Ordizia, hiri hezitzailea

In this text we realize of the analysis and of the result of the project "Ordizia, hiri hezitzailea". This project has been developed in Ordizia (Gipuzkoa) between the years 2008 and 2012. At present, the experience continues with a very positive valuation.ln this article we have thought if the educational cities fulfill the function of revitalazing the educational capacities that the cities have innate. In addition to that, we have born in mind the benefits of the management of the networks partner educational taking into account that they promote a majar cooperative efficiency and we do ours many oj the principies of the educational community referring to the stari--up and to the development uf the educational cities 'project.The project has be en designed by people in charge of Ordizia 's local government and by a research group of the University of the Rasque Country and, in a beginning; it was planned from 2008 until 2011. The Plan continues working and it is actual/y infullforce. The schools, associations and departments of the tawn hall take part in it. In this project, we organized an agenda of activities for 2011 that was renewedfor the year 2012.25 associations and groups took part in it. Moreover, we prepared a catalogue with 34 initiatives for interinstitutional cooperation. One of the main conclusions of the project has been that the educational cooperation improves and optimizes the global relation of the municipality and, at the same time, the groups involved in these projects fortify and their efficiency increases.; Dans ce texte, nous réalisons l'analyse et les résultats du projet "Ordizia, Hiri hezitzailea". Ce projet a été développé en Ordizia (Gipuzkoa) entre 2()()8 et 2012. A l'heure actuelle, l'expérience se poursuit avec un bilan tres positif Tout d'abord, nous avons réjléchi a savoir si les villes éducatrices jouent le rOle de dynamisation des compétences éducatives qui ont les villes. En outre, nous avons vu les avantages de la gestion des réseaux socio-éducatifs qui envisagent de promouvoir une plus grande coopération de l'effiracité, el nousfaisons nOtres bon nombre des prindpes de la communauté éducative dans la mesure oii la mise en service et le développement de projets de villes éducatrices.Le projet a été conru par les responsables de la Ville de Ordízia et un groupe de recherche a l'Université du Pays Basque-EHU et, d'abord, nous avons travaíllé depuis 2008-2011. Le plan se poursuit aujourd'hui en place et est pleinement en vigueur. Les écoles, les associations et les services du conseil sont impliqués dans le projet maintenam.Dans ce projet, nous avons organisé un programme d'activités pour 2011 qui a été renouvelé pour l' année 2012 avec la participacion de 25 associations et groupes. En plus, nous avons préparé une liste de 34 initiatives de coopération. L'une des principales conclusions du projet a été que la coopération éducative améliore et optimise l' ensemble des relations de la municipalité et au mime temps, les groupes impliqués dans ces projets sont renforcées et leur efficacité augmente.; En este texto damos cuenta del análisis y del resultado del proyecto "Ordizia. hiri hezitzailea". Este proyecto se desarrolló en Ordizia (Gipuzkoa) entre los años 2008 y 2012. En la actualidad, la experiencia continúa con una valorarión muy positiva. En este artículo hemos reflexionado sobre las ciudades educadoras, si estas cumplen la función de dinamizadoras de las capacidades educativas innatas que tienen las ciudades. Además, hemos contemplado los beneficios de la gestión de las redes socio-educativas teniendo en cuenta que promueven una mayor eficacia cooperativa, y hacemos nuestros muchos de los principios de la comunidad educativa en lo que a la puesta en marcha y al desarrollo del proyecto de ciudades educadoras se refiere. El proyecto ha sido diseñado por responsables del Ayuntamiento de Ordizia y por un grupo de investigación de la Universidad del País Vasco/Euskal Herriko Unibertsitatea y, en un principio, se trabajó en él desde 2008 hasta 2011. El Plan continua en marcha y a día de hoy está en plena vigencia. Los colegios, asociaciones y departamentos del ayuntamiento participan en él actualmente. Dentro de ese proyecto, organizamos una agenda de actividades para 2011 que se renovó para el año 2012 participando 25 asociaciones y grupos. Además, preparamos un catálogo con 34 iniciativas para la cooperación interinstitucional. Una de las principales conclusiones del proyecto ha sido que la cooperación educativa mejora y optimiza la relación global del municipio y, al mismo tiempo, los grupos implicados en estos proyectos se fortalecen y su efectividad aumenta

MDE based IoT Service to enhance the safety of controllers at runtime

One of the challenges for complex IoT software systems is toincrease their safety. A Model Driven Development approach helps in the design and development phase of these systems while runtime checkin gtechniques help to enhance safety. To supervise the status of different IoT services that are registered in a local cloud at runtime, the solution that is presented in this work uses the information that it receives from the different services registered in a local cloud in model terms. The runtime checker, the new Safety related service of the Arrowhead framework, has predefined contracts to ensure the correctness of the services at runtime.Based on these contracts and checking the information that it receives at runtime it is able to detect unsafe scenarios. Once an unsafe scenario is detected, it starts a safe process to protect the behaviour of the whole system adapting the wrong service or services to a degraded operation mode at runtime. All these services will be Arrowhead compliant

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Cet article de recherche découle du projet Développement de compétencess pécifiques des professeurs et du personnel d'appui pour réussir dans l'intégration des élèves immigrés; ceprojet a commencé dans le cours 2008-2009, par rapport aux compétences que les professeurs d’enseignement enfantin et primaire doivent avoir pourtravailler avec des élèves immigrés. Ona proposé un questionnaire avec trente-cinq 35 items référés à: la conscience,l'attitude, la connaissance, l'adresseet les habilités. Le test a compté aussiavec des questions ouvertes par rapportaux niveaux de satisfaction, les expectatives de formation, la situation personnelle des personnes interrogées. Dans les conclusions on a observéle défaut de préparation des professeurs dans le travail avec des élèves immigrés, et aussi une prédispositionpar rapport à l'amélioration de leurpratique éducative. Transfert à la pratiqueCe travail de recherche a lieu en tant que conséquence de l'augmentation des élèves immigrés dans les centresd'enseignement du Pays Basquependant les dernières années, une situation qui a permis détecter certain escarences dans la formationdes professeurs qui ont travaillé avecce type d'élèves. Depuis la détectiondes carences on a élaboré un décaloguequi contribue à les diminuer, enmême temps, en collaboration avecles universités d'Aquitaine (France),on a organisé des cours de formation pour les professeurs et les éducateurs sociaux qui ont eu lieu à SanSebastian (Espagne) et Pau (France),avec l'objectif d'améliorer la pratiqued'enseignement des professeurs et dupersonnel qui travaille avec des élèves immigrés.Este artigo de pesquisa se deriva do projeto Desenvolvimento de competências específicas do professorado epessoal de apoio para conseguir a integraçãodo corpo discente imigrante, iniciado no curso 2008/09, sobre as competências que deve apresentar o professorado que trabalha com corpodiscente imigrante nas etapas de Ensino Infantil e Primária. Foi proposto um questionário com 35 itens referidos a:Consciência, Atitude, Conhecimento,Destreza e Habilidades. Também contoucom perguntas abertas sobre os níveis de satisfação, expectativas deformação, situação pessoal… dos entrevistados. Nas conclusões se observaa falta de preparação do professorado para trabalhar com corpo discente imigrante, bem como sua predisposição para a melhora de sua prática educativa. Transferência à práticaEste trabalho de pesquisa é consequênciado notável aumento do corpodiscente imigrante nos centros de ensino do País Vasco durante os últimos anos, uma situação que permitiu detectar determinadas carências naformação do professorado que trabalhacom este tipo de corpo discente.A partir da detecção de referidas lacunas se elabora um decálogo quecontribui para atenuar as mesmas e,em colaboração com as universidades de Aquitania (França), organizaram-secursos de formação para professorado e educadores/as sociais que se realizaramem San Sebastián (Espanha) e Pau(França), com o objetivo de melhorar a prática docente do professorado e dopessoal que trabalha com corpo discente imigrante.Este artículo de investigación se deriva del proyecto Desarrollo de competencias específicas del profesorado y personal de apoyo para lograr la integración del alumnado inmigrante, iniciado en el curso 2008/09, sobre las competencias que debe presentar el profesorado que trabaja con alumnado inmigrante en las etapas de enseñanza infantil y primaria. Se planteó un cuestionario con 35 ítems referidos a Consciencia, Actitud, Conocimiento y Destreza y Habilidades. También contó con preguntas abiertas sobre los niveles de satisfacción, expectativas de formación, situación personal… de los encuestados. En las conclusiones se observan la falta de preparación del profesorado paratrabajar con alumnado inmigrante y su predisposición para la mejora de su práctica educativa.Transferencia a la prácticaEste trabajo de investigación tiene lugar como consecuencia del notable aumento de alumnado inmigrante en los centros de enseñanza del País Vasco durante los últimos años,una situación que ha permitido detectar determinadas carencias en la formación del profesorado que ejercía coneste tipo de alumnado. Desde la detección de esas falencias se elabora un decálogo que contribuye a paliarlas, a la vez que, en colaboración con las universidades de Aquitania(Francia), se organizaron unos cursos de formación para profesorado y educadores/as sociales que se celebraron en San Sebastián (España) y Pau (Francia), con el objetivo demejorar la práctica docente del profesorado y del personal que trabaja con alumnado inmigrante.This research article resulting from the project Development of specific competences of teachers and support staff to achieve the integration of immigrant students, started in the academic year 2008/09, on the skills required from the teachers working with immigrant students in stages ofearly childhood in Primary Education. It raised a questionnaire with 35 items related to: Awareness, Attitude, Skills and Knowledge and Skills. Also featured open questions on satisfaction levels, training expectations, personal situation, of respondents. The conclusions noted the lack of preparation of teachers to work with immigrant students and their willingness to improve their educational practice.Transference to practiceThis research takes place as a result of the substantial increase of immigrant students in schools in the Basque Country in recent years, a situation that led to the identification of certain short comings in teacher education who exercised with this type of student. Since the detection of such a decalogue is made by relieving them, while, in collaboration with the Universitiesof Aquitaine (France), organizeda training for teachers and educators/ social as held in San Sebastian(Spain) and Pau (France), with the goal of improving teaching practice of teachers and staff who work with immigrant students

Préjugés des étudiants de l’enseignement secondaire sur l’immigration

We carried out a review of the best-known questionnaires and catalogues on prejudices regarding immigration that exist in society and we drew up a new questionnaire, with positive and negative scales of prejudices, in order to apply them to secondary school students in the Basque Country. We analysed the responses of almost 1,500 students and thus obtained results for the main prejudices existing amongst the students. Subsequently we examined these, the most consolidated, prejudices and compared them with scientific data, reports and other research, and which have generated debate about these prejudices. As a result of this research, we believe that we have made available to educators, inside and outside the classroom, the basis for drawing up strategies and plans for educational intervention with secondary school students.Hacemos una recopilación de los cuestionarios y los catálogos más conocidos sobre los prejuicios que existen en la sociedad en materia de inmigración y elaboramos un nuevo cuestionario, con escalas positivas y negativas de prejuicios, para aplicarlo al alumnado de secundaria del País Vasco. Analizamos las respuestas de casi 1.500 alumnos y obtenemos los principales prejuicios que existen entre este alumnado. Después examinamos esos prejuicios más consolidados y establecemos un contraste con datos científicos, informes, estudios, etc., que ponen en discusión la solidez de esos prejuicios. Como resultado de este trabajo, creemos que ponemos a disposición de los educadores, dentro y fuera del aula, las bases para elaborar estrategias y planes de intervención educativa con el alumnado de secundaria.Nous avons fait une collecte des questionnaires et des catalogues connus sur les préjugés qui existent dans la société en matière d’immigration. Nous avons aussi développé un nouveau questionnaire, avec des échelles positives et négatives des préjugés, pour demander à des élèves du secondaire dans le Pays Basque. Nous avons analysé les réponses de plus de 1.500 étudiants et nous avons réussi une liste des préjugés les plus puissants qui existent parmi ces étudiants. Après, nous avons analysé ces préjugés plus solides pour établir un contraste avec les données scientifiques, rapports, études, etc. qui remettent en question le bien-fondé de ces préjugés. À la suite de ce travail, nous croyons que nous fournissons des éducateurs dedans et hors du centre scolaire, la base pour l’élaboration de stratégies d’intervention et d’éducation avec les élèves du secondaire

Convective storms in closed cyclones in Jupiter's South Temperate Belt: (I) observations

On May 31, 2020 a short-lived convective storm appeared in one of the small cyclones of Jupiter's South Temperate Belt (STB) at planetographic latitude 30.8S. The outbreak was captured by amateur astronomer Clyde Foster in methane-band images, became widely known as Clyde's Spot, and was imaged at very high resolution by the Junocam instrument on board the Juno mission 2.5 days later. Junocam images showed a white two-lobed cyclonic system with high clouds observed in the methane-band at 890 nm. The storm evolved over a few days to become a dark feature that showed turbulence for months, presented oscillations in its drift rate, and slowly expanded, first into a Folded Filamentary Region (FFR), and later into a turbulent segment of the STB over a timescale of one year. On August 7, 2021, a new storm strikingly similar to Clyde's Spot erupted in a cyclone of the STB. The new storm exhibited first a similar transformation into a turbulent dark feature, and later transformed into a dark cyclone fully formed by January 2022. We compare the evolution into a FFR of Clyde's Spot with the formation of a FFR observed by Voyager 2 in 1979 in the South South Temperate Belt (SSTB) after a convective outburst in a cyclone that also developed a two-lobed shape. We also discuss the contemporaneous evolution of an additional cyclone of the STB, which was similar to the one were Clyde's Spot developed. This cyclone did not exhibit visible internal convective activity, and transformed from pale white in 2019, with low contrast with the environment, to dark red in 2020, and thus, was very similar to the outcome of the second storm. This cyclone became bright again in 2021 after interacting with Oval BA. We present observations of these phenomena obtained by amateur astronomers, ground-based telescopes, Hubble Space Telescope and Junocam. This study reveals that short-lived small storms that are active for only a few days can produce complex longterm changes that extend over much larger areas than those initially covered by the storms. In a second paper [In tilde urrigarro et al., 2022] we use the EPIC numerical model to simulate these storms and study moist convection in closed cyclones.We are very thankful to the large community of amateur observers operating small telescopes that submit their Jupiter observations to databases such as PVOL and ALPO-Japan. We are also grateful to two anonymous reviewers for their comments that improved the clarity of this paper. This work has been supported by Grant PID2019-109467GB-I00 funded by MCIN/AEI/10.13039/501100011033/and by Grupos Gobierno Vasco IT1366-19. PI acknowledges a PhD scholarship from Gobierno Vasco. GSO and TM were supported by NASA with funds distributed to the Jet Propulsion Laboratory, California Institute of Technology under contract 80NM0018D0004. C. J. Hansen was sup-ported by funds from NASA, USA to the Juno mission via the Planetary Science Institute. IOE was supported by a contract funded by Europlanet 2024 RI to navigate Junocam images, now available as maps in PVOL at http://pvol2.ehu.eus. Europlanet 2024 RI has received funding from the European Unions Horizon 2020 research and innovation programme under grant agreement No 871149. G.S. Orton, S. R. Brueshaber, T. W. Momary, K. H. Baines and E. K. Dahl were visiting Astronomers at the Infrared Telescope Facility, which is operated by the University of Hawaii under contract 80HQTR19D0030 with the National Aeronautics and Space Administration. In addition, support from NASA Juno Participating Scientist award 80NSSC19K1265 was provided to M.H. Wong. This work has used data acquired from the NASA/ESA Hubble Space Telescope (HST) , which is operated by the Association of 807 Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These HST observations are associated with several HST observing programs: GO/DD 14661 (PI: M.H. Wong) , GO/DD 15665 (PI: I. de Pater) , GO/DD 15159 (PI: M. H. Wong) , GO/DD 15502 (PI: A. Simon) , GO/DD 14661 (PI: M. H. Wong) , GO/DD 16074 (PI: M.H. Wong) , GO/DD 16053 (PI: I. de Pater) , GO/DD 15929 (PI: A. Simon) , GO/DD 16269 (PI: A. Simon) . PlanetCam observations were collected at the Centro Astronomico Hispanico en Andalucia (CAHA) , operated jointly by the Instituto de Astrofisica de Andalucia (CSIC) and the Andalusian Universities (Junta de Andalucia) . This work was enabled by the location of the IRTF and Gemini North telescopes within the Mauakea Science Reserve, adjacent to the summit of Maunakea. We are grateful for the privilege of observing Kaawela (Jupiter) from a place that is unique in both its astronomical quality and its cultural signifi-cance. This research has made use of the USGS Integrated Software for Imagers and Spectrometers (ISIS) . Voyager 2 images were accessed through The PDS Ring-Moon Systems Nodes OPUS search service

Constraints on the structure and seasonal variations of Triton's atmosphere from the 5 October 2017 stellar occultation and previous observations

Context. A stellar occultation by Neptune's main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of which yielded a central flash detection. Aims. We aimed at constraining Triton's atmospheric structure and the seasonal variations of its atmospheric pressure since the Voyager 2 epoch (1989). We also derived the shape of the lower atmosphere from central flash analysis. Methods. We used Abel inversions and direct ray-tracing code to provide the density, pressure, and temperature profiles in the altitude range similar to 8 km to similar to 190 km, corresponding to pressure levels from 9 mu bar down to a few nanobars. Results. (i) A pressure of 1.18 +/- 0.03 mu bar is found at a reference radius of 1400 km (47 km altitude). (ii) A new analysis of the Voyager 2 radio science occultation shows that this is consistent with an extrapolation of pressure down to the surface pressure obtained in 1989. (iii) A survey of occultations obtained between 1989 and 2017 suggests that an enhancement in surface pressure as reported during the 1990s might be real, but debatable, due to very few high S/N light curves and data accessible for reanalysis. The volatile transport model analysed supports a moderate increase in surface pressure, with a maximum value around 2005-2015 no higher than 23 mu bar. The pressures observed in 1995-1997 and 2017 appear mutually inconsistent with the volatile transport model presented here. (iv) The central flash structure does not show evidence of an atmospheric distortion. We find an upper limit of 0.0011 for the apparent oblateness of the atmosphere near the 8 km altitude.J.M.O. acknowledges financial support from the Portuguese Foundation for Science and Technology (FCT) and the European Social Fund (ESF) through the PhD grant SFRH/BD/131700/2017. The work leading to these results has received funding from the European Research Council under the European Community's H2020 2014-2021 ERC grant Agreement nffi 669416 "Lucky Star". We thank S. Para who supported some travels to observe the 5 October 2017 occultation. T.B. was supported for this research by an appointment to the National Aeronautics and Space Administration (NASA) Post-Doctoral Program at the Ames Research Center administered by Universities Space Research Association (USRA) through a contract with NASA. We acknowledge useful exchanges with Mark Gurwell on the ALMA CO observations. This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium).Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. J.L.O., P.S.-S., N.M. and R.D. acknowledge financial support from the State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award to the Instituto de Astrofisica de Andalucia (SEV-2017-0709), they also acknowledge the financial support by the Spanish grant AYA-2017-84637-R and the Proyecto de Excelencia de la Junta de Andalucia J.A. 2012-FQM1776. The research leading to these results has received funding from the European Union's Horizon 2020 Research and Innovation Programme, under Grant Agreement no. 687378, as part of the project "Small Bodies Near and Far" (SBNAF). P.S.-S. acknowledges financial support by the Spanish grant AYA-RTI2018-098657-J-I00 "LEO-SBNAF". The work was partially based on observations made at the Laboratorio Nacional de Astrofisica (LNA), Itajuba-MG, Brazil. The following authors acknowledge the respective CNPq grants: F.B.-R. 309578/2017-5; R.V.-M. 304544/2017-5, 401903/2016-8; J.I.B.C. 308150/2016-3 and 305917/2019-6; M.A. 427700/20183, 310683/2017-3, 473002/2013-2. This study was financed in part by the Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior -Brasil (CAPES) -Finance Code 001 and the National Institute of Science and Technology of the e-Universe project (INCT do e-Universo, CNPq grant 465376/2014-2). G.B.R. acknowledges CAPES-FAPERJ/PAPDRJ grant E26/203.173/2016 and CAPES-PRINT/UNESP grant 88887.571156/2020-00, M.A. FAPERJ grant E26/111.488/2013 and A.R.G.Jr. FAPESP grant 2018/11239-8. B.E.M. thanks CNPq 150612/2020-6 and CAPES/Cofecub-394/2016-05 grants. Part of the photometric data used in this study were collected in the frame of the photometric observations with the robotic and remotely controlled telescope at the University of Athens Observatory (UOAO; Gazeas 2016). The 2.3 m Aristarchos telescope is operated on Helmos Observatory by the Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing of the National Observatory of Athens. Observations with the 2.3 m Aristarchos telescope were carried out under OPTICON programme. This project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 730890. This material reflects only the authors views and the Commission is not liable for any use that may be made of the information contained therein. The 1. 2m Kryoneri telescope is operated by the Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing of the National Observatory of Athens. The Astronomical Observatory of the Autonomous Region of the Aosta Valley (OAVdA) is managed by the Fondazione Clement Fillietroz-ONLUS, which is supported by the Regional Government of the Aosta Valley, the Town Municipality of Nus and the "Unite des Communes valdotaines Mont-Emilius". The 0.81 m Main Telescope at the OAVdA was upgraded thanks to a Shoemaker NEO Grant 2013 from The Planetary Society. D.C. and J.M.C. acknowledge funds from a 2017 'Research and Education' grant from Fondazione CRT-Cassa di Risparmio di Torino. P.M. acknowledges support from the Portuguese Fundacao para a Ciencia e a Tecnologia ref. PTDC/FISAST/29942/2017 through national funds and by FEDER through COMPETE 2020 (ref. POCI010145 FEDER007672). F.J. acknowledges Jean Luc Plouvier for his help. S.J.F. and C.A. would like to thank the UCL student support observers: Helen Dai, Elise Darragh-Ford, Ross Dobson, Max Hipperson, Edward Kerr-Dineen, Isaac Langley, Emese Meder, Roman Gerasimov, Javier Sanjuan, and Manasvee Saraf. We are grateful to the CAHA, OSN and La Hita Observatory staffs. This research is partially based on observations collected at Centro Astronomico HispanoAleman (CAHA) at Calar Alto, operated jointly by Junta de Andalucia and Consejo Superior de Investigaciones Cientificas (IAA-CSIC). This research was also partially based on observation carried out at the Observatorio de Sierra Nevada (OSN) operated by Instituto de Astrofisica de Andalucia (CSIC). This article is also based on observations made with the Liverpool Telescope operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council. Partially based on observations made with the Tx40 and Excalibur telescopes at the Observatorio Astrofisico de Javalambre in Teruel, a Spanish Infraestructura Cientifico-Tecnica Singular (ICTS) owned, managed and operated by the Centro de Estudios de Fisica del Cosmos de Aragon (CEFCA). Tx40 and Excalibur are funded with the Fondos de Inversiones de Teruel (FITE). A.R.R. would like to thank Gustavo Roman for the mechanical adaptation of the camera to the telescope to allow for the observation to be recorded. R.H., J.F.R., S.P.H. and A.S.L. have been supported by the Spanish projects AYA2015-65041P and PID2019-109467GB-100 (MINECO/FEDER, UE) and Grupos Gobierno Vasco IT1366-19. Our great thanks to Omar Hila and their collaborators in Atlas Golf Marrakech Observatory for providing access to the T60cm telescope. TRAPPIST is a project funded by the Belgian Fonds (National) de la Recherche Scientifique (F.R.S.-FNRS) under grant PDR T.0120.21. TRAPPIST-North is a project funded by the University of Liege, and performed in collaboration with Cadi Ayyad University of Marrakesh. E.J. is a FNRS Senior Research Associate