Let's talk about data: Citation and publication

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This document discusses citation and publication of data from various marine research organizations. It provides links to sites hosting Irish marine data and research on data infrastructure. It addresses issues like making data openly accessible, ensuring catalogue entries are citable, and having organizational policies for persistent storage. The document asks for questions and lists upcoming workshops to further discuss working with marine research data.

Science

Let’s talk about data:
Citation & publication
Adam Leadbetter
Information Services & Development, OSIS

http://www.alanhull.com/september-2014
http://mispint:8080/teamareas/mi_data_planning/
http://data.marine.ie
http://erddap.marine.ie

https://www.elsevier.com/connect/building-a-global-infrastructure-for-research-data

http://blog.thomsonreuters.com/index.php/thomson-reuters-technologists-partnered-with-global-organizations-on-new-research-tool

• Openly accessible landing pages
• Specific fields in the catalogue entries
• Catalogue entries themselves are not citable
• Organisational policy on persistence of data
• Who do we have authority to issue DOIs for?

“Well managed high quality Irish marine data
from the Marine Institute and partner organisations
will underpin the sustainable development
of Ireland’s marine resource”

Any Questions?
Dates for your diary:
8th December – Data workshop
16th December – Next seminar – your input needed

1. The document discusses various strategies for marketing an institutional repository (IR), including using social media, registering the IR in relevant directories and harvesters, and participating in events like Open Access Week. 2. It provides details on registering an open access policy with ROARMap and ensuring the IR is OAI-PMH compliant and harvestable by listing the OAI base URL and examples. 3. The presentation recommends marketing the IR through various directories, indexes, and aggregators like OpenDOAR, ROAR, Ranking Web of Repositories, re3data.org, DuraSpace, BASE, CORE, Open Access Map, Repository 66, OAIster, and the UIUC O

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Academy of Science of South Africa (ASSAf)

This document outlines the criteria for trusted institutional repositories in Africa to be included in the DATAD-R registry. It discusses what constitutes a trusted institutional repository, outlines various auditing and certification systems used internationally, and emphasizes the importance of metadata compatibility. The DATAD-R criteria cover aspects like contact details, technical infrastructure, policies, and governance. Inclusion in DATAD-R involves a self-review using their criteria, an independent peer-review, and reapplying every 3 years to maintain inclusion. Harmonizing with standards helps ensure African repositories are interoperable and their data reliably preserved.

DATAD-R African Open Science Platform (AOSP)

Academy of Science of South Africa

The document summarizes the African Open Science Platform (AOSP), which aims to coordinate open science activities across Africa. It discusses open science principles and the rationale for an African platform to increase collaboration, data reuse, and accelerate discovery. The AOSP is funded by the NRF of South Africa and managed by ASSAf. It focuses on establishing an open data forum, funding research infrastructure and projects, developing open data policies and training, and creating incentives for data sharing. Initial actions include workshops on policy, capacity building, and surveys to inform the platform's development.

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This document provides information about contributing bibliographic data to AGRIS, a database containing over 7 million references related to agricultural research. It outlines the benefits of publishing data in AGRIS such as becoming part of a global network and increased access and visibility without giving up content rights. The steps for joining AGRIS include checking topic coverage, metadata formats, and vocabulary requirements. Methods for acquiring and providing metadata like AgriMetaMaker, Mendeley, AgriDrupal and AgriOcean DSpace are described. Common mistakes to avoid and a registration process are also detailed.

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From the ORCID Outreach Meeting, May 21-22, 2014, Chicago, Illinois, USA, https://orcid.org/content/orcid-outreach-meeting-and-codefest-may-2014 ORCID identifiers in access management Universities and other research organizations have begun utilizing the ORCID identifier to manage access to repositories and research information systems. This session will feature a discussion of integration opportunities, policy and privacy issues, and demonstrations by research organizations. Moderator: Ed Pentz, Executive Director, CrossRef Presenters: Keith Hazelton, Senior IT Architect the University of Wisconsin-Madison/Chair of Internet2 MACE-Dir working group Jared Lyle, Director of Curation Services, Inter-university Consortium for Political and Social Research (ICPSR), University of Michigan Ken Okaya, Product Manager, Rightsholder Services, Copyright Clearance Center / slides Doug Hahn, Senior Information Technology Manager, Texas A&M University Elaine Westbrooks, Associate University Librarian for Research, University of Michigan

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AGRIS is an international system started in 1975 by FAO to provide access to agricultural research and technology information. It includes (1) a collection of over 8 million bibliographic records contributed by over 150 partner institutions in 65 countries, (2) an RDF database with 250 million triples, and (3) a multilingual web portal for searching records. Users can search by keyword, filter results, and access over 1.3 million records with links to full text. Partner institutions can submit new records through an online submission workflow.

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The document introduces the TRUST principles for digital repositories. The TRUST principles consist of 5 components: Transparency, Responsibility, User community, Sustainability, and Technology. The principles are meant to provide a framework for evaluating trustworthiness and establishing guidelines for repositories to manage and provide long-term access to research data in a transparent, reliable manner focused on serving user communities. A white paper on the TRUST principles provides further details on the motivations and definitions of each component.

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This document discusses using ORCID identifiers to track research data management and sharing. It covers linking ORCID profiles to institutional and third-party data repositories like Zenodo, Dataverse, and Figshare using services like DataCite. Populating ORCID records through DataCite's auto-update feature allows researchers to identify datasets stored in external repositories via their ORCID profile.

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Kate Wittenberg discusses Portico's current work and future plans. Portico has signed 320 publisher participants representing over 2,000 societies. Efforts are being made to preserve links between publications and underlying data through projects like RMap. Portico also partners with national libraries like the BL and KB to leverage their infrastructure for legal deposit programs. Looking ahead, Portico aims to broaden preservation efforts to more content types and collaborate more with other organizations.

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ORCID, Inc

This document discusses CONVERIS, a research information system created by AVEDAS to manage the entire research lifecycle. CONVERIS allows universities and research organizations to increase visibility of research activities, improve management information through features like CVs and publication tracking, and streamline administrative processes. It integrates information from across the organization in a single system. The document highlights AVEDAS' interest in ORCID integration to uniquely identify researchers and better connect data between systems.

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ORCID, Inc

The document discusses the Wellcome Trust's current and future use of ORCID identifiers in researcher workflows from a funder's perspective. It outlines that the Trust currently mandates ORCID on all grant applications. Future plans include pulling publication and dataset information from ORCID profiles and pushing grant information back to ORCID to better link researchers to their work. This is intended to simplify processes and create more accurate researcher records.

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Connecting Research and Researchers: How ORCID is Facilitating the Interoperable Exchange of Information, presented at the annual meeting of the Society for Scholarly Publishing, 30 May 2014. ABSTRACT: The publishing community has been an early and enthusiastic adopter of the work of ORCID, an independent non-profit organization with a twofold mission: to provide an open registry of unique identifiers for researchers, and to work with the scholarly community to ensure that this persistent identifier is embedded in research workflows. ORCID serves as a hub, linking existing identifiers, such as CrossRef and DataCite DOIs, ISNI organizational identifiers, and author identifiers including ResearcherId and ScopusAuthor ID with the ultimate goal of connecting researchers with their contributions. This session will provide an opportunity to learn about the status of ORCID integration into manuscript submission and production systems, into reviewer workflows, into conference systems, and into repositories and evaluation systems. A panel of experts from diverse publishing will provide practical examples and best practices for how the scholarly communications community is using ORCID. Moderator: Rebecca Bryant, ORCID Speakers Martin Fenner, PLOS Cesar Berrios-Otero, F1000 Research Michael Habib, Elsevier B.V. Brooks Hanson, American Geophysical Union Rebecca Bryant, ORCID

Enabling information interoperability with identifiers (L. Haak)

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1) ORCID provides persistent digital identifiers that uniquely identify researchers and enable information interoperability by connecting researchers to their work like publications and grants. 2) Over 2 million researchers have registered for an ORCID identifier which are associated with over 5 million publications and 40 thousand organizations. 3) Major publishers, funders, and universities are using ORCID to simplify researcher workflows by allowing information to be entered once and then reused, reducing duplicate effort and improving reporting and attribution of work.

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This document summarizes differences between 20th century and 21st century data processing approaches. In the 20th century, single machines were used for one-to-one communication with fixed schemas and encodings, while the 21st century utilizes distributed processing with publish-subscribe patterns, replication for fault tolerance, and schema management with evolvable encodings. It also lists further work such as investigating architectures for reprocessing historic data, incorporating standards like Sensor Web Enablement and OM-JSON, deploying to mobile/remote platforms, and investigating Apache NiFi.

Ocean Data Interoperability Platform - Big Data

Adam Leadbetter

Where did my layer come from? The semantics of data release

Adam Leadbetter

Vocabulary Services in EMODNet and SeaDataNet

Adam Leadbetter

Oceans of Linked Data

Adam Leadbetter

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United by a Common Language

The Place of Schema.org in Linked Ocean Data

Using Erddap as a building block in Ireland's Integrated Digital Ocean

Where Linked Data meets Big Data: Applying standard data models to environmen...

Managing data for marine sciences

Linked Ocean Data - Exploring connections between marine datasets in a Big Da...

Connected Ocean Data

Linking Open Data in Ireland's Digital Ocean

Ocean Data Interoperability Platform - Vocabularies: DOIs for NVS Controlled ...

Ocean Data Interoperability Platform - Big Data: Velocity

Research Vessel Data Management

Practical solutions to implementing "Born Connected" data systems

Linked Ocean Data

Irish Integrated Digital Ocean

Ocean Data Interoperability Platform - Big Data - Streams & Workflows

Ocean Data Interoperability Platform - Big Data

Where did my layer come from? The semantics of data release

Vocabulary Services in EMODNet and SeaDataNet

Oceans of Linked Data

Recently uploaded

GBSN - Biochemistry (Unit 6) Chemistry of Proteins

Areesha Ahmad

Compexometric titration/Chelatorphy titration/chelating titration

Vandana Devesh Sharma

Classification Metal ion ion indicators Masking and demasking reagents Estimation of Magnisium sulphate Calcium gluconate Complexometric Titration/ chelatometry titration/chelating titration, introduction, Types- 1.Direct Titration 2.Back Titration 3.Replacement Titration 4.Indirect Titration Masking agent, Demasking agents formation of complex comparition between masking and demasking agents, Indicators/Metal ion indicators/ Metallochromic indicators/pM indicators, Visual Technique,PM indicators (metallochromic), Indicators of pH, Redox Indicators Instrumental Techniques-Photometry Potentiometry Miscellaneous methods. Complex titration with EDTA.

CLASS 12th CHEMISTRY SOLID STATE ppt (Animated)

eitps1506

Description: Dive into the fascinating realm of solid-state physics with our meticulously crafted online PowerPoint presentation. This immersive educational resource offers a comprehensive exploration of the fundamental concepts, theories, and applications within the realm of solid-state physics. From crystalline structures to semiconductor devices, this presentation delves into the intricate principles governing the behavior of solids, providing clear explanations and illustrative examples to enhance understanding. Whether you're a student delving into the subject for the first time or a seasoned researcher seeking to deepen your knowledge, our presentation offers valuable insights and in-depth analyses to cater to various levels of expertise. Key topics covered include: Crystal Structures: Unravel the mysteries of crystalline arrangements and their significance in determining material properties. Band Theory: Explore the electronic band structure of solids and understand how it influences their conductive properties. Semiconductor Physics: Delve into the behavior of semiconductors, including doping, carrier transport, and device applications. Magnetic Properties: Investigate the magnetic behavior of solids, including ferromagnetism, antiferromagnetism, and ferrimagnetism. Optical Properties: Examine the interaction of light with solids, including absorption, reflection, and transmission phenomena. With visually engaging slides, informative content, and interactive elements, our online PowerPoint presentation serves as a valuable resource for students, educators, and enthusiasts alike, facilitating a deeper understanding of the captivating world of solid-state physics. Explore the intricacies of solid-state materials and unlock the secrets behind their remarkable properties with our comprehensive presentation.

The debris of the ‘last major merger’ is dynamically young

Sérgio Sacani

The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the ‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space, because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago. We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data 1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’ did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within the last few Gyr, consistent with the body of work surrounding the VRM.

Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...

Sérgio Sacani

Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation

MICROBIAL INTERACTION PPT/ MICROBIAL INTERACTION AND THEIR TYPES // PLANT MIC...

ABHISHEK SONI NIMT INSTITUTE OF MEDICAL AND PARAMEDCIAL SCIENCES , GOVT PG COLLEGE NOIDA

Microbial interaction Microorganisms interacts with each other and can be physically associated with another organisms in a variety of ways. One organism can be located on the surface of another organism as an ectobiont or located within another organism as endobiont. Microbial interaction may be positive such as mutualism, proto-cooperation, commensalism or may be negative such as parasitism, predation or competition Types of microbial interaction Positive interaction: mutualism, proto-cooperation, commensalism Negative interaction: Ammensalism (antagonism), parasitism, predation, competition I. Mutualism: It is defined as the relationship in which each organism in interaction gets benefits from association. It is an obligatory relationship in which mutualist and host are metabolically dependent on each other. Mutualistic relationship is very specific where one member of association cannot be replaced by another species. Mutualism require close physical contact between interacting organisms. Relationship of mutualism allows organisms to exist in habitat that could not occupied by either species alone. Mutualistic relationship between organisms allows them to act as a single organism. Examples of mutualism: i. Lichens: Lichens are excellent example of mutualism. They are the association of specific fungi and certain genus of algae. In lichen, fungal partner is called mycobiont and algal partner is called II. Syntrophism: It is an association in which the growth of one organism either depends on or improved by the substrate provided by another organism. In syntrophism both organism in association gets benefits. Compound A Utilized by population 1 Compound B Utilized by population 2 Compound C utilized by both Population 1+2 Products In this theoretical example of syntrophism, population 1 is able to utilize and metabolize compound A, forming compound B but cannot metabolize beyond compound B without co-operation of population 2. Population 2is unable to utilize compound A but it can metabolize compound B forming compound C. Then both population 1 and 2 are able to carry out metabolic reaction which leads to formation of end product that neither population could produce alone. Examples of syntrophism: i. Methanogenic ecosystem in sludge digester Methane produced by methanogenic bacteria depends upon interspecies hydrogen transfer by other fermentative bacteria. Anaerobic fermentative bacteria generate CO2 and H2 utilizing carbohydrates which is then utilized by methanogenic bacteria (Methanobacter) to produce methane. ii. Lactobacillus arobinosus and Enterococcus faecalis: In the minimal media, Lactobacillus arobinosus and Enterococcus faecalis are able to grow together but not alone. The synergistic relationship between E. faecalis and L. arobinosus occurs in which E. faecalis require folic acid

Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...

Travis Hills MN

Authoring a personal GPT for your research and practice: How we created the Q...

Leonel Morgado

Thematic analysis in qualitative research is a time-consuming and systematic task, typically done using teams. Team members must ground their activities on common understandings of the major concepts underlying the thematic analysis, and define criteria for its development. However, conceptual misunderstandings, equivocations, and lack of adherence to criteria are challenges to the quality and speed of this process. Given the distributed and uncertain nature of this process, we wondered if the tasks in thematic analysis could be supported by readily available artificial intelligence chatbots. Our early efforts point to potential benefits: not just saving time in the coding process but better adherence to criteria and grounding, by increasing triangulation between humans and artificial intelligence. This tutorial will provide a description and demonstration of the process we followed, as two academic researchers, to develop a custom ChatGPT to assist with qualitative coding in the thematic data analysis process of immersive learning accounts in a survey of the academic literature: QUAL-E Immersive Learning Thematic Analysis Helper. In the hands-on time, participants will try out QUAL-E and develop their ideas for their own qualitative coding ChatGPT. Participants that have the paid ChatGPT Plus subscription can create a draft of their assistants. The organizers will provide course materials and slide deck that participants will be able to utilize to continue development of their custom GPT. The paid subscription to ChatGPT Plus is not required to participate in this workshop, just for trying out personal GPTs during it.

(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...

Scintica Instrumentation

JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDS

Sérgio Sacani

The pathway(s) to seeding the massive black holes (MBHs) that exist at the heart of galaxies in the present and distant Universe remains an unsolved problem. Here we categorise, describe and quantitatively discuss the formation pathways of both light and heavy seeds. We emphasise that the most recent computational models suggest that rather than a bimodal-like mass spectrum between light and heavy seeds with light at one end and heavy at the other that instead a continuum exists. Light seeds being more ubiquitous and the heavier seeds becoming less and less abundant due the rarer environmental conditions required for their formation. We therefore examine the different mechanisms that give rise to different seed mass spectrums. We show how and why the mechanisms that produce the heaviest seeds are also among the rarest events in the Universe and are hence extremely unlikely to be the seeds for the vast majority of the MBH population. We quantify, within the limits of the current large uncertainties in the seeding processes, the expected number densities of the seed mass spectrum. We argue that light seeds must be at least 103 to 105 times more numerous than heavy seeds to explain the MBH population as a whole. Based on our current understanding of the seed population this makes heavy seeds (Mseed > 103 M⊙) a significantly more likely pathway given that heavy seeds have an abundance pattern than is close to and likely in excess of 10−4 compared to light seeds. Finally, we examine the current state-of-the-art in numerical calculations and recent observations and plot a path forward for near-future advances in both domains.

HOW DO ORGANISMS REPRODUCE?reproduction part 1

Shashank Shekhar Pandey

EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...

Sérgio Sacani

Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions among stars. Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars. The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun. Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically, the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec. Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation were carried out using the ACIS-Extract software. Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a photon flux threshold of approximately 2 × 10−8 photons cm−2 s −1 . The X-ray sources exhibit a highly concentrated spatial distribution, with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.

AJAY KUMAR NIET GreNo Guava Project File.pdf

AJAY KUMAR

Mending Clothing to Support Sustainable Fashion_CIMaR 2024.pdf

Selcen Ozturkcan

8.Isolation of pure cultures and preservation of cultures.pdf

by6843629

cathode ray oscilloscope and its applications

sandertein

23PH301 - Optics - Optical Lenses.pptx

RDhivya6

Direct Seeded Rice - Climate Smart Agriculture

International Food Policy Research Institute- South Asia Office

在线办理(salfor毕业证书)索尔福德大学毕业证毕业完成信一模一样

vluwdy49

学校原件一模一样【微信：741003700 】《(salfor毕业证书)索尔福德大学毕业证》【微信：741003700 】学位证，留信认证（真实可查，永久存档）原件一模一样纸张工艺/offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。本公司拥有海外各大学样板无数，能完美还原。 1:1完美还原海外各大学毕业材料上的工艺：水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠。文字图案浮雕、激光镭射、紫外荧光、温感、复印防伪等防伪工艺。材料咨询办理、认证咨询办理请加学历顾问Q/微741003700 【主营项目】一.毕业证【q微741003700】成绩单、使馆认证、教育部认证、雅思托福成绩单、学生卡等！二.真实使馆公证(即留学回国人员证明,不成功不收费) 三.真实教育部学历学位认证（教育部存档！教育部留服网站永久可查）四.办理各国各大学文凭(一对一专业服务,可全程监控跟踪进度) 如果您处于以下几种情况： ◇在校期间，因各种原因未能顺利毕业……拿不到官方毕业证【q/微741003700】 ◇面对父母的压力，希望尽快拿到； ◇不清楚认证流程以及材料该如何准备； ◇回国时间很长，忘记办理； ◇回国马上就要找工作，办给用人单位看； ◇企事业单位必须要求办理的 ◇需要报考公务员、购买免税车、落转户口 ◇申请留学生创业基金留信网认证的作用: 1:该专业认证可证明留学生真实身份 2:同时对留学生所学专业登记给予评定 3:国家专业人才认证中心颁发入库证书 4:这个认证书并且可以归档倒地方 5:凡事获得留信网入网的信息将会逐步更新到个人身份内，将在公安局网内查询个人身份证信息后，同步读取人才网入库信息 6:个人职称评审加20分 7:个人信誉贷款加10分 8:在国家人才网主办的国家网络招聘大会中纳入资料，供国家高端企业选择人才

Describing and Interpreting an Immersive Learning Case with the Immersion Cub...

Leonel Morgado

Current descriptions of immersive learning cases are often difficult or impossible to compare. This is due to a myriad of different options on what details to include, which aspects are relevant, and on the descriptive approaches employed. Also, these aspects often combine very specific details with more general guidelines or indicate intents and rationales without clarifying their implementation. In this paper we provide a method to describe immersive learning cases that is structured to enable comparisons, yet flexible enough to allow researchers and practitioners to decide which aspects to include. This method leverages a taxonomy that classifies educational aspects at three levels (uses, practices, and strategies) and then utilizes two frameworks, the Immersive Learning Brain and the Immersion Cube, to enable a structured description and interpretation of immersive learning cases. The method is then demonstrated on a published immersive learning case on training for wind turbine maintenance using virtual reality. Applying the method results in a structured artifact, the Immersive Learning Case Sheet, that tags the case with its proximal uses, practices, and strategies, and refines the free text case description to ensure that matching details are included. This contribution is thus a case description method in support of future comparative research of immersive learning cases. We then discuss how the resulting description and interpretation can be leveraged to change immersion learning cases, by enriching them (considering low-effort changes or additions) or innovating (exploring more challenging avenues of transformation). The method holds significant promise to support better-grounded research in immersive learning.

Recently uploaded (20)

GBSN - Biochemistry (Unit 6) Chemistry of Proteins

Compexometric titration/Chelatorphy titration/chelating titration

CLASS 12th CHEMISTRY SOLID STATE ppt (Animated)

The debris of the ‘last major merger’ is dynamically young

Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...

MICROBIAL INTERACTION PPT/ MICROBIAL INTERACTION AND THEIR TYPES // PLANT MIC...

Travis Hills of MN is Making Clean Water Accessible to All Through High Flux ...

Authoring a personal GPT for your research and practice: How we created the Q...

(June 12, 2024) Webinar: Development of PET theranostics targeting the molecu...

JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDS

HOW DO ORGANISMS REPRODUCE?reproduction part 1

EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...

AJAY KUMAR NIET GreNo Guava Project File.pdf

Mending Clothing to Support Sustainable Fashion_CIMaR 2024.pdf

8.Isolation of pure cultures and preservation of cultures.pdf

cathode ray oscilloscope and its applications

23PH301 - Optics - Optical Lenses.pptx

Direct Seeded Rice - Climate Smart Agriculture

在线办理(salfor毕业证书)索尔福德大学毕业证毕业完成信一模一样

Describing and Interpreting an Immersive Learning Case with the Immersion Cub...