ELIXIR
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This presentation was given as part of the EOSC Stakeholders Forum Scientific Community Workshop which gives the opportunity to prospective consumers and providers - from both the public and commercial sectors - to discuss needs and opportunities that should drive the definition of the EOSC service portfolio roadmap. This workshop aims to answer the following: - What prospective needs and priorities do scientific communities have as consumers of the EOSC? - How should EOSC facilitate the sharing of data, scientific outputs and services across national and organisational borders? The workshop starts with a presentation of today’s state of play in federating resources and services to enable multi-disciplinary science and transnational access; it featured invited talks from representatives of digital infrastructures, research projects and communities and the long-tail of science. The workshop also involved representatives from both public and commercial organisations in their role as a service provider and service consumer. The workshop participants also took the opportunity to define a list of recommendations giving direction to the development and provisioning of the EOSC portfolio.
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The document discusses ELIXIR, the European infrastructure for biological information. ELIXIR aims to build a sustainable infrastructure to support life science research and its translation to various sectors. It coordinates existing bioinformatics services across Europe. The Italian node of ELIXIR (ELIXIR-ITA) coordinates domestic bioinformatics resources and connects them to the broader ELIXIR network. It works to aggregate and integrate Italy's small but excellent bioinformatics community and supports the large amount of data being generated through high-throughput sequencing platforms in Italy.
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This document provides an overview of the European Life Sciences Infrastructure for Biological Information (ELIXIR). ELIXIR aims to build a sustainable infrastructure for biological data by coordinating existing life science resources across Europe. It will provide services for data, tools, computing, standards, and training. ELIXIR is establishing pilot projects to test integration of these services and address challenges like data access and scale. A Technical Coordination Group leads implementation and coordinates task forces to develop each area of the infrastructure. ELIXIR also partners with e-infrastructures to utilize high-performance computing and networking resources. Its goal is to support life science research and translation to areas like medicine, the environment, and bioindustry.
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ELIXIR
ELIXIR is a European research infrastructure for biological information that aims to support life science research. It brings together major bioinformatics providers and is supported by 17 EU member states. ELIXIR works to safeguard biological data and build sustainable data services. It establishes a distributed infrastructure to handle the large growth of data and provides tools, services, and platforms to facilitate access and analysis of data. ELIXIR also develops standards and provides training to support computational biology. Key activities include establishing national nodes, technical task forces, and pilot projects in areas like cloud resources, data transfer, and linking distributed databases.
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ELIXIR
ELIXIR is a European research infrastructure for biological information that aims to facilitate life sciences research across Europe. It brings together life science resources from member countries to build a robust infrastructure for biological data. Individual organizations or countries cannot achieve this alone. ELIXIR establishes national nodes that leverage local strengths and priorities to deliver shared services through a distributed network. This allows the infrastructure to scale effectively with increasing data challenges. ELIXIR also works to improve data integration and interoperability across distributed resources through activities like developing standards and linking related communities.
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The document discusses ELIXIR, the European infrastructure for biological information. ELIXIR aims to build a sustainable infrastructure to support life science research and its translation to various sectors. It coordinates existing bioinformatics services across Europe. The Italian node of ELIXIR (ELIXIR-ITA) coordinates domestic bioinformatics resources and connects them to the broader ELIXIR network. It works to aggregate and integrate Italy's small but excellent bioinformatics community and supports the large amount of data being generated through high-throughput sequencing platforms in Italy.
ELIXIR
This document provides an overview of the European Life Sciences Infrastructure for Biological Information (ELIXIR). ELIXIR aims to build a sustainable infrastructure for biological data by coordinating existing life science resources across Europe. It will provide services for data, tools, computing, standards, and training. ELIXIR is establishing pilot projects to test integration of these services and address challenges like data access and scale. A Technical Coordination Group leads implementation and coordinates task forces to develop each area of the infrastructure. ELIXIR also partners with e-infrastructures to utilize high-performance computing and networking resources. Its goal is to support life science research and translation to areas like medicine, the environment, and bioindustry.
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ELIXIR is a European research infrastructure for biological information that aims to support life science research. It brings together major bioinformatics providers and is supported by 17 EU member states. ELIXIR works to safeguard biological data and build sustainable data services. It establishes a distributed infrastructure to handle the large growth of data and provides tools, services, and platforms to facilitate access and analysis of data. ELIXIR also develops standards and provides training to support computational biology. Key activities include establishing national nodes, technical task forces, and pilot projects in areas like cloud resources, data transfer, and linking distributed databases.
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The workshop starts with a presentation of today’s state of play in federating resources and services to enable multi-disciplinary science and transnational access; it featured invited talks from representatives of digital infrastructures, research projects and communities and the long-tail of science. The workshop also involved representatives from both public and commercial organisations in their role as a service provider and service consumer. The workshop participants also took the opportunity to define a list of recommendations giving direction to the development and provisioning of the EOSC portfolio.
EOSC Stakeholders Forum: Interoperability Session and Panel Discussion
The EOSC faces as well technical, social and economic challenges on interoperability. These have to be overcome in order to provide an efficient EOSC architecture. Some solutions are in place in some domains, but these have to be expanded to the cross-disciplinary and/or international level. We will summarize what the results of our studies within the EOSCpilot on interoperability and FAIR data sharing are. Then we will discuss openly solutions, opportunities and showstoppers with respect to an interoperable and FAIR EOSC with key experts in the field.
EOSC Stakeholders Forum: For a FAIR Europe-What's Needed, What's Existing
The EOSC faces as well technical, social and economic challenges on interoperability. These have to be overcome in order to provide an efficient EOSC architecture. Some solutions are in place in some domains, but these have to be expanded to the cross-disciplinary and/or international level. In this presentation, we discuss FAIR data sharing and current developments.
EOSC Stakeholders Forum: Enabling Interoperability-Experience from EOSCpilot
The EOSC faces as well technical, social and economic challenges on interoperability. These have to be overcome in order to provide an efficient EOSC architecture. Some solutions are in place in some domains, but these have to be expanded to the cross-disciplinary and/or international level. In this presentation, we summarise what the results of our studies within the EOSCpilot on interoperability
Science Demonstrator Session: Physics and Astrophysics
The main focus of Science Demonstrator sessions is to provide feedback to the EOSC community on the first experience of science demonstrators in the practical use of the emerging EOSC ecosystem.
Each panel will consist of a representative of a Science Demonstrator that will provide an overview of their experiences in the use of emerging EOSC services.
These sessions will help members of the scientific communities understanding the current state of maturity of the EOSC ecosystem and what is obtainable in a field of scientific research. It is also valuable to prospective Service Providers who wish to discover what are the challenges and opportunities that user communities might have to deal with, as a result of the adoption of their services.
This session will focus on Physics and Astrophysics.
Science Demonstrator Session: Social and Earth Sciences
The main focus of Science Demonstrator sessions is to provide feedback to the EOSC community on the first experience of science demonstrators in the practical use of the emerging EOSC ecosystem.
Each panel will consist of a representative of a Science Demonstrator that will provide an overview of their experiences in the use of emerging EOSC services.
These sessions will help members of the scientific communities understanding the current state of maturity of the EOSC ecosystem and what is obtainable in a field of scientific research. It is also valuable to prospective Service Providers who wish to discover what are the challenges and opportunities that user communities might have to deal with, as a result of the adoption of their services.
This session will focus on Social and Earth Sciences.
Science Demonstrator Session: Life and Materials Sciences
The main focus of Science Demonstrator sessions is to provide feedback to the EOSC community on the first experience of science demonstrators in the practical use of the emerging EOSC ecosystem.
Each panel will consist of a representative of a Science Demonstrator that will provide an overview of their experiences in the use of emerging EOSC services.
These sessions will help members of the scientific communities understanding the current state of maturity of the EOSC ecosystem and what is obtainable in a field of scientific research. It is also valuable to prospective Service Providers who wish to discover what are the challenges and opportunities that user communities might have to deal with, as a result of the adoption of their services.
This session will focus on life science and materials science.
EOSC Architecture Session - EOSC Stakeholders Forum 2018
The EOSC initiative aims at setting up a complex an articulated “system” consisting of interconnected and interoperating IT systems, policies, procedures, people and activities. The ultimate goal of such a system is to realise an Open Science-oriented working environment where offerings and demand for Open Science enacting commodities (computing and storage, services, data, software, and more in general any research artefacts ) meet. The success of the entire initiative largely depends on the capacity to meet Open Science practitioners demand (namely researchers) and on its “attractiveness” for practitioners willing to play the role of commodity “provider” & “(re)seller”. Resellers will be willing to bring their commodities into the EOSC marketplace if and only if they “see” a business opportunity, if and only if the benefits they may get are higher than the costs they have to sustain. The goal of this session is to identify the set of services EOSC should put in place to “temp” a larger number of “resellers” to contribute to the development of the EOSC marketplace.
Building a European policy framework
This presentation was held at the 1st EOSC Stakeholder Forum 28-29/11/2017 in Brussels.
For more information on the 1st EOSC Stakeholder Forum visit: https://eoscpilot.eu/eosc-stakeholder-forum-shaping-future-eosc
Follow EOSCpilot on Twitter: https://twitter.com/eoscpilot
and LinkedIn: https://uk.linkedin.com/in/eoscpiloteu
EOSC Architecture: a System of Systems
This presentation was held at the 1st EOSC Stakeholder Forum 28-29/11/2017 in Brussels.
For more information on the 1st EOSC Stakeholder Forum visit: https://eoscpilot.eu/eosc-stakeholder-forum-shaping-future-eosc
Follow EOSCpilot on Twitter: https://twitter.com/eoscpilot
and LinkedIn: https://uk.linkedin.com/in/eoscpiloteu
More from EOSCpilot .eu (20)
EOSC FAIR Data Session - EOSC Stakeholders Forum 2018
EOSC FAIR Data Session - EOSC Stakeholders Forum 2018
Results from the FAIR Expert Group Stakeholder Consultation on the FAIR Data ...
Results from the FAIR Expert Group Stakeholder Consultation on the FAIR Data ...
EOSC Governance Session - EOSC Stakeholders Forum 2018
EOSC Governance Session - EOSC Stakeholders Forum 2018
EOSC Policy Session - EOSC Stakeholders Forum 2018
EOSC Policy Session - EOSC Stakeholders Forum 2018
EMBL-Sustainable Access to the World's Largest Biomolecular Data Resources
EMBL-Sustainable Access to the World's Largest Biomolecular Data Resources
Earth Science Needs and Opportunities to Define the EOSC Service Roadmap
Earth Science Needs and Opportunities to Define the EOSC Service Roadmap
EOSC Stakeholders Forum: Interoperability Session and Panel Discussion
EOSC Stakeholders Forum: Interoperability Session and Panel Discussion
EOSC Stakeholders Forum: For a FAIR Europe-What's Needed, What's Existing
EOSC Stakeholders Forum: For a FAIR Europe-What's Needed, What's Existing
EOSC Stakeholders Forum: Enabling Interoperability-Experience from EOSCpilot
EOSC Stakeholders Forum: Enabling Interoperability-Experience from EOSCpilot
Science Demonstrator Session: Physics and Astrophysics
Science Demonstrator Session: Physics and Astrophysics
Science Demonstrator Session: Social and Earth Sciences
Science Demonstrator Session: Social and Earth Sciences
Science Demonstrator Session: Life and Materials Sciences
Science Demonstrator Session: Life and Materials Sciences
EOSC Architecture Session - EOSC Stakeholders Forum 2018
EOSC Architecture Session - EOSC Stakeholders Forum 2018
Recently uploaded
Anti-Universe And Emergent Gravity and the Dark Universe
Recent theoretical progress indicates that spacetime and gravity emerge together from the entanglement structure of an underlying microscopic theory. These ideas are best understood in Anti-de Sitter space, where they rely on the area law for entanglement entropy. The extension to de Sitter space requires taking into account the entropy and temperature associated with the cosmological horizon. Using insights from string theory, black hole physics and quantum information theory we argue that the positive dark energy leads to a thermal volume law contribution to the entropy that overtakes the area law precisely at the cosmological horizon. Due to the competition between area and volume law entanglement the microscopic de Sitter states do not thermalise at sub-Hubble scales: they exhibit memory effects in the form of an entropy displacement caused by matter. The emergent laws of gravity contain an additional ‘dark’ gravitational force describing the ‘elastic’ response due to the entropy displacement. We derive an estimate of the strength of this extra force in terms of the baryonic mass, Newton’s constant and the Hubble acceleration scale a0 = cH0, and provide evidence for the fact that this additional ‘dark gravity force’ explains the observed phenomena in galaxies and clusters currently attributed to dark matter.
一比一原版美国佩斯大学毕业证如何办理
原版一模一样【微信：741003700 】【美国佩斯大学毕业证成绩单】【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
办理美国佩斯大学毕业证【微信：741003700 】外观非常简单，由纸质材料制成，上面印有校徽、校名、毕业生姓名、专业等信息。
办理美国佩斯大学毕业证【微信：741003700 】格式相对统一，各专业都有相应的模板。通常包括以下部分：
校徽：象征着学校的荣誉和传承。
校名:学校英文全称
授予学位：本部分将注明获得的具体学位名称。
毕业生姓名：这是最重要的信息之一，标志着该证书是由特定人员获得的。
颁发日期：这是毕业正式生效的时间，也代表着毕业生学业的结束。
其他信息：根据不同的专业和学位，可能会有一些特定的信息或章节。
办理美国佩斯大学毕业证【微信：741003700 】价值很高，需要妥善保管。一般来说，应放置在安全、干燥、防潮的地方，避免长时间暴露在阳光下。如需使用，最好使用复印件而不是原件，以免丢失。
综上所述，办理美国佩斯大学毕业证【微信：741003700 】是证明身份和学历的高价值文件。外观简单庄重，格式统一，包括重要的个人信息和发布日期。对持有人来说，妥善保管是非常重要的。
BIRDS DIVERSITY OF SOOTEA BISWANATH ASSAM.ppt.pptx
Ahota Beel, nestled in Sootea Biswanath Assam , is celebrated for its extraordinary diversity of bird species. This wetland sanctuary supports a myriad of avian residents and migrants alike. Visitors can admire the elegant flights of migratory species such as the Northern Pintail and Eurasian Wigeon, alongside resident birds including the Asian Openbill and Pheasant-tailed Jacana. With its tranquil scenery and varied habitats, Ahota Beel offers a perfect haven for birdwatchers to appreciate and study the vibrant birdlife that thrives in this natural refuge.
Discovery of Merging Twin Quasars at z=6.05
We report the discovery of two quasars at a redshift of z = 6.05 in the process of merging. They were
serendipitously discovered from the deep multiband imaging data collected by the Hyper Suprime-Cam (HSC)
Subaru Strategic Program survey. The quasars, HSC J121503.42−014858.7 (C1) and HSC J121503.55−014859.3
(C2), both have luminous (>1043 erg s−1
) Lyα emission with a clear broad component (full width at half
maximum >1000 km s−1
). The rest-frame ultraviolet (UV) absolute magnitudes are M1450 = − 23.106 ± 0.017
(C1) and −22.662 ± 0.024 (C2). Our crude estimates of the black hole masses provide log 8.1 0. ( ) M M BH = 3
in both sources. The two quasars are separated by 12 kpc in projected proper distance, bridged by a structure in the
rest-UV light suggesting that they are undergoing a merger. This pair is one of the most distant merging quasars
reported to date, providing crucial insight into galaxy and black hole build-up in the hierarchical structure
formation scenario. A companion paper will present the gas and dust properties captured by Atacama Large
Millimeter/submillimeter Array observations, which provide additional evidence for and detailed measurements of
the merger, and also demonstrate that the two sources are not gravitationally lensed images of a single quasar.
Unified Astronomy Thesaurus concepts: Double quasars (406); Quasars (1319); Reionization (1383); High-redshift
galaxies (734); Active galactic nuclei (16); Galaxy mergers (608); Supermassive black holes (1663)
Methods of grain storage Structures in India.pdf
•Post-harvestlossesaccountforabout10%oftotalfoodgrainsduetounscientificstorage,insects,rodents,micro-organismsetc.,
•Totalfoodgrainproductioninindiais311milliontonnesandstorageis145mt.InIndia,annualstoragelosseshavebeenestimated14mtworthofRs.7,000croreinwhichinsectsaloneaccountfornearlyRs.1,300crores.
•InIndiaoutofthetotalproduction,about30%ismarketablesurplus
•Remaining70%isretainedandstoredbyfarmersforconsumption,seed,feed.Hence,growerneedstoragefacilitytoholdaportionofproducetosellwhenthemarketingpriceisfavourable
•TradersandCo-operativesatmarketcentresneedstoragestructurestoholdgrainswhenthetransportfacilityisinadequate
Holsinger, Bruce W. - Music, body and desire in medieval culture [2001].pdf
Music and Medieval History
Rodents, Birds and locust_Pests of crops.pdf
Mole rat or Lesser bandicoot rat, Bandicotabengalensis
•Head -round and broad muzzle
•Tail -shorter than head, body
•Prefers damp areas
•Burrows with scooped soil before entrance
•Potential rat, one pair can produce more than 800 offspringsin one year
Signatures of wave erosion in Titan’s coasts
The shorelines of Titan’s hydrocarbon seas trace flooded erosional landforms such as river valleys; however, it isunclear whether coastal erosion has subsequently altered these shorelines. Spacecraft observations and theo-retical models suggest that wind may cause waves to form on Titan’s seas, potentially driving coastal erosion,but the observational evidence of waves is indirect, and the processes affecting shoreline evolution on Titanremain unknown. No widely accepted framework exists for using shoreline morphology to quantitatively dis-cern coastal erosion mechanisms, even on Earth, where the dominant mechanisms are known. We combinelandscape evolution models with measurements of shoreline shape on Earth to characterize how differentcoastal erosion mechanisms affect shoreline morphology. Applying this framework to Titan, we find that theshorelines of Titan’s seas are most consistent with flooded landscapes that subsequently have been eroded bywaves, rather than a uniform erosional process or no coastal erosion, particularly if wave growth saturates atfetch lengths of tens of kilometers.
Reaching the age of Adolescence- Class 8
This is a presentation on understanding the age of adolescence.
Quality assurance B.pharm 6th semester BP606T UNIT 5
Warehousing
Good warehousing practices
Material management
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
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
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JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDS
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.
Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...
A proprietary approach developed by bringing together the best of learning theories from Psychology, design principles from the world of visualization, and pedagogical methods from over a decade of training experience, that enables you to: Learn better, faster!
The Limited Role of the Streaming Instability during Moon and Exomoon Formation
It is generally accepted that the Moon accreted from the disk formed by an impact between the proto-Earth and
impactor, but its details are highly debated. Some models suggest that a Mars-sized impactor formed a silicate
melt-rich (vapor-poor) disk around Earth, whereas other models suggest that a highly energetic impact produced a
silicate vapor-rich disk. Such a vapor-rich disk, however, may not be suitable for the Moon formation, because
moonlets, building blocks of the Moon, of 100 m–100 km in radius may experience strong gas drag and fall onto
Earth on a short timescale, failing to grow further. This problem may be avoided if large moonlets (?100 km)
form very quickly by streaming instability, which is a process to concentrate particles enough to cause gravitational
collapse and rapid formation of planetesimals or moonlets. Here, we investigate the effect of the streaming
instability in the Moon-forming disk for the first time and find that this instability can quickly form ∼100 km-sized
moonlets. However, these moonlets are not large enough to avoid strong drag, and they still fall onto Earth quickly.
This suggests that the vapor-rich disks may not form the large Moon, and therefore the models that produce vaporpoor disks are supported. This result is applicable to general impact-induced moon-forming disks, supporting the
previous suggestion that small planets (<1.6 R⊕) are good candidates to host large moons because their impactinduced disks would likely be vapor-poor. We find a limited role of streaming instability in satellite formation in an
impact-induced disk, whereas it plays a key role during planet formation.
Unified Astronomy Thesaurus concepts: Earth-moon system (436)
Mites,Slug,Snail_Infesting agricultural crops.pdf
Order : Trombidiformes (Acarina) Class : Arachnida
Mites normally feed on the undersurface of the leaves but the symptoms are more easily seen on the uppersurface.
Tetranychids produce blotching (Spots) on the leaf-surface.
Tarsonemids and Eriophyids produce distortion (twist), puckering (Folds) or stunting (Short) of leaves.
Eriophyids produce distinct galls or blisters (fluid-filled sac in the outer layer)
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
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Anti-Universe And Emergent Gravity and the Dark Universe
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Holsinger, Bruce W. - Music, body and desire in medieval culture [2001].pdf
Holsinger, Bruce W. - Music, body and desire in medieval culture [2001].pdf
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Quality assurance B.pharm 6th semester BP606T UNIT 5
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Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...
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Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...
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The Limited Role of the Streaming Instability during Moon and Exomoon Formation
The Limited Role of the Streaming Instability during Moon and Exomoon Formation
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...
ELIXIR
- 1. ELIXIR’s mission is to operate a sustainable European infrastructure for biological information, supporting life-science research and its translation to society, the bio- industries, environment and medicine ELIXIR’s strategy is to connect national bioinformatics centres and EMBL-EBI into a distributed infrastructure build from coordinated national and international data resources, tools and services
- 2. What are the ELIXIR services? ELIXIR Platforms bring coordinate services provided by our nodes Beacons/Local EGA – Federated Genomics Discovery & Query services ELIXIR / Life Science AAI ELIXIRCommunities bring together Node experts and users around standards and ELIXIR services Plant Community: Standards and services for federated plant phenotyping data
- 3. ELIXIR in 2023: ‘Well-connected and collaborating Nodes allow users to access and extract knowledge from large and distributed life science data sets’