
Publisher: name: arXiv
Year: 2012
Subjects: subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 37B05, 37B20, 37B40 (Primary) 54H20 (Secondary)

description: We show that every dendrite satisfying the condition that no subtree of it contains all free arcs admits a transitive, even exactly Devaney chaotic map with arbitrarily small entropy. This gives a partial answer to a question of Baldwin from 2001.
description: 26 pages, 4 figures
Neoperla yaoshana Li, Wang & Lu 2011
Creators: name: Li, Weihai
name: Li, Shan
name: Feng, Guangwei
name: Wang, Yunbing
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperla
Neoperla yaoshana

description: Neoperla yaoshana Li, Wang & Lu, 2011
 Neoperla yaoshana Li, Wang & Lu, 2011. Zootaxa. 2735: 58. Type locality: Henan, Lushan County, Yaoshan.
 Distribution. China (Henan Province) (Li et al. 2011).
description: Published as part of Li, Weihai, Li, Shan, Feng, Guangwei & Wang, Yunbing, 2014, Species of Neoperla (Plecoptera: Perlidae) from Henan Province, China, pp. 174-182 in Zootaxa 3838 (2) on page 178, DOI: 10.11646/zootaxa.3838.2.2, http://zenodo.org/record/226918
Tachydromia bickeli Grootaert 2011, n.sp.
Creators: name: Grootaert, Patrick
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Hybotidae
Tachydromia
Tachydromia bickeli

description: Tachydromia bickeli n.sp. Fig. 2 Type material. HOLOTYPE ♂, Australia, New South Wales, Fenwicks Ck, Doyles Riv. SF, 6.12.1986, D.J. Bickel; AMS K258849. PARATYPES: 1♀, same data as in holotype, AMS K258832; 1♂, 10 km NE of “ Tuglo ”, 48 km N of Singleton, N.S.W., Dec 1981, B.J. Day, AMS K258761; 1♂, 33 km NNE Singleton, “ Tuglo ”, on E. caniculata, 17.11.1985, D.J. Bickel, AMS K258793; 1♂, Styx River SF, 1300 m Cunnawarra Rd nr Georges Ck, cool temperate rain forest, sticky trap on tree, 19– 20.12.1998, D.J. Bickel, AMS K258863; 1♂, Tuglo, 48 km N of Singleton, 15 Nov. 1985, AMS K258745; 1♂, Carrai SF, 31°00'19"S 152°16'24"E, 940 m, E. Tasker, 11.01– 16.01.1998, sticky trap on E. saligna, CS-PG-018–3, AMS K258876; 1♂, Coombadjha Ck, Washpool NP, rainforest, sticky traps trunks, 29°25'S 152°23'E, 12– 13.01.2001, D. Bickel, AMS K258813; 1♀, Barrington Tops NP, Upper Williams R., 550 m, tree trunk E. sp., 26.01.1987, D.J. Bickel, AMS K258728; 1♀, Mt. Royal nr. Singleton, 20 Nov. 1988, B.J. Day, AMS K258739; 1♀, Wenikimbe NP, 900 m, Mooraback area, sticky trap snow gum, 17– 19.11.1998, D. Bickel, AMS K258727; 1♀, Coombadjha Ck, Washpool S.F., 10 Feb. 1982, B.J. Day, AMS K258825; 3♀♀, Royal NP, Bela Ck., closed forest, 12.02.1985, D.J. Bickel, AMS K258831, AMS K258838, AMS K258846; 1♀, Esk River, nr Iluka, rain forest, 24.11.1985, D. Bickel & G. Cassis, AMS K259315; 1♀, Myall Lakes Nat. Park, 22.11.1985, D.B. Bickel & G. Cassis, AMS K258882; 1♂, Fenwicks Ck, Dayles River State Forest, 6.xii.1986, 1056 m, D.J. Bickel (AMS); 1♀, 33 km NNE Singleton, 17.xi.1985, “Tuglo”, D.J. Bickel, on E. caniculata. Additional material. NEW SOUTH WALES: 1♀, Wentworth Falls, Blue Mts, 6.12.1986, D.K. McAlpine, K.C. Khoo, R. de Keyzer; AMS K258744. 1♀, Banda Banda FR, 31.10S 152.26E, 1020 m, temporary rain forest, sticky trap Nothofagus, 19.11.1998, D. Bickel; AMS K258795. These specimens are in bad condition that is why we did not include them to the paratypes. Diagnosis. Recognized by the fore femur with broad brown ring in apical half leaving narrow, yellow subapical space, mid and hind femora entirely brown.
description: Published as part of Grootaert, Patrick, 2011, The Genus Tachydromia Meigen (Diptera: Hybotidae) from Australia, pp. 103-112 in Records of the Australian Museum 63 (1) on page 105, DOI: 10.3853/j.0067-1975.63.2011.1552, http://zenodo.org/record/5239377
Additional file 1 of Evaluating a research training programme for frontline health workers in conflict-affected and fragile settings in the middle east
Creators: name: Naal, Hady
name: Daou, Tracy
name: Brome, Dayana
name: Mansour, Rania
name: Sittah, Ghassan Abu
name: Giannou, Christos
name: Steiger, Enrique
name: Saleh, Shadi
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Supplementary Material 1
GRB 110721A: photosphere "death line" and the physical origin of the GRB "Band" function
Creators: name: Zhang, Bing
name: Lu, Rui-Jing
name: Liang, En-Wei
name: Wu, Xue-Feng
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The prompt emission spectra of gamma-ray bursts (GRBs) usually have a dominant component that is well described by a phenomenological "Band" function. The physical origin of this spectral component is debated. Although the traditional interpretation is synchrotron radiation of non-thermal electrons accelerated in internal shocks or magnetic dissipation regions, a growing trend in the community is to interpret this component as modified thermal emission from a dissipative photosphere of a GRB fireball. We analyze the time dependent spectrum of GRB 110721A detected by {\em Fermi} GBM and LAT, and pay special attention to the rapid evolution of the peak energy $E_p$. We define a "death line" of thermally-dominated dissipative photospheric emission in the $E_p - L$ plane, and show that $E_p$ of GRB 110721A at the earliest epoch has a very high $E_p \sim 15$ MeV that is beyond the "death line". Together with the finding that an additional "shoulder" component exists in this burst that is consistent with a photospheric origin, we suggest that at least for some bursts, the "Band" component is not from a dissipative photosphere, but must invoke a non-thermal origin (e.g. synchrotron or inverse Compton) in the optically thin region of a GRB outflow. We also suggest that the rapid "hard-to-soft" spectral evolution is consistent with the quick discharge of magnetic energy in a magnetically-dominated outflow in the optically thin region.
description: 5 pages, 4 figures, ApJL, in press
Additional file 1 of Thromboelastometry-guided haemostatic resuscitation in severely injured patients: a propensity score-matched study
Creators: name: David, Jean-Stéphane
name: James, Arthur
name: Orion, Maxime
name: Selves, Agathe
name: Bonnet, Mélody
name: Glasman, Pauline
name: Vacheron, Charles-Hervé
name: Raux, Mathieu
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy

description: Additional file 1: Table S1. Missing data. Table S2. ROTEM analysis for patients in the VHA group at admission. Table S3. Blood products and coagulation factors cost before and after matching in euros
Mining Social Data to Extract Intellectual Knowledge
Creators: name: Rahman, Muhammad Mahbubur
Publisher: name: arXiv
Year: 2012
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Social and Information Networks (cs.SI)
subject: FOS: Computer and information sciences

description: Social data mining is an interesting phe-nomenon which colligates different sources of social data to extract information. This information can be used in relationship prediction, decision making, pat-tern recognition, social mapping, responsibility distri-bution and many other applications. This paper presents a systematical data mining architecture to mine intellectual knowledge from social data. In this research, we use social networking site facebook as primary data source. We collect different attributes such as about me, comments, wall post and age from facebook as raw data and use advanced data mining approaches to excavate intellectual knowledge. We also analyze our mined knowledge with comparison for possible usages like as human behavior prediction, pattern recognition, job responsibility distribution, decision making and product promoting.
description: 8 pages, 19 figures, 4 tables, 3 equations, ISSN: 2074-904X (Print), ISSN: 2074-9058 (Online)
Scaling theory of driven polymer translocation
Creators: name: Ikonen, Timo
name: Bhattacharya, Aniket
name: Ala-Nissila, Tapio
name: Sung, Wokyung
Publisher: name: arXiv
Year: 2012
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present a theoretical argument to derive a scaling law between the mean translocation time $τ$ and the chain length $N$ for driven polymer translocation. This scaling law explicitly takes into account the pore-polymer interactions, which appear as a correction term to asymptotic scaling and are responsible for the dominant finite size effects in the process. By eliminating the correction-to-scaling term we introduce a rescaled translocation time and show, by employing both the Brownian Dynamics Tension Propagation theory [Ikonen {\it et al.}, Phys. Rev. E {\bf 85}, 051803 (2012)] and molecular dynamics simulations that the rescaled exponent reaches the asymptotic limit in a range of chain lengths that is easily accessible to simulations and experiments. The rescaling procedure can also be used to quantitatively estimate the magnitude of the pore-polymer interaction from simulations or experimental data. Finally, we also consider the case of driven translocation with hydrodynamic interactions (HIs). We show that by augmenting the BDTP theory with HIs one reaches a good agreement between the theory and previous simulation results found in the literature. Our results suggest that the scaling relation between $τ$ and $N$ is retained even in this case.
description: 5 pages, 4 figures
Neoperla
Creators: name: Li, Weihai
name: Li, Shan
name: Feng, Guangwei
name: Wang, Yunbing
Publisher: name: Zenodo
Year: 2014
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Plecoptera
Perlidae
Neoperla

description: Key to species of Neoperla (males) known from Henan
1. Aedeagal tube completely sclerotized...................................................................... 2
-. Aedeagal tube incompletely sclerotized.................................................................... 4
 2. Aedeagal tube with ventral lobes (Fig. 5, Li et al. 2011)............................................. N. flavescens
-. Aedeagal tube without ventral lobes....................................................................... 3
 3. Aedeagal sac about as long as tube, with small spines (Fig. 4, Li et al. 2014).............................. N. cavaleriei
 -. Aedeagal sac ca. 1.5x tube length, with linear large spines (Fig. 1 d).................................. N. baotianmana
4. Aedeagal tube with single ventral lobes.................................................................... 5
-. Aedeagal tube with one pair of ventral lobes................................................................ 6
 5. Aedeagal lobe finger like (Figs. 4 a & b)................................................. N. jigongshana sp. nov.
 -. Aedeagal lobe bifurcate........................................................................ N. forcipata
 6. Aedeagal tube with a pair of ventral projections in addition to lateral lobes apically.................... N. magisterchoui
-. Aedeagal tube only with a pair of ventral projections apically................................................... 7
 7. Aedeagal sac lacking ventral spines (Fig. 15, Li et al. 2011); apical half with a field of fine spinules separated by a lateral membranous area (Fig. 17, Li et al. 2011)........................................................ N. yaoshana
 -. Aedeagal sac with ventral spines medially; apical half evenly covered by fine lateral spinules with no membranous area (Fig. 3, Li et al. 2011)................................................................................ N. henana
description: Published as part of Li, Weihai, Li, Shan, Feng, Guangwei & Wang, Yunbing, 2014, Species of Neoperla (Plecoptera: Perlidae) from Henan Province, China, pp. 174-182 in Zootaxa 3838 (2) on page 181, DOI: 10.11646/zootaxa.3838.2.2, http://zenodo.org/record/226918
Evolution of the Solar Flare Energetic Electrons in the Inhomogeneous Inner Heliosphere
Creators: name: Reid, Hamish A. S.
name: Kontar, Eduard P.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Solar flare accelerated electrons escaping into the interplanetary space and seen as type III solar radio bursts are often detected near the Earth. Using numerical simulations we consider the evolution of energetic electron spectrum in the inner heliosphere and near the Earth. The role of Langmuir wave generation, heliospheric plasma density fluctuations, and expansion of magnetic field lines on the electron peak flux and fluence spectra is studied to predict the electron properties as could be observed by Solar Orbiter and Solar Probe Plus. Considering various energy loss mechanisms we show that the substantial part of the initial energetic electron energy is lost via wave-plasma processes due to plasma inhomogeneity. For the parameters adopted, the results show that the electron spectra changes mostly at the distances before $\sim20 R_\odot$. Further into the heliosphere, the electron flux spectra of electrons forms a broken power-law relatively similar to what is observed at 1 AU.
description: 16 pages, 7 figures, Published in Solar Physics
Additional file 2 of Evaluating a research training programme for frontline health workers in conflict-affected and fragile settings in the middle east
Creators: name: Naal, Hady
name: Daou, Tracy
name: Brome, Dayana
name: Mansour, Rania
name: Sittah, Ghassan Abu
name: Giannou, Christos
name: Steiger, Enrique
name: Saleh, Shadi
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Supplementary Material 2
Influence of non-universal effects on dynamical scaling in driven polymer translocation
Creators: name: Ikonen, Timo
name: Bhattacharya, Aniket
name: Ala-Nissila, Tapio
name: Sung, Wokyung
Publisher: name: arXiv
Year: 2012
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We study the dynamics of driven polymer translocation using both molecular dynamics (MD) simulations and a theoretical model based on the non-equilibrium tension propagation on the {\it cis} side subchain. We present theoretical and numerical evidence that the non-universal behavior observed in experiments and simulations are due to finite chain length effects that persist well beyond the relevant experimental and simulation regimes. In particular, we consider the influence of the pore-polymer interactions and show that they give a major contribution to the non-universal effects. In addition, we present comparisons between the theory and MD simulations for several quantities, showing extremely good agreement in the relevant parameter regimes. Finally, we discuss the potential limitations of the present theories.
description: 17 pages, 15 figures
Additional file 3 of Evaluating a research training programme for frontline health workers in conflict-affected and fragile settings in the middle east
Creators: name: Naal, Hady
name: Daou, Tracy
name: Brome, Dayana
name: Mansour, Rania
name: Sittah, Ghassan Abu
name: Giannou, Christos
name: Steiger, Enrique
name: Saleh, Shadi
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Supplementary Material 3
PSR J1838-0537: Discovery of a young, energetic gamma-ray pulsar
Creators: name: Pletsch, H. J.
name: Guillemot, L.
name: Allen, B.
name: Kramer, M.
name: Aulbert, C.
name: Fehrmann, H.
name: Baring, M. G.
name: Camilo, F.
name: Caraveo, P. A.
name: Grove, J. E.
name: Kerr, M.
name: Marelli, M.
name: Ransom, S. M.
name: Ray, P. S.
name: Parkinson, P. M. Saz
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We report the discovery of PSR J1838-0537, a gamma-ray pulsar found through a blind search of data from the Fermi Large Area Telescope (LAT). The pulsar has a spin frequency of 6.9 Hz and a frequency derivative of -2.2e-11 Hz/s, implying a young characteristic age of 4970 years and a large spin-down power of 5.9e36 erg/s. Follow-up observations with radio telescopes detected no pulsations, thus PSR J1838-0537 appears radio-quiet as viewed from Earth. In September 2009 the pulsar suffered the largest glitch so far seen in any gamma-ray-only pulsar, causing a relative increase in spin frequency of about 5.5e-6. After the glitch, during a putative recovery period, the timing analysis is complicated by the sparsity of the LAT photon data, the weakness of the pulsations, and the reduction in average exposure from a coincidental, contemporaneous change in the LAT's sky-survey observing pattern. The pulsar's sky position is coincident with the spatially extended TeV source HESS J1841-055 detected by the High Energy Stereoscopic System (H.E.S.S.). The inferred energetics suggest that HESS J1841-055 contains a pulsar wind nebula powered by the pulsar.
description: 6 pages, 3 figures. To appear in the Astrophysical Journal Letters
A FLEXÃO DE GÊNERO E A ESTUPIDEZ
Creators: name: Santana, José Cláudio Pavão
Publisher: name: Zenodo - Cadernos da Pena do Pavao
Year: 2023

description: Ano 09 – vol. 02 – n. 21/2021
Leio, com dissabor, que o Conselho Nacional de Justiça "obriga o uso da flexão de gênero no judiciário nacional".
Dissabor porque eu desrespeite as opções sexuais ou de identidade?
Não, porque sou…, digamos assim, portador de sanidade mental, característica, aliás, em escassez
no Brasil.
Are Outflows Biasing Single-Epoch CIV Black Hole Mass Estimates?
Creators: name: Denney, Kelly D.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use a combination of reverberation mapping data and single-epoch spectra of the CIV emission line in a sample of both low and high-redshift active galactic nuclei (AGNs) to investigate sources of the discrepancies between CIV- and Hbeta-based single-epoch black hole mass estimates. We find that for all reverberation mapped sources, there is a component of the line profile that does not reverberate, and the velocity characteristics of this component vary from object-to-object. The differing strength and properties of this non-variable component are responsible for much of the scatter in CIV-based black hole masses compared to Hbeta masses. The CIV mass bias introduced by this non-variable component is correlated with the shape of the CIV line, allowing us to make an empirical correction to the black hole mass estimates. Using this correction and accounting for other sources of scatter such as poor data quality and data inhomogeneity reduces the scatter between the CIV and Hbeta masses in our sample by a factor of ~2, to only ~0.2 dex. We discuss the possibility that this non-variable CIV component originates in an orientation-dependent outflow from either the proposed broad line region (BLR) disk-wind or the intermediate line region (ILR), a high-velocity inner extension of the narrow line region (NLR).
description: 16 pages, 10 figures, accepted for publication in the Astrophysical Journal (v2 addresses suggestions of the referee, which includes only minor text modifications compared to v1)
Generation of spatially pure photon pairs in a multimode nonlinear waveguide using intermodal dispersion
Creators: name: Karpinski, Michal
name: Radzewicz, Czeslaw
name: Banaszek, Konrad
Publisher: name: arXiv
Year: 2012
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We present experimental realization of type-II spontaneous parametric down-conversion in a periodically poled potassium titanyl phosphate (KTiOPO4) nonlinear waveguide. We demonstrate that by careful exploitation of intermodal dispersion in the waveguide it is feasible to produce photon pairs in well defined transverse modes without any additional spatial filtering at the output. Spatial characteristics is verified by measurements of the M2 beam quality factors. We also prepared a postselected polarization-entangled two-photon state shown to violate Bell's inequality. Similar techniques based on intermodal dispersion can be used to generate spatial entanglement and hyperentanglement.
description: 11 pages, 5 figures, submitted to Proceedings of Quantum Communications and Quantum Imaging X Conference at SPIE 2012 Optics + Photonics, San Diego, 12-16 August 2012
title: Forschungsdatenmanagement für Einzel- und Verbundprojekte: Aufbau und Erprobung von Bausteinen für ein effektives und effizientes FDM
Creators: name: Baaske, Markus
name: Hesse, Bettina
name: Gerlach, Roman
name: Baaske, Franka
name: König-Ries, Brigitta
Publisher: name: Friedrich-Schiller-Universität Jena
Year: 2017
Subjects: subject: Forschungsdatenmanagement
subject: 004

description: Das hier beschriebene Projekt untersucht verschiedene konzeptuelle Ansätze und mögliche Strategien zur Generalisierung von geeigneten Angeboten zum Forschungsdatenmanagement (FDM) für Forschende in Verbundprojekten und als Einzelwissenschaftler entlang des gesamten Datenlebenszyklus. Die Ergebnisse sollen in die Bereiche des nachhaltigen Forschungsdatenmanagements, der Personalentwicklung und der Lehre transportiert werden .
title: Entwicklung von FDM-Kompetenzen an der FSU Jena: Aufbau und Erprobung von Bausteinen für ein effektives und effizientes FDM
Creators: name: Baaske, Franka
name: Baaske, Markus
name: Gerlach, Roman
name: Hesse, Bettina
name: König-Ries, Brigitta
Publisher: name: Friedrich-Schiller-Universität Jena
Year: 2017
Subjects: subject: Forschungsdatenmanagement, Lehre
subject: 004

description: Im Mittelpunkt des hier beschriebenen Teilprojekts steht die Entwicklung der Kompetenzen verschiedenster Akteure im Umgang mit Forschungsdaten. Dabei sollen bestehende Konzepte und Materialien zum Forschungsdatenmanagement geprüft und ggt. angepasst bzw. neu entwickelt werden.
A multi-spacecraft view of a giant filament eruption during 26/27 September 2009
Creators: name: Gosain, Sanjay
name: Schmieder, Brigitte
name: Artzner, Guy
name: Bogachev, Sergei
name: Torok, Tibor
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We analyze multi-spacecraft observations of a giant filament eruption that occurred during 26 and 27 September 2009. The filament eruption was associated with a relatively slow coronal mass ejection (CME). The filament consisted of a large and a small part, both parts erupted nearly simultaneously. Here we focus on the eruption associated with the larger part of the filament. The STEREO satellites were separated by about 117 degree during this event, so we additionally used SoHO/EIT and CORONAS/TESIS observations as a third eye (Earth view) to aid our measurements. We measure the plane-of-sky trajectory of the filament as seen from STEREO-A and TESIS view-points. Using a simple trigonometric relation, we then use these measurements to estimate the true direction of propagation of the filament which allows us to derive the true R=R_sun v/s time profile of the filament apex. Furthermore, we develop a new tomographic method that can potentially provide a more robust three-dimensional reconstruction by exploiting multiple simultaneous views. We apply this method also to investigate the 3D evolution of the top part of filament. We expect this method to be useful when SDO and STEREO observations are combined. We then analyze the kinematics of the eruptive filament during its rapid acceleration phase by fitting different functional forms to the height-time data derived from the two methods. We find that, for both methods, an exponential function fits the rise profile of the filament slightly better than parabolic or cubic functions. Finally, we confront these results with the predictions of theoretical eruption models.
description: 16 pages, 9 figures, to appear in Astrophysical Journal
The Identity String Field and the Sliver Frame Level Expansion
Creators: name: Erler, Theodore
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a modified version of the sliver-frame level expansion which gives a tool for analyzing singularities related to the identity string field. We apply this formalism to the newly discovered solutions of Masuda, Noumi, and Takahashi.
description: 27 pages, 2 figures V2: typos fixed, added citations, minor improvements
Additional file 1 of A tumor microenvironment-based prognostic index for osteosarcoma
Creators: name: Wu, Changwu
name: Gong, Siming
name: Duan, Yingjuan
name: Deng, Chao
name: Kallendrusch, Sonja
name: Berninghausen, Laura
name: Osterhoff, Georg
name: Schopow, Nikolas
Publisher: name: figshare
Year: 2023
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1: Table S1. Clinical characteristics of patients with osteosarcoma in each dataset. Table S5. Univariate and multivariate Cox regression analysis of overall survival, relapse free survival and metastasis free survival in each data set. Figure S1. The flow diagram of this study. Figure S2. ImmuneScore and StromalScore associate with clinical features and outcomes. Figure S3. Analysis of network topology for various soft-thresholding powers. Figure S4. OS prediction value of 4 genes in the TMEindex. Figure S5. RFS prediction value of 4 genes in the TMEindex. Figure S6. Differences in survival time and TMEindex genes expression between high and low TMEindex groups. Figure S7. Stratified analysis to further determine the prognostic value of the TMEindex based on the clinical characteristics of patients. Figure S8. Progonsis prediction value of the TMEindex in osteoblastic and chondroblastic osteosarcoma in the GSE21257 cohort. Figure S9. Validation of the prognostic value of the TMEindex in GSE33382. Figure S10. GSEA enrichment plots base on KEGG gene set showing the relatively enriched pathways in TMEindex-high (A) and TMEindex-low (B) group. Figure S11. GO enrichment and KEGG pathway analysis of DEGs identified between high and low TMEindex groups. Figure S12. Pan-cancer analysis of the prognostic predictive value of TMEindex. Figure S13. Univariate Cox regression analysis reveals the association of TMEindex with the PFS of 32 tumor types.
Freeze-out Conditions from Lattice QCD
Creators: name: Mukherjee, Swagato
Publisher: name: arXiv
Year: 2012
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We describe a procedure for determination of freeze-out parameters of heavy-ion collisions through direct comparisons between experimentally measured higher order cumulants of charge fluctuations and first principle (lattice) QCD calculations.
description: Talk given at Quark Matter 2012, August 13-18, 2012, Washington DC
The Neutrino Mass Hierarchy at Reactor Experiments now that theta13 is Large
Creators: name: Ciuffoli, Emilio
name: Evslin, Jarah
name: Zhang, Xinmin
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Now that theta13 is known to be large, a medium baseline reactor experiment can observe the fine structure of the electron antineutrino survival probability curve, approximately periodic oscillations in L/E with wavelength 4pi/Delta M^2_31. The periodicity with respect to L/E is broken by 2-3 oscillations which, in the case of the normal (inverted) hierarchy, shift the first 16 oscillations nearly 1% higher (lower) and move the next 16 lower (higher). The energy of each peak determines a particular combination of the mass differences, for example cos^2(theta12)Delta M^2_31 + sin^2(theta12)Delta M^2_32 for nearly all peaks visible at baselines under 40 km. Comparing these combinations with each other or with NOvA results one can in principle determine the mass hierarchy. Alternately, as the Fourier transforms of the 1-3 and 2-3 oscillation probabilities are out of phase by the 1-2 oscillation probability, near the maximum of the 1-2 oscillation the complex phase of the total survival probability can be used to determine the hierarchy. Two interference effects make this task difficult. First, kilometer distances between the reactors reduce the amplitudes of peaks below about 4 MeV. Second, even reactors 100 or more kilometers away significantly obscure the 1-2 oscillation maximum, which also complicates a measurement of the solar mixing angle with a single detector.
description: 32 pages, 15 pdf figures, refs added
Additional file 1 of Evaluation of safety and efficacy of autologous oral mucosa-derived epithelial cell sheet transplantation for prevention of anastomotic restenosis in congenital esophageal atresia and congenital esophageal stenosis
Creators: name: Fujino, Akihiro
name: Fuchimoto, Yasushi
name: Mori, Teizaburo
name: Kano, Motohiro
name: Yamada, Yohei
name: Ohno, Michinobu
name: Baba, Yoshiyuki
name: Isogawa, Nobutaka
name: Arai, Katsuhiro
name: Yoshioka, Takako
name: Abe, Makoto
name: Kanai, Nobuo
name: Takagi, Ryo
name: Maeda, Masanori
name: Umezawa, Akihiro
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Hematology

description: Additional file 1: Table S1. Preparation of oral mucosal epithelial cell sheets.
Additional file 2 of Evaluation of safety and efficacy of autologous oral mucosa-derived epithelial cell sheet transplantation for prevention of anastomotic restenosis in congenital esophageal atresia and congenital esophageal stenosis
Creators: name: Fujino, Akihiro
name: Fuchimoto, Yasushi
name: Mori, Teizaburo
name: Kano, Motohiro
name: Yamada, Yohei
name: Ohno, Michinobu
name: Baba, Yoshiyuki
name: Isogawa, Nobutaka
name: Arai, Katsuhiro
name: Yoshioka, Takako
name: Abe, Makoto
name: Kanai, Nobuo
name: Takagi, Ryo
name: Maeda, Masanori
name: Umezawa, Akihiro
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Hematology

description: Additional file 2: Table S2. Inspection items for epithelial cell sheet transplantation and their timing.
A BECA, A BOCA E O ESCÁRNIO
Creators: name: Santana, José Cláudio Pavão
Publisher: name: Zenodo - Cadernos da Pena do Pavao
Year: 2023

description: Ano 09 – vol. 12 – n. 80/2021
Assisti um vídeo que circula pelas redes sociais em que um militante (não posso atribuir outra denominação) efusivamente exibe uma beca como "manto da justiça" e, convidando uma defensora pública, faz entrega ao ex presidiário e agora o maior símbolo de impunidade do Brasil, com o enfático destaque de que o mesmo seja
merecedor.
Generalized Transversality Conditions in Fractional Calculus of Variations
Creators: name: Almeida, Ricardo
name: Malinowska, Agnieszka B.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics
subject: 49K05, 26A33

description: Problems of calculus of variations with variable endpoints cannot be solved without transversality conditions. Here, we establish such type of conditions for fractional variational problems with the Caputo derivative. We consider: the Bolza-type fractional variational problem, the fractional variational problem with a Lagrangian that may also depend on the unspecified end-point $φ(b)$, where $x=φ(t)$ is a given curve, and the infinite horizon fractional variational problem.
description: This is a preprint of a paper whose final and definite form will be published in Communications in Nonlinear Science and Numerical Simulation, accepted 14-July-2012
A scale-covariant quantum space-time
Creators: name: Perini, Claudio
name: Tornetta, Gabriele Nunzio
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: A noncommutative space-time admitting dilation symmetry was briefly mentioned in the seminal work of Doplicher, Fredenhagen and Roberts. In this paper we explicitly construct the model in details and carry out an in-depth analysis. The C*-algebra that describes this quantum space-time is determined, and it is shown that it admits an action by *-automorphisms of the dilation group, along with the expected Poincaré covariance. In order to study the main physical properties of this scale-covariant model, a free scalar neutral field is introduced as a investigation tool. Our key results are then the loss of locality and the irreducibility, or triviality, of special field algebras associated with regions of the ordinary Minkowski space-time. It turns out, in the conclusions, that this analysis allows also to argue on viable ways of constructing a full conformally covariant model for quantum space-time.
description: 38 pages
Aerodynamic Investigation of the High-Lift Performance of a Propeller-Driven Regional Transport Aircraft with Distributed Propulsion
Creators: name: Keller Denis
Publisher: name: Zenodo
Year: 2022
Subjects: IMOTHEP
green aviation
H2020 Transport
climate change
electric aircraft
hybrid electric propulsion

description: Presentation at the 12th EASN International Conference on “Innovation in aviation & space for opening new horizons", 18-21 Oct 2022, Barcelona, Spain, https://easnconference.eu/
String Derived Exophobic SU(6)xSU(2) GUTs
Creators: name: Bernard, Laura
name: Faraggi, Alon E
name: Glasser, Ivan
name: Rizos, John
name: Sonmez, Hasan
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: With the apparent discovery of the Higgs boson, the Standard Model has been confirmed as the theory accounting for all sub-atomic phenomena. This observation lends further credence to the perturbative unification in Grand Unified Theories (GUTs) and string theories. The free fermionic formalism yielded fertile ground for the construction of quasi--realistic heterotic--string models, which correspond to toroidal Z2xZ2 orbifold compactifications. In this paper we study a new class of heterotic-string models in which the GUT group is SU(6)xSU(2) at the string level. We use our recently developed fishing algorithm to extract an example of a three generation SU(6)xSU(2) GUT model. We explore the phenomenology of the model and show that it contains the required symmetry breaking Higgs representations. We show that the model admits flat directions that produce a Yukawa coupling for a single family. The novel feature of the SU(6)xSU(2) string GUT models is that they produce an additional family universal anomaly free U(1)symmetry that may remain unbroken below the string scale. The massless spectrum of the model is free of exotic states.
description: 20 pages. Standard LaTeX
Running coupling and pomeron loop effects on inclusive and diffractive DIS cross sections
Creators: name: Ducati, M. B. Gay
name: de Oliveira, E. G.
name: Amaral, J. T. de Santana
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Within the framework of a (1+1)--dimensional model which mimics high energy QCD, we study the behavior of the cross sections for inclusive and diffractive deep inelastic $γ^*h$ scattering cross sections. We analyze the cases of both fixed and running coupling within the mean field approximation, in which the evolution of the scattering amplitude is described by the Balitsky-Kovchegov equation, and also through the pomeron loop equations, which include in the evolution the gluon number fluctuations. In the diffractive case, similarly to the inclusive one, the suppression of the diffusive scaling, as a consequence of the inclusion of the running of the coupling, is observed.
description: 10 pages, 8 figures, submitted to Eur. Phy. J. C
Additional file 3 of Evaluation of safety and efficacy of autologous oral mucosa-derived epithelial cell sheet transplantation for prevention of anastomotic restenosis in congenital esophageal atresia and congenital esophageal stenosis
Creators: name: Fujino, Akihiro
name: Fuchimoto, Yasushi
name: Mori, Teizaburo
name: Kano, Motohiro
name: Yamada, Yohei
name: Ohno, Michinobu
name: Baba, Yoshiyuki
name: Isogawa, Nobutaka
name: Arai, Katsuhiro
name: Yoshioka, Takako
name: Abe, Makoto
name: Kanai, Nobuo
name: Takagi, Ryo
name: Maeda, Masanori
name: Umezawa, Akihiro
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Hematology

description: Additional file 3: Table S3. Quality control tests for oral mucosal epithelial cell sheets.
Non-perturbative description of self-interacting charged scalar field at finite temperature and in the presence of an external magnetic field
Creators: name: Duarte, D. C.
name: Farias, R. L. S.
name: Ramos, R. O.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Superconductivity (cond-mat.supr-con)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: It is studied the symmetry restoration in a theory of a self-interacting charged scalar field at finite temperature and in the presence of an external magnetic field. The effective potential is evaluated nonperturbatively through the Optimized Perturbation Theory (OPT) nonperturbative method. In addition, we present an efficient numeric way to deal with the sum over the Landau levels in the case of working with weak magnetic fields
description: 3 pages, 4 figures, Proceedings contribution for Hadrons XII
Dual Trigger of Transverse Oscillations in a Prominence by EUV Fast and Slow Coronal Waves: SDO/AIA and STEREO/EUVI Observations
Creators: name: Gosain, Sanjay
name: Foullon, Claire
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We analyze flare-associated transverse oscillations in a quiescent solar prominence on 8-9 September, 2010. Both the flaring active region and the prominence were located near the West limb, with a favorable configuration and viewing angle. The fulldisk extreme ultraviolet (EUV) images of the Sun obtained with high spatial and temporal resolution by the Atmospheric Imaging Assembly (AIA) aboard the Solar Dynamics Observatory, show flare-associated lateral oscillations of the prominence sheet. The STEREO-A spacecraft, 81.5 degrees ahead of the Sun-Earth line, provides on-disk view of the flare-associated coronal disturbances. We derive the temporal profile of the lateral displacement of the prominence sheet by using the image cross-correlation technique. The displacement curve was de-trended and the residual oscillatory pattern was derived. We fit these oscillations with a damped cosine function with a variable period and find that the period is increasing. The initial oscillation period (P0) is 28.2 minutes and the damping time (t_D) of 44 minutes. We confirm the presence of fast and slow EUV wave components. Using STEREO-A observations we derive a propagation speed of 250 km/s for the slow EUV wave by applying time-slice technique to the running difference images. We propose that the prominence oscillations are excited by the fast EUV wave while the increase in oscillation period of the prominence is an apparent effect, related to a phase change due to the slow EUV wave acting as a secondary trigger. We discuss implications of the dual trigger effect for coronal prominence seismology and scaling law studies of damping mechanisms.
description: 14 pages, 8 figures, to appear in Astrophysical Journal
Importance of cooling in triggering the collapse of hypermassive neutron stars
Creators: name: Paschalidis, Vasileios
name: Etienne, Zachariah B.
name: Shapiro, Stuart L.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The inspiral and merger of a binary neutron star (NSNS) can lead to the formation of a hypermassive neutron star (HMNS). As the HMNS loses thermal pressure due to neutrino cooling and/or centrifugal support due to gravitational wave (GW) emission, and/or magnetic breaking of differential rotation it will collapse to a black hole. To assess the importance of shock-induced thermal pressure and cooling, we adopt an idealized equation of state and perform NSNS simulations in full GR through late inspiral, merger, and HMNS formation, accounting for cooling. We show that thermal pressure contributes significantly to the support of the HMNS against collapse and that thermal cooling accelerates its "delayed" collapse. Our simulations demonstrate explicitly that cooling can induce the catastrophic collapse of a hot hypermassive neutron star formed following the merger of binary neutron stars. Thus, cooling physics is important to include in NSNS merger calculations to accurately determine the lifetime of the HMNS remnant and to extract information about the NS equation of state, cooling mechanisms, bar instabilities and B-fields from the GWs emitted during the transient phase prior to BH formation.
description: 13 pages, 7 figures, matches published version
Functionals on Triangulations of Delaunay Sets
Creators: name: Dolbilin, Nikolay P.
name: Edelsbrunner, Herbert
name: Glazyrin, Alexey
name: Musin, Oleg R.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Metric Geometry (math.MG)
subject: FOS: Mathematics

description: We study densities of functionals over uniformly bounded triangulations of a Delaunay set of vertices, and prove that the minimum is attained for the Delaunay triangulation if this is the case for finite sets.
description: 8 pages, 2 figures
Magnetic-coupling-dependent spin-triplet supercurrents in helimagnet/ferromagnet Josephson junctions
Creators: name: Halász, Gábor B.
name: Blamire, M. G.
name: Robinson, J. W. A.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The experimental achievements during the past year in demonstrating the existence of long-ranged spin-triplet supercurrents in ferromagnets proximity coupled to singlet superconductors open up the possibility for new interesting physics and applications [for a review, see M. Eschrig, Phys. Today 64(1), 43 (2011)]. Our group reported the injection of triplet supercurrents into a magnetically uniform ferromagnet (Co) by sandwiching it between two helimagnet/superconductor (Ho/Nb) bilayers to form a Nb/Ho/Co/Ho/Nb-type Josephson device. In the function of the Ho layer thicknesses, the supercurrent was found to modulate in a complex way that seemed to depend on the magnetic structure of Ho. To understand this unusual behavior, we have theoretically studied the properties of an ideal Josephson device with a helimagnet/ferromagnet/helimagnet (HM/F/HM) barrier in the clean limit using the Eilenberger equation; we show, in particular, that the maximum triplet supercurrent that can pass across the barrier will depend non-monotonically on the thicknesses of the HM layers if the HM and F layers are magnetically exchange coupled at their interface.
description: 5 pages, 3 figures
Herbert Reiter, Politisches Asyl im 19. Jahrhundert. Die deutschen politischen Flüchtlinge des Vormärz und der Revolution von 1848/49 in Europa und in den USA, 1992
Creators: name: McClelland, Charles E.
Publisher: name: Francia
Year: 2019

description: -
description: Francia, Bd. 21, Nr. 3 (1994)
Resolving Azimuth Ambiguity Using Vertical Nature of Solar Quiet-Sun Magnetic Fields
Creators: name: Gosain, Sanjay
name: Pevtsov, Alexei A.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The measurement of solar magnetic fields using the Zeeman effect diagnostics has a fundamental 180 degree ambiguity in the determination of the azimuth angle of the transverse field component. There are several methods that are used in the community and each one has its merits and demerits. Here we present a disambiguation idea that is based on the assumption that most of the magnetic field on the sun is predominantly vertical. While the method is not applicable to penumbra or other features harboring predominantly horizontal fields like the sheared neutral lines, it is useful for regions where fields are predominantly vertical like network and plage areas. The method is tested with the full-disk solar vector magnetograms observed by the VSM/SOLIS instrument. We find that statistically about 60-85 % of the pixels in a typical full-disk magnetogram has field inclination in the range of 0-30 degrees with respect to the local solar normal, and thus can be successfully disambiguated by the proposed method. Due to its non-iterative nature, the present method is extremely fast and therefore can be used as a good initial guess for iterative schemes like nonpotential field computation (NPFC) method. Furthermore, the method is insensitive to noisy pixels as it does not depend upon the neighboring pixels or derivatives.
description: 12 pages, 5 figures, in Solar Physics