Academic literature on the topic 'AlMn System'

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Journal articles on the topic "AlMn System"

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Lilienfeld, D. A., M. Nastasi, H. H. Johnson, D. G. Ast, and J. W. Mayer. "The quasicrystalline transformation in the AlCr system." Journal of Materials Research 1, no. 2 (April 1986): 237–42. http://dx.doi.org/10.1557/jmr.1986.0237.

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Amorphous Al80Cr20 films were made by coevaporation and by room temperature ion irradiation of the coevaporated films. The amorphous phase was transformed into the quasicrystalline state through two routes: thermal and ion beam assisted anneal. The intensity of the quasicrystalline electron diffraction pattern increases continuously within the annealing temperature range from 547°to 607°C. The starting state of the films (as-deposited or ion-irradiated codeposited) had no effect on the thermal transformation to the quasicrystalline state. Ion irradiation of the amorphous phase at 200°C produces a more complete set of icosahedral diffraction lines. Icosahedral AlCr has the same reciprocal lattice spacings as icosahedral AlMn.
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Kang, Byung-Sub, Kwang-Pyo Chae, and Haeng-Ki Lee. "Half-Metallic Ferromagnetism in Chalcopyrite (AlGaMn)P2Alloys." Advances in Condensed Matter Physics 2015 (2015): 1–7. http://dx.doi.org/10.1155/2015/706957.

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We studied the electronic and magnetic properties of (Al1−yMny)GaP2(Ga-rich) and Al(Ga1−yMny)P2(Al-rich) withy = 0.03125, 0.0625, 0.09375, and 0.125 by using the first-principles calculations. The ferromagnetic Mn-doped AlGaP2chalcopyrite is the most energetically favorable one. The spin polarized Al(GaMn)P2state (Al-rich system) is more stable than spin polarized (AlMn)GaP2state (Ga-rich) with the magnetic moment of 3.8 μB/Mn. The Mn-doped AlGaP2yields strong half-metallic ground states. The states of host Al, Ga, or P atoms at the Fermi level are mainly a P-3pcharacter, which mediates a strong interaction between the Mn-3dand P-3pstates.
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Vlach, Martin, Ivana Stulíková, Bohumil Smola, Hana Kudrnova, Tomáš Kekule, Jaroslav Malek, and Vladivoj Ocenasek. "Phase Transformations and Recrystallization in Cold-Rolled Al–Mn, Al–Sc–Zr and Al–Mn–Sc–Zr Alloy." Defect and Diffusion Forum 354 (June 2014): 93–100. http://dx.doi.org/10.4028/www.scientific.net/ddf.354.93.

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The effect of cold-rolling on mechanical and electrical properties, microstructure and recrystallization behaviour of the AlMn, AlScZr and AlMnScZr alloys was studied. The materials were investigated during isothermal annealing at 300, 400, 500 and 550°C and during step-by-step quasilinear annealing from 200°C up to 600°C with a heating rate of 100 K/h followed by subsequent isothermal annealing at 600°C/5 h. Precipitation reactions were studied by electrical resistometry and (micro) hardness measurements. The microstructure development was investigated by electron microscopy and electron backscatter diffraction examinations. The hardening effect is due to uniformly distributed Al3Sc and/or Al3(Sc,Zr) particles. The distinct changes in resistivity of the alloys above ∼ 300°C are mainly caused by precipitation of Mn-containing particles. It has a negligible effect on hardness. Phase transformations in the AlMn and AlMnScZr alloys are highly enhanced by cold rolling. The precipitation is dependent on the deformation degree – the more deformation the more intensive precipitation of the Mn-containing particles. The combination of Mn, Sc and Zr additions to Al substantially suppresses recrystallization at 550°C. A partial recrystallization was observed in the AlScZr alloy and AlMnScZr alloy after annealing 550°C/60 min and 550°C/760 min, respectively. The decomposition sequence of the supersaturated solid solution of the AlMnScZr alloy is compatible with the decomposition sequence of the AlScZr system accompanied and/or followed by the formation of Mn-containing particles.
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Snitovsky, Yuri P. "Changes in the physical and mechanical properties of aluminum depending on the composition of the alloying elements." Yugra State University Bulletin 18, no. 4 (January 14, 2023): 68–76. http://dx.doi.org/10.18822/byusu20220468-76.

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Subject of research: the influence of the concentration and composition of alloying elements Mn, Ti, Cr, Y, Mo, W, V on the change in the aluminum recrystallization temperature. Purpose of research: to find the optimal concentration of alloying additives, at which the recrystallization temperature reaches its maximum value. Methods and objects of research: using the methods of thermodynamic analysis of binary state diagrams of aluminum with alloying additives, it has been established that the nature of the change in the recrystallization temperature depends on what type of eutectic or peritectic reaction the formation of intermetallic compounds belongs to. It is shown that aluminides act as alloy modifiers and impart high mechanical properties to products. Main results of research: it was found that for the AlMn system, the optimal content of Mn should be considered 0.2%, for the AlCr system, the maximum increase in the Al recrystallization temperature is observed at 0.6% Cr, for the AlY system, the mechanical properties of Al at elevated temperatures maximum at 1% Y.
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Zupanič, Franc, Boštjan Markoli, Iztok Naglič, Tobias Weingärtner, Anton Meden, and Tonica Bončina. "Phases in the Al-Corner of the Al–Mn–Be System." Microscopy and Microanalysis 19, no. 5 (June 18, 2013): 1308–16. http://dx.doi.org/10.1017/s1431927613001852.

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AbstractThis work studied the phases in the Al corner of the Al–Mn–Be phase diagram in the as-cast state and heat-treated conditions. Metallographic investigations, X-ray diffraction, scanning electron microscopy, and energy-dispersive spectroscopy were used for identifying the phases. The Be contents in the identified phases were precisely determined using Auger electron spectroscopy. The results indicated that Al6Mn does not dissolve Be, whilst λ-Al4Mn dissolves up to 7 at.% Be. The average composition of the T phase, which is normally designated as Al15Mn3Be2, was 72 at.% Al, 19 at.% Mn, and 9 at.% Be. The phase with the nominal composition Be4AlMn contained more Al than Mn. The atomic ratio Al:Mn was between 1.3:1 and 2:1. The hexagonal Be-rich phase did not dissolve any Al and Mn. The icosahedral quasicrystalline (IQC) phase contained up to 45 at.% Be. The compositions of T phase, λ–Al4Mn, IQC, and Be4AlMn may vary, however, the ratio (Al + Be):Mn remained constant, and was close either to four or six indicating substitution of Al atoms with Be atoms in these phases.
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ÇIRAK, Ezgi. "AN EVALUATION OF THE CURRENT REGULATIONS IN TURKISH AND GERMAN LEGAL SYSTEMS REGARDING CRIMINAL LIABILITY FOR THE DISCLOSURE OF TRADE SECRETS." Ticaret ve Fikri Mülkiyet Hukuku Dergisi 8, no. 1 (June 30, 2022): 179–206. http://dx.doi.org/10.55027/tfm.1053471.

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Ticari sır, bir ticarî işletme veya şirketin faaliyet alanı ile ilgili olarak bağımsız ve ekonomik bir değeri olan veya sır sahibine rekabette avantaj sağlayan ve piyasada ilgili işletmeye başarı getiren, sınırlı bir çevre tarafından bilinen ve sahibinin alenileşmesini istemediği her türlü üretim, iş, pazarlama gibi hususlardaki bilgi, belge ve verilerdir. Ticari sırrın hukuka aykırı olarak ifşası, sır sahibine iktisadi açıdan zarar vereceği gibi serbest piyasa ekonomisinin istikrarını ve güvenini de zedeleyecektir. Ticari sırların ifşasının önlenmesi ve buna yönelik eylemlerin caydırıcılığının sağlanması için ceza hukukunun himayesi gerekli görülmektedir. Bu bağlamda hem Türk hukukunda hem de Alman hukukunda cezai düzenlemeler yer almaktadır. Ticari sırrın ve serbest piyasa ekonomisinin korunmasına yönelik olarak Türk Ticaret Kanunu (TTK) 62/1-a maddesinin atfıyla TTK madde 55/1-b-3 ve TTK madde 55/1-d bentlerinde yer alan fiiller, ticari sırların ifşasına ilişkin olarak TTK madde 62/1-a’daki haksız rekabet suçunun seçimlik hareketleri arasında düzenlenmiştir. Ayrıca TTK madde 62/1-c’de ticari sırların ele geçirilmesi suçu yer almaktadır. Bunun yanında korunan hukuki değer farklı olsa da suçun konusu bakımından benzer bir düzenleme Türk Ceza Kanunu’nun (TCK) 239. maddesinde ticarî sır, bankacılık sırrı veya müşteri sırrı niteliğindeki bilgi veya belgelerin açıklanması suçu yer almaktadır. Bu düzenlemeler birbirinden suça konu olan sırrın hukuka uygun ya da hukuka aykırı olarak elde edilip edilmediğine göre, sırrı bizzat ifşa etme ya da ifşaya yöneltme hareketine göre ayrılmaktadır. Ayrıca iki farklı kanunda yer alan bu düzenlemeler, suçun konusu bakımından benzer olduklarından somut olaya uygulanabilirlikleri ayrıca değerlendirilmelidir. Alman Haksız Rekabet Kanunu’nun (UWG) §17 ise iş ve işletme sırlarının ifşası suçunu düzenlemekteydi. Ancak Avrupa Birliği’nin 2016/943 sayılı Direktifi’ne uyum çalışmaları sonucunda UWG’de yer alan cezai yaptırımlar mülga edilip Ticari Sırların Korunması Kanunu’nun (GeschGehG) § 23 yeniden düzenlenmiş ancak suçun kapsamına giren haller GeschGehG’de yer alan diğer maddelere atıf yapılmak suretiyle düzenlenmiştir. Bunun yanında Alman Ceza Kanunun (StGB) § 203’te özel sırların ihlali suçu da ayrıca düzenlenmektedir. Ticari sırrın ifşasına yönelik suçlar her iki ülkenin mevzuatında da dağınık bir şekilde ele alınıp, eksik norm yöntemi ile düzenlenmiştir. Bu durum somut olaya hangi suç tipinin ya da suçun hangi seçimlik hareketinin uygulanması gerektiği konusunda problemlere neden olmaktadır. Bu bakımdan çalışmada ilgili suç tiplerinin ele alınış biçimleri, uygulama alanlarının sınırları ve ayrımları ele alınacaktır. Her bir suç tipinin unsurlarına ayrılarak incelenmesi daha detaylı bir çalışma gerektirdiğinden, bu çalışmada konuya ilişkin suç tiplerinin genel hatlarıyla ortaya konulması amaçlanmaktadır.
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ITO, Noboru, and Masaya INOUE. "Direct Drive System for ALMA Antenna." Journal of The Institute of Electrical Engineers of Japan 130, no. 4 (2010): 212–15. http://dx.doi.org/10.1541/ieejjournal.130.212.

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Wong, Sandra. "Database Discovery: From a Migration Project to a Content Strategy." Library Resources & Technical Services 64, no. 2 (May 8, 2020): 72. http://dx.doi.org/10.5860/lrts.64n2.72.

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After migrating to Ex Libris’s Alma and Primo for its integrated library system (ILS) and discovery layer, library staff at Simon Fraser University (SFU) maintained duplicate database information in a locally developed electronic resources management (ERM) system known as the CUFTS ERM for fifteen months. The CUFTS ERM provided the data for the library’s public-facing database list known as the CUFTS resource database (CRDB). A database search function had been on Ex Libris’s Primo roadmap for product development and was announced six months after the library went live with Alma and Primo. However, the new Primo database search function lacked the ability to replace the CRDB. Members of the library’s ILS Steering Committee who managed Alma and Primo were concerned about significant negative impacts on end-users if the library adopted Primo to replace the CRDB. The steering committee formed a task group to investigate options for creating a database list from Alma records to reduce duplication of staff time and effort, and systems resources, and to replicate the main functions of the existing CRDB for end-user discovery and access.
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Marino, S., M. C. Wyatt, G. M. Kennedy, W. Holland, L. Matrà, A. Shannon, and R. J. Ivison. "ALMA observations of the multiplanet system 61 Vir: what lies outside super-Earth systems?" Monthly Notices of the Royal Astronomical Society 469, no. 3 (May 6, 2017): 3518–31. http://dx.doi.org/10.1093/mnras/stx1102.

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Yang, Yushi, Antonia Joy Rivera, Christopher R. Fortier, and James H. Abernathy. "A Human Factors Engineering Study of the Medication Delivery Process during an Anesthetic." Anesthesiology 124, no. 4 (April 1, 2016): 795–803. http://dx.doi.org/10.1097/aln.0000000000001040.

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Abstract Background Prefilled syringes (PFS) have been recommended by the Anesthesia Patient Safety Foundation. However, aspects in PFS systems compared with self-filled syringes (SFS) systems have never been explored. The aim of this study is to compare system vulnerabilities (SVs) in the two systems and understand the impact of PFS on medication safety and efficiency in the context of anesthesiology medication delivery in operating rooms. Methods This study is primarily qualitative research, with a quantitative portion. A work system analysis was conducted to analyze the complicated anesthesia work system using human factors principles and identify SVs. Anesthesia providers were shadowed: (1) during general surgery cases (n = 8) exclusively using SFS and (2) during general surgery cases (n = 9) using all commercially available PFS. A proactive risk assessment focus group was followed to understand the risk of each identified SV. Results PFS are superior to SFS in terms of the simplified work processes and the reduced number and associated risk of SVs. Eight SVs were found in the PFS system versus 21 in the SFS system. An SV example with high risk in the SFS system was a medication might need to be “drawn-up during surgery while completing other requests simultaneously.” This SV added cognitive complexity during anesthesiology medication delivery. However, it did not exist in the PFS system. Conclusions The inclusion of PFS into anesthesiology medication delivery has the potential to improve system safety and work efficiency. However, there were still opportunities for further improvement by addressing the remaining SVs and newly introduced complexity.
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Dissertations / Theses on the topic "AlMn System"

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Ricci, L., P. Cazzoletti, I. Czekala, S. M. Andrews, D. Wilner, L. Szűcs, G. Lodato, et al. "ALMA Observations of the Young Substellar Binary System 2M1207." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624920.

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We present ALMA observations of the 2M1207 system, a young binary made of a brown dwarf with a planetary-mass companion at a projected separation of about 40 au. We detect emission from dust continuum at 0.89 mm and from the J = 3 - 2 rotational transition of CO from a very compact disk around the young brown dwarf. The small radius found for this brown dwarf disk may be due to truncation from the tidal interaction with the planetary-mass companion. Under the assumption of optically thin dust emission, we estimate. a dust mass of 0.1 M-circle plus. for the 2M1207A disk and a 3 sigma upper limit of similar to 1 M-Moon for dust surrounding 2M1207b, which is the tightest upper limit obtained so far for the mass of dust particles surrounding a young planetary-mass companion. We discuss the impact of this and other non-detections of young planetary-mass companions for models of planet formation that predict circumplanetary material to surround these objects.
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Naischtein, Katja. "Vem är Alma? : Ett aktör-nätverksperspektiv på bibliotekens IT-system." Thesis, Uppsala universitet, Institutionen för ABM, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-352611.

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Today’s library acquisition, circulation, metadata management, cataloging and administration of all kind of resources are too laborious and cannot be performed manually. These tasks are run by or with the help of an IT-system. This master thesis aims to start an analytical discussion of the modern library's central tool, library IT-systems, a discussion much missing in Library and Infor-mation Science. The data on two library IT-systems Alma and Sierra was collected by partici-pant observations, interviews and document studies at Karolinska institute university library and Södertörns university college library.The data was analyzed through actor-network theory perspective. The study’s main questions are how the library IT-system actor-network is assembled and function, and what role does the technology play in library’s practices.The study shows that a complex actor-network emerges in order to automate and computerize library tasks. In this actor-network library IT-systems vendors, the library community, KIB’s and SHB’s practices and the technology are actors who actively impact and affect each other. They are associated with each other through negotiations, a process in ANT referred to as translation. The study also shows that as the actors are not completely in agreement with each other, the library IT-system actor-network has not yet transformed into a fully convergent actor-network which ANT compares to a black box. The study shows that nonhumans, the IT-systems, are not neutral tools. They mediate, organize and document library practices. But they are also a product of modern library knowledge.The study concludes that the fully functioning solution for libraries automated and computer-ized services is the joined production of human and nonhuman actor-network where IT technology play a mediating role.
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MacGregor, Meredith A., David J. Wilner, Ian Czekala, Sean M. Andrews, Y. Sophia Dai, Gregory J. Herczeg, Kaitlin M. Kratter, Adam L. Kraus, Luca Ricci, and Leonardo Testi. "ALMA MEASUREMENTS OF CIRCUMSTELLAR MATERIAL IN THE GQ LUP SYSTEM." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/622871.

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We present Atacama Large Millimeter/submillimeter Array observations of the GQ Lup system, a young Sun-like star with a substellar-mass companion in a wide-separation orbit. These observations of 870 mu m continuum and CO J = 3-2 line emission with beam size similar to 0."3 (similar to 45 au) resolve the disk of dust and gas surrounding the primary star, GQ Lup A, and provide deep limits on any circumplanetary disk surrounding the companion, GQ Lup b. The circumprimary dust disk is compact with an FWHM of 59 +/- 12 au, while the gas has a larger extent with a characteristic radius of 46.5 +/- 1.8 au. By forward-modeling the velocity field of the circumprimary disk based on the CO emission, we constrain the mass of GQ Lup. A to be M-* = (1.03 +/- 0.05) * (d/156 pc) M-circle dot, where d is a known distance, and determine that we view the disk at an inclination angle of 60 degrees 5 +/- 0 degrees 5 and a position angle of 346 degrees +/- 1 degrees. The 3s upper limit on the 870 mu m flux density of any circumplanetary disk associated with GQ Lup b of <0.15 mJy implies an upper limit on the dust disk mass of <0.04M(circle dot) for standard assumptions about optically thin emission. We discuss proposed mechanisms for the formation of wide-separation substellar companions given the non-detection of circumplanetary disks around GQ Lup b and other similar systems.
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Tapia, Labarca Valeria Victoria. "Design and measurements of an optical system for Alma Band 1." Tesis, Universidad de Chile, 2015. http://repositorio.uchile.cl/handle/2250/133513.

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Magíster en Ingeniería Eléctrica
El proyecto astronómico ALMA, Atacama Large Millimeter/submillimeter Array, es el radiobservatorio interferométrico más grande del mundo. Se compone de 66 antenas con diámetros de 7 y 12~m, ubicadas en el norte de Chile a una altitud de 5000~m sobre el nivel del mar. Su excelente localización y tecnología proveerán sensibilidad y resolución sin presedentes para el estudio de los origenes del universo, formación y evolución de galaxias, estrellas, planetas y la compleja química del medio interestelar. Por ello, ALMA constituye un gran desafío en diversas áreas de la ciencia y la tecnología. En esta tesis se presenta el diseño, contrucción y caracterización del sistema óptico para el receptor heterodino de la Banda 1 de ALMA. Este sistema combina una serie de exigentes especificaciones técnicas, limitaciones de construcción y restricciones de costo que requieren equilibrarse. El sistema debe cubrir el rango de frecuencia entre 35-50 GHz (con el objetivo de extenderlo hasta 52 GHz) sin ninguna sintonización mecánica, lograr un eficiencia de apertura para toda la banda que supere el 80%, poseer una apertura de polarización superior a 99.5%, incluir en torno a 10 K de ruido, poseer un error de alineamiento menor a 5~mrad respecto a la posición nominal y no debe interferir con los dispositivos ya existentes. Además, el sistema debe ser compatible para las antenas de 7 y 12 m, que poseen un ángulo de iluminación distinto al secundario. El sistema óptico consiste en una antena tipo bocina compacta corrugada, una membrana de gore-tex y membrana ranurada de teflón como filtros de las etapas de 15 y 110 K, respectivamente, y un lente con zona biconvexo fabricado de polietileno que incluye corrugaciones como capa anti-reflectora. Está tesis se enfoca en la antena tipo bocina y el lente. El proceso de diseño de los dipositivos se realizó de manera iterativa, por lo que dos modelos de antenas tipo bocina y tres lentes de una zona son presentados. El diseño de las antenas consistió en determinar las características necesarias del patrón radiativo utilizando modelos cuasiópticos. Luego se optimizó su perfil utilizando ténicas de adaptación modal y algoritmos genéticos. El procedimiento de diseño de lentes fue similar al utilizado para la bocina. Primero, se consideraron como parámetros iniciales los valores calculados mediante el modelo quasioptico y luego se realizaron análisis de sensibilidad utilizando la ténica de método de los momentos y método de elementos finitos. El mejor sistema en simulación corresponde a la segunda versión de la antena y la tercera del lente. Este sistema cumple totalmente las especificaciones mencionadas, logrando eficiencias de apertura mejores que 80.4% para toda la banda. La temperaturas de ruido promedio calculada es de 10.4 K, donde el lente presenta la mayor contribución con aproximadamente 7 K. Además, el sistema es compatible para la antena de 7 y 12 m, si el lente se desplaza 5.66 mm hacia el centro del criostato en la configuración de 7 m, con degradaciones en eficiencia de apertura menores a 0.5%. Por último se presentan dos sistemas caracterizados, correspondientes a la primera antena más la primera o segunda lente, pues al momento de escribir esta tesis, el resto de dispositivos se encontraban en construcción. El mejor sistema medido poseen eficiencias de apertura mejores que 79.2% en excelente concordancia con las simulaciones. Además, se han identificado algunas fuentes de error que poseen las mediciones, incluyendo errores en alineamientos y cambios de fase por temperatura.
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MacGregor, Meredith A., Luca Matra, Paul Kalas, David J. Wilner, Margaret Pan, Grant M. Kennedy, Mark C. Wyatt, et al. "A Complete ALMA Map of the Fomalhaut Debris Disk." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624433.

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We present ALMA mosaic observations at 1.3. mm (223 GHz) of the Fomalhaut system with a sensitivity of 14 mu Jy/beam. These observations provide the first millimeter map of the continuum dust emission from the complete outer debris disk with uniform sensitivity, enabling the first conclusive detection of apocenter glow. We adopt an MCMC modeling approach that accounts for the eccentric orbital parameters of a collection of particles within the disk. The outer belt is radially confined with an inner edge of 136.3 +/- 0.9. au and width of 13.5 +/- 1.8. au. We determine a best-fit eccentricity of 0.12 +/- 0.01. Assuming a size distribution power-law index of q. =. 3.46 +/- 0.09, we constrain the dust absorptivity power-law index a to be 0.9
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Booth, Mark, William R. F. Dent, Andrés Jordán, Jean-François Lestrade, Antonio S. Hales, Mark C. Wyatt, Simon Casassus, et al. "The Northern arc of ε Eridani’s Debris Ring as seen by ALMA." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/625481.

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We present the first Atacama Large Millimeter/submillimeter Array (ALMA) observations of the closest known extrasolar debris disc. This disc orbits the star is an element of Eri, a K-type star just 3.2 pc away. Due to the proximity of the star, the entire disc cannot fit within the ALMA field of view. Therefore, the observations have been centred 18" North of the star, providing us with a clear detection of the Northern arc of the ring, at a wavelength of 1.3 mm. The observed disc emission is found to be narrow with a width of just 11-13 AU. The fractional disc width we find is comparable to that of the Solar system's Kuiper Belt and makes this one of the narrowest debris discs known. If the inner and outer edges are due to resonances with a planet then this planet likely has a semi-major axis of 48 AU. We find tentative evidence for clumps in the ring, although there is a strong chance that at least one is a background galaxy. We confirm, at much higher significance, the previous detection of an unresolved emission at the star that is above the level of the photosphere and attribute this excess to stellar chromospheric emission.
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SPINELLI, FABRIZIO. "Single-minded intention commitment strategy in ALAN." Doctoral thesis, Università Politecnica delle Marche, 2011. http://hdl.handle.net/11566/241996.

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L'obiettivo di questa tesi è quello di introdurre il concetto di obbligazione in ALAN, un linguaggio di programmazione orientato agli agenti-oggetti che permette di fondere il paradigma di programmazione orientato agli oggetti con quello orientato agli agenti.In particolare l'attenzione è rivolta all'introduzione di una strategia di obbligazione "single-minded" per le intenzioni che permetterà ad un agente modellato in ALAN di poter reagire in maniera significativa ai cambiamenti che avvengono nel suo ambiente.Per poter ottenere tale risultato prima di tutto viene analizzata la strategia di obbligazione delle intenzioni attualmente adottata nel linguaggio, dopodichè un insieme di modifiche da apportare sia al modello che alla semnatica operazionale del linguaggio vengono proposte ed applicate allo stesso.Nella tesi viene introdotta anche una nuova architettura parallela per gli agenti. L'architettura proposta non solo permette l'implementazione della strategia di obbligazione "single-minded" delle intenzioni tenendo in considerazione e limitando il possibile degrado delle prestazioni del sistema, ma permette anche agli agenti di esguire in maniera concorrente le loro fasi di percezione, di ragionamento e di attuazione, conducendo alla creazione di agenti più capaci e reattivi.
The aim of this thesis is to introduce the concept of commitment in ALAN, an agent-object oriented programming language that fuses the object oriented and the agent oriented programming paradignms. In order to achieve such result first the actual intention commitment strategy embodied in the languages is analyzed, then a set of modification to both the language model and to its operational semantics is proposed and applied to the language.The thesis also introduces a new parallel architecture for the agents. The proposed architecture not only permits the implementation of the single-minded intention commitment strategy taking into account and limiting possible performance degradation of the system, but also allows agents to execute concurrently their sensing, thinking and acting phases, leading to more reactive and capable agents.
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Winter, Matthias. "Concentrated patterns in biological systems." [S.l. : s.n.], 2003. http://www.bsz-bw.de/cgi-bin/xvms.cgi?SWB11163816.

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Eisner, J. A., J. M. Bally, A. Ginsburg, and P. D. Sheehan. "PROTOPLANETARY DISKS IN THE ORION OMC1 REGION IMAGED WITH ALMA." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621374.

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We present ALMA observations of the Orion Nebula that cover the OMC1 outflow region. Our focus in this paper is on compact emission from protoplanetary disks. We mosaicked a field containing similar to 600 near-IR-identified young stars, around which we can search for sub-millimeter emission tracing dusty disks. Approximately 100 sources are known proplyds identified with the Hubble Space Telescope. We detect continuum emission at 1 mm wavelengths toward similar to 20% of the proplyd sample, and similar to 8% of the larger sample of near-IR objects. The noise in our maps allows 4 sigma detection of objects brighter than similar to 1.5 mJy, corresponding to protoplanetary disk masses larger than 1.5 M-J (using standard assumptions about dust opacities and gas-to-dust ratios). None of these disks are detected in contemporaneous CO(2-1) or (CO)-O-18(2-1) observations, suggesting that the gas-to-dust ratios may be substantially smaller than the canonical value of 100. Furthermore, since dust grains may already be sequestered in large bodies in Orion Nebula cluster (ONC) disks, the inferred masses of disk solids may be underestimated. Our results suggest that the distribution of disk masses in this region is compatible with the detection rate of massive planets around M dwarfs, which are the dominant stellar constituent in the ONC.
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Long, Feng, Gregory J. Herczeg, Ilaria Pascucci, Emily Drabek-Maunder, Subhanjoy Mohanty, Leonardo Testi, Daniel Apai, et al. "An ALMA Survey of CO Isotopologue Emission from Protoplanetary Disks in Chamaeleon I." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/625159.

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The mass of a protoplanetary disk limits the formation and future growth of any planet. Masses of protoplanetary disks are usually calculated from measurements of the dust continuum emission by assuming an interstellar gas-to-dust ratio. To investigate the utility of CO as an alternate probe of disk mass, we use ALMA to survey (CO)-C-13 and (CO)-O-18 J = 3-2 line emission from a sample of 93 protoplanetary disks around stars and brown dwarfs with masses from 0.03 to 2 M-circle dot in the nearby Chamaeleon I star-forming region. We detect (CO)-C-13 emission from 17 sources and (CO)-O-18 from only one source. Gas masses for disks are then estimated by comparing the CO line luminosities to results from published disk models that include CO freeze-out and isotope-selective photodissociation. Under the assumption of a typical interstellar medium CO-to-H-2 ratio of 10(-4), the resulting gas masses are implausibly low, with an average gas mass of similar to 0.05M(Jup) as inferred from the average flux of stacked (CO)-C-13 lines. The low gas masses and gas-to-dust ratios for Cha I disks are both consistent with similar results from disks in the Lupus star-forming region. The faint CO line emission may instead be explained if disks have much higher gas masses, but freeze-out of CO or complex C-bearing molecules is underestimated in disk models. The conversion of CO flux to CO gas mass also suffers from uncertainties in disk structures, which could affect gas temperatures. CO emission lines will only be a good tracer of the disk mass when models for C and CO depletion are confirmed to be accurate.
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Books on the topic "AlMn System"

1

Tuccille, Jerome. Alan Shrugged. New York: John Wiley & Sons, Ltd., 2002.

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Alan, Simpson. Alan Simpson's Windows XP bible. 2nd ed. Indianapolis, IN: Wiley Pub., 2005.

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Alan, Simpson. Alan Simpson's Windows XP bible. New York: Wiley, 2004.

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Alan, Simpson. Alan Simpson's Windows XP bible. New York, NY: Hungry Minds, 2001.

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Alan, Simpson. Alan Simpson's Windows XP Bible. New York: John Wiley & Sons, Ltd., 2004.

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Alan, Simpson. Alan Simpson's Windows XP Bible. New York: John Wiley & Sons, Ltd., 2005.

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Alan, Simpson. Alan Simpson's Windows Me Millennium edition bible. Foster City, Calif: IDG Books Worldwide, 2000.

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Alan shrugged: The life and times of Alan Greenspan, the world's most powerful banker. Hoboken, N.J: Wiley, 2002.

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Alan Simpson's DOS secrets unleashed. Carmel, Ind: Sams Pub., 1993.

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Alan Greenspan: The oracle behind the curtain. New Jersey: World Scientific, 2006.

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Book chapters on the topic "AlMn System"

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Huang, Zhenkun, and Laner Wu. "AlN-Based Ceramics Systems." In Phase Equilibria Diagrams of High Temperature Non-oxide Ceramics, 69–102. Singapore: Springer Singapore, 2018. http://dx.doi.org/10.1007/978-981-13-0463-7_3.

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Tomashyk, Vasyl. "Systems Based on AlN." In Quaternary Alloys Based on III-V Semiconductors, 51–91. Boca Raton, FL : CRC Press, Taylor & Francis Group, [2018]: CRC Press, 2018. http://dx.doi.org/10.1201/9780429508080-4.

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Vasyl, Tomashyk. "Systems Based on AlN." In Ternary Alloys Based on III-V Semiconductors, 37–62. Boca Raton, FL : CRC Press, Taylor & Francis Group, [2017]: CRC Press, 2017. http://dx.doi.org/10.1201/9781315116624-4.

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Bowen, Jonathan P. "Alan Turing: Founder of Computer Science." In Engineering Trustworthy Software Systems, 1–15. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-56841-6_1.

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Lu, Jianjiang, Baowen Xu, Yanhui Li, Dazhou Kang, and Peng Wang. "Extended Fuzzy ALCN and Its Tableau Algorithm." In Fuzzy Systems and Knowledge Discovery, 232–42. Berlin, Heidelberg: Springer Berlin Heidelberg, 2005. http://dx.doi.org/10.1007/11539506_30.

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Bacciotti, F., J. M. Girart, M. Padovani, L. Podio, R. Paladino, L. Testi, E. Bianchi, et al. "ALMA Polarimetric Studies of Rotating Jet/Disk Systems." In Astrophysics and Space Science Proceedings, 87–95. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-14128-8_13.

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Abbruzzese, F., E. Minicozzi, G. Nardiello, and G. Piazzullo. "Coordination and Dynamic Organization in the ALM System." In AI and Cognitive Science ’92, 44–55. London: Springer London, 1993. http://dx.doi.org/10.1007/978-1-4471-3207-3_5.

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Bowen, Jonathan P. "The Impact of Alan Turing: Formal Methods and Beyond." In Engineering Trustworthy Software Systems, 202–35. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-17601-3_5.

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Comai, Sara, Emanuele De Bernardi, Andrea Masciadri, Matteo Matteucci, Fabio Salice, and Fabio Veronese. "ALMA: An Indoor Localization and Navigation System for the Elderly." In Smart Objects and Technologies for Social Good, 82–91. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-76111-4_9.

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Lopes, Rui J., Laurent Mathy, and David Hutchison. "Bandwidth Measurements of ALM Trees for Content Distribution." In Protocols for Multimedia Systems, 89–102. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/3-540-45481-0_8.

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Conference papers on the topic "AlMn System"

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Vlasov, V., A. Klopotov, K. Bezukhov, N. Golobokov, M. Syrtanov, and G. Volokitin. "Study of the structure of SiAlON obtained by synthesis with low-temperature plasma energy." In 8th International Congress on Energy Fluxes and Radiation Effects. Crossref, 2022. http://dx.doi.org/10.56761/efre2022.c1-p-009301.

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This article presents the results of studies of the effect of low-temperature plasma on a sample prepared from powders Si 3 N, AlN, urea solution and liquid glass. X-ray phase analysis established, that the use of plasma chemical synthesis produced the phase β-SiAlON compositions Si 5 AlON 7 with hexagonal system (Pearson symbol hP14, space group P6 3 /m. The diffractograms also show an X-ray amorphous phase and traces of initial compounds. A diagram showing the physical and chemical processes occurring during the interaction of the plasma flux with components in plasma chemical synthesis is presented.
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Sramek, Richard, Koh-Ichiro Morita, Masahiro Sugimoto, Peter Napier, Maurizio Miccolis, Pavel Yagoubov, Denis Barkats, et al. "ALMA system verification." In SPIE Astronomical Telescopes + Instrumentation, edited by Larry M. Stepp, Roberto Gilmozzi, and Helen J. Hall. SPIE, 2012. http://dx.doi.org/10.1117/12.925449.

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Glendenning, B. E. "The ALMA software system." In 2011 XXXth URSI General Assembly and Scientific Symposium. IEEE, 2011. http://dx.doi.org/10.1109/ursigass.2011.6051290.

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Marchiori, Gianpietro, Francesco Rampini, Massimiliano Tordi, Matteo Spinola, and Riccardo Bressan. "From ALMA to Super-ALMA." In 2019 IEEE International Conference on Microwaves, Antennas, Communications and Electronic Systems (COMCAS). IEEE, 2019. http://dx.doi.org/10.1109/comcas44984.2019.8958113.

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Matthews, Jennifer K., and Christine Davidian. "Migrating to Alma Without an Acquisitions Staff: Evolving Acquisitions and Electronic Workflows From Their Legacy Silos." In Charleston Library Conference. Purdue Univeristy, 2020. http://dx.doi.org/10.5703/1288284317187.

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When the decision was made to migrate to Alma integrated library system, Rowan University libraries had an acquisitions department and a moderate understanding of how this migration would occur. With the official announcement of the migration to Alma, the entire acquisitions team announced their retirement shortly thereafter. While Alma provided the library with an opportunity to reevaluate workflows and collaborations this was a curveball that no one was expecting. Additionally, many resources were not traditionally tracked in Voyager, the previous library management system but tracked in Intota the previous electronic resource management system. However, these resources would now be tracked in Alma for a variety of reasons. This added another layer of complication to the retirements that occurred and the implementation that was well underway. This paper will discuss how Rowan University Libraries has managed the Alma migration without the historical institutional memory of the former acquisitions team. It will also examine how the libraries have examined workflows anew as a result of both the migration and these vacancies, and how Rowan University Library has taken advantage of these expanding opportunities since the beginning of the migration until and through the go-live date to account for these new integrations.
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Pisano, Jim, Rodrigo Amestica, and Jesus Perez. "ALMA correlator computer systems." In SPIE Astronomical Telescopes + Instrumentation. SPIE, 2004. http://dx.doi.org/10.1117/12.550066.

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Danassis, Panayiotis, Florian Wiedemair, and Boi Faltings. "Improving Multi-agent Coordination by Learning to Estimate Contention." In Thirtieth International Joint Conference on Artificial Intelligence {IJCAI-21}. California: International Joint Conferences on Artificial Intelligence Organization, 2021. http://dx.doi.org/10.24963/ijcai.2021/18.

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We present a multi-agent learning algorithm, ALMA-Learning, for efficient and fair allocations in large-scale systems. We circumvent the traditional pitfalls of multi-agent learning (e.g., the moving target problem, the curse of dimensionality, or the need for mutually consistent actions) by relying on the ALMA heuristic as a coordination mechanism for each stage game. ALMA-Learning is decentralized, observes only own action/reward pairs, requires no inter-agent communication, and achieves near-optimal (<5% loss) and fair coordination in a variety of synthetic scenarios and a real-world meeting scheduling problem. The lightweight nature and fast learning constitute ALMA-Learning ideal for on-device deployment.
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Haupt, Christoph, Richard Sramek, and Koh-Ichiro Morita. "System engineering in the ALMA project." In SPIE Astronomical Telescopes + Instrumentation, edited by Martin J. Cullum and George Z. Angeli. SPIE, 2006. http://dx.doi.org/10.1117/12.670350.

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Shillue, Bill, Wes Grammer, Christophe Jacques, Rodrigo Brito, Jack Meadows, Jason Castro, Yoshihiro Masui, Robert Treacy, and Jean-François Cliche. "The ALMA photonic local oscillator system." In SPIE Astronomical Telescopes + Instrumentation, edited by Wayne S. Holland. SPIE, 2012. http://dx.doi.org/10.1117/12.927174.

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Reyes, N., C. Jarufe, F. P. Mena, J. Pizarro, L. Bronfman, and J. May. "Amplification system of ALMA Band 1." In SPIE Astronomical Telescopes + Instrumentation, edited by Wayne S. Holland and Jonas Zmuidzinas. SPIE, 2010. http://dx.doi.org/10.1117/12.857396.

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Reports on the topic "AlMn System"

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KAMAN SCIENCES CORP COLORADO SPRINGS CO. Microcomputer Missile Performance Software System: ASSIGNMENT Computer Software Component, ALM Maintenance Manual (MM-04). Fort Belvoir, VA: Defense Technical Information Center, January 1990. http://dx.doi.org/10.21236/ada257660.

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Author, Not Given. The U.S. Advanced Liquid Metal Reactor Program (ALMR) Actinide Recycle System 1994 Capital and Busbar Cost Estimates. Office of Scientific and Technical Information (OSTI), March 1995. http://dx.doi.org/10.2172/1108730.

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African Open Science Platform Part 1: Landscape Study. Academy of Science of South Africa (ASSAf), 2019. http://dx.doi.org/10.17159/assaf.2019/0047.

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This report maps the African landscape of Open Science – with a focus on Open Data as a sub-set of Open Science. Data to inform the landscape study were collected through a variety of methods, including surveys, desk research, engagement with a community of practice, networking with stakeholders, participation in conferences, case study presentations, and workshops hosted. Although the majority of African countries (35 of 54) demonstrates commitment to science through its investment in research and development (R&D), academies of science, ministries of science and technology, policies, recognition of research, and participation in the Science Granting Councils Initiative (SGCI), the following countries demonstrate the highest commitment and political willingness to invest in science: Botswana, Ethiopia, Kenya, Senegal, South Africa, Tanzania, and Uganda. In addition to existing policies in Science, Technology and Innovation (STI), the following countries have made progress towards Open Data policies: Botswana, Kenya, Madagascar, Mauritius, South Africa and Uganda. Only two African countries (Kenya and South Africa) at this stage contribute 0.8% of its GDP (Gross Domestic Product) to R&D (Research and Development), which is the closest to the AU’s (African Union’s) suggested 1%. Countries such as Lesotho and Madagascar ranked as 0%, while the R&D expenditure for 24 African countries is unknown. In addition to this, science globally has become fully dependent on stable ICT (Information and Communication Technologies) infrastructure, which includes connectivity/bandwidth, high performance computing facilities and data services. This is especially applicable since countries globally are finding themselves in the midst of the 4th Industrial Revolution (4IR), which is not only “about” data, but which “is” data. According to an article1 by Alan Marcus (2015) (Senior Director, Head of Information Technology and Telecommunications Industries, World Economic Forum), “At its core, data represents a post-industrial opportunity. Its uses have unprecedented complexity, velocity and global reach. As digital communications become ubiquitous, data will rule in a world where nearly everyone and everything is connected in real time. That will require a highly reliable, secure and available infrastructure at its core, and innovation at the edge.” Every industry is affected as part of this revolution – also science. An important component of the digital transformation is “trust” – people must be able to trust that governments and all other industries (including the science sector), adequately handle and protect their data. This requires accountability on a global level, and digital industries must embrace the change and go for a higher standard of protection. “This will reassure consumers and citizens, benefitting the whole digital economy”, says Marcus. A stable and secure information and communication technologies (ICT) infrastructure – currently provided by the National Research and Education Networks (NRENs) – is key to advance collaboration in science. The AfricaConnect2 project (AfricaConnect (2012–2014) and AfricaConnect2 (2016–2018)) through establishing connectivity between National Research and Education Networks (NRENs), is planning to roll out AfricaConnect3 by the end of 2019. The concern however is that selected African governments (with the exception of a few countries such as South Africa, Mozambique, Ethiopia and others) have low awareness of the impact the Internet has today on all societal levels, how much ICT (and the 4th Industrial Revolution) have affected research, and the added value an NREN can bring to higher education and research in addressing the respective needs, which is far more complex than simply providing connectivity. Apart from more commitment and investment in R&D, African governments – to become and remain part of the 4th Industrial Revolution – have no option other than to acknowledge and commit to the role NRENs play in advancing science towards addressing the SDG (Sustainable Development Goals). For successful collaboration and direction, it is fundamental that policies within one country are aligned with one another. Alignment on continental level is crucial for the future Pan-African African Open Science Platform to be successful. Both the HIPSSA ((Harmonization of ICT Policies in Sub-Saharan Africa)3 project and WATRA (the West Africa Telecommunications Regulators Assembly)4, have made progress towards the regulation of the telecom sector, and in particular of bottlenecks which curb the development of competition among ISPs. A study under HIPSSA identified potential bottlenecks in access at an affordable price to the international capacity of submarine cables and suggested means and tools used by regulators to remedy them. Work on the recommended measures and making them operational continues in collaboration with WATRA. In addition to sufficient bandwidth and connectivity, high-performance computing facilities and services in support of data sharing are also required. The South African National Integrated Cyberinfrastructure System5 (NICIS) has made great progress in planning and setting up a cyberinfrastructure ecosystem in support of collaborative science and data sharing. The regional Southern African Development Community6 (SADC) Cyber-infrastructure Framework provides a valuable roadmap towards high-speed Internet, developing human capacity and skills in ICT technologies, high- performance computing and more. The following countries have been identified as having high-performance computing facilities, some as a result of the Square Kilometre Array7 (SKA) partnership: Botswana, Ghana, Kenya, Madagascar, Mozambique, Mauritius, Namibia, South Africa, Tunisia, and Zambia. More and more NRENs – especially the Level 6 NRENs 8 (Algeria, Egypt, Kenya, South Africa, and recently Zambia) – are exploring offering additional services; also in support of data sharing and transfer. The following NRENs already allow for running data-intensive applications and sharing of high-end computing assets, bio-modelling and computation on high-performance/ supercomputers: KENET (Kenya), TENET (South Africa), RENU (Uganda), ZAMREN (Zambia), EUN (Egypt) and ARN (Algeria). Fifteen higher education training institutions from eight African countries (Botswana, Benin, Kenya, Nigeria, Rwanda, South Africa, Sudan, and Tanzania) have been identified as offering formal courses on data science. In addition to formal degrees, a number of international short courses have been developed and free international online courses are also available as an option to build capacity and integrate as part of curricula. The small number of higher education or research intensive institutions offering data science is however insufficient, and there is a desperate need for more training in data science. The CODATA-RDA Schools of Research Data Science aim at addressing the continental need for foundational data skills across all disciplines, along with training conducted by The Carpentries 9 programme (specifically Data Carpentry 10 ). Thus far, CODATA-RDA schools in collaboration with AOSP, integrating content from Data Carpentry, were presented in Rwanda (in 2018), and during17-29 June 2019, in Ethiopia. Awareness regarding Open Science (including Open Data) is evident through the 12 Open Science-related Open Access/Open Data/Open Science declarations and agreements endorsed or signed by African governments; 200 Open Access journals from Africa registered on the Directory of Open Access Journals (DOAJ); 174 Open Access institutional research repositories registered on openDOAR (Directory of Open Access Repositories); 33 Open Access/Open Science policies registered on ROARMAP (Registry of Open Access Repository Mandates and Policies); 24 data repositories registered with the Registry of Data Repositories (re3data.org) (although the pilot project identified 66 research data repositories); and one data repository assigned the CoreTrustSeal. Although this is a start, far more needs to be done to align African data curation and research practices with global standards. Funding to conduct research remains a challenge. African researchers mostly fund their own research, and there are little incentives for them to make their research and accompanying data sets openly accessible. Funding and peer recognition, along with an enabling research environment conducive for research, are regarded as major incentives. The landscape report concludes with a number of concerns towards sharing research data openly, as well as challenges in terms of Open Data policy, ICT infrastructure supportive of data sharing, capacity building, lack of skills, and the need for incentives. Although great progress has been made in terms of Open Science and Open Data practices, more awareness needs to be created and further advocacy efforts are required for buy-in from African governments. A federated African Open Science Platform (AOSP) will not only encourage more collaboration among researchers in addressing the SDGs, but it will also benefit the many stakeholders identified as part of the pilot phase. The time is now, for governments in Africa, to acknowledge the important role of science in general, but specifically Open Science and Open Data, through developing and aligning the relevant policies, investing in an ICT infrastructure conducive for data sharing through committing funding to making NRENs financially sustainable, incentivising open research practices by scientists, and creating opportunities for more scientists and stakeholders across all disciplines to be trained in data management.
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