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German physics gaudi speakers platform

This later crystallized into a working group that developed the mission of FAC in spring when the curators convened in Berkeley, facilitated by a grant from the Warhol Foundation for the Visual Arts. Alongside the steering committee, all FAC participants are encouraged to self-organize working groups around issues they consider urgent, and each project is organized by the originating institution. This grassroots initiative strives to maintain a nonhierarchical working model that questions and seeks to overcome colonial and patriarchal narratives within institutional spaces. The exhibition features women artists of various cultures who are broadly from the West, and whose creative possibilities use the theme of feminism in its most expansive meaning. Works are far-reaching from a diasporic experience, the politics of body, resilience, self-determination, and land.


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WATCH RELATED VIDEO: German Physiks Unlimited Ultimate HIFI Speakers REVIEW #highend

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Boarding time is PM with departure at 7 PM. Shuttle buses will depart from Kimmel Center at PM. Buses will provide a return trip to various points in Manhattan within walking distance of conference hotels. Photo ID is required for boarding. Boarding cards will be distributed to participants at boarding time at Chelsea Piers. Choose Timezone. Specify a timezone. Monday, May Plenary Skirball Center Skirball Center. Convener : Michael Ernst Unknown.

Welcome to CHEP 5m. Speaker : Michael Ernst Unknown. Video in CDS. Welcome to NYU 10m. LHC experience so far, prospects for the future 30m.

Speaker : Prof. HEP Computing 30m. Lunch break 1h 30m. Over the years, Socrates and other great teachers developed the methodology of this practice.

Yet, as small groups of friends morphed into large classrooms of students, readers of journals, and audiences of television viewers, science conversation evolved into lecturing and broadcasting. The birth of Web 2. I discuss both the danger and the powerful potential of this phenomenon, and present methods currently used in HEP to make the best of it. Code and papers: computing publication patterns in the LHC era 25m. Publications in scholarly journals establish the body of knowledge deriving from scientific research; they also play a fundamental role in the career path of scientists and in the evaluation criteria of funding agencies.

This presentation reviews the evolution of computing-oriented publications in HEP following the start of operation of LHC. Several scientometric indicators are analyzed to characterize the role of computing in HEP literature.

Distinctive features of scholarly publication production in the software-oriented and hardware-oriented experimental HEP communities are highlighted. The results of this scientometric analysis document objectively the contribution of computing to HEP scientific production and technology transfer to other fields.

They also provide elements for discussion about how to more effectively promote the role played by computing-oriented research in high energy physics. Since , the development of Indico has focused on usability, performance and new features, especially the ones related to meeting collaboration. Usability studies have resulted in the biggest change Indico has experienced up to now, a new web layout that makes the user experience better. Performance improvements were also a key goal since ; the main features of Indico have been optimized remarkably.

Along with usability and performance, new features have been added to Indico such as webchat integration, video services bookings, webcast and recording requests, designed to really reinforce Indico position as the main hub for all CERN collaboration services, and many others which aim is to complete the conference lifecycle management. Indico development is also moving towards a broader collaboration where other institutes, hosting their own Indico instance, can contribute to the project in order make it a better and more complete tool.

In this talk, we will explain how CERN digital library services have evolved to deal with the publication of the first results of the LHC.

We will describe the work-flow of the documents on CERN Document Server and the diverse constraints relative to this work-flow. We will also give an overview on how the underlying software, Invenio, has been enriched to cope with special needs.

In a second part, the impact in terms of user access to the publication of the experiments and to the multimedia material will be detailed. The age and size of the CMS collaboration at the LHC means it now has many hundreds of inhomogeneous web sites and services and more than , documents.

We describe a major initiative to create a single coherent CMS internal and public web site. We describe the information architecture; the system design, implementation and monitoring; the document and content database; security aspects; and our deployment strategy which ensured continual smooth operation of all systems at all times. Physicists are using LHC to recreate the conditions just after the Big Bang, by colliding two beams of particles and heavy ions head-on at very high energy.

The project is expected to generate 27 TB of raw data per day, plus 10 TB of "event summary data". Network monitoring on such complex network architecture to ensure robust and reliable operation is of crucial importance. It contains a set of services delivering performance measurements in a multi-domain environment.

These services act as an intermediate layer, between the performance measurement tools and the visualization applications. This layer is aimed at exchanging performance measurements between networks, using well defined protocols. The proposed presentation will introduce the main points of the LHCOPN structure, provide an introduction about perfSONAR framework software, architecture, service structure and finally describe the way the whole monitoring infrastructure is monitored and how the support is organised.

The much-heralded exhaustion of the IPv4 networking address space has finally started. While many of the research and education networks have been ready and poised for years to carry IPv6 traffic, there is a well-known lack of academic institutes using the new protocols. One reason for this is an obvious absence of pressure due to the extensive use of NAT or that most currently still have sufficient IPv4 addresses. More importantly though, the fact is that moving your distributed applications to IPv6 involves much more than the routing, naming and addressing solutions provided by your campus and national networks.

Application communities need to perform a full analysis of their applications, middleware and tools to confirm how much development work is required to use IPv6 and to plan a smooth transition. The activities include the analysis and testing of the readiness for IPv6 and performance of many different components, including the applications, middleware, management and monitoring tools essential for HEP computing.

A distributed IPv6 testbed has been deployed and used for this purpose and we have been working closely with the HEP experiment collaborations. The working group is also considering other operational issues such as the implications for security arising from a move to IPv6. This paper describes the work done by the HEPiX IPv6 working group since its inception and presents our current conclusions and recommendations.

Status and trends in networking at LHC Tier1 facilities 25m. The LHC is entering its fourth year of production operation. Many Tier1 facilities can count up to a decade of existence when development and ramp-up efforts are included. LHC computing has always been heavily dependent on high capacity, high performance network facilities for both the LAN and WAN data movement, particularly within the Tier1 centers.

As a result, the Tier1 centers tend to be on the leading edge of data center networking technology. In this paper, we conduct an analysis of past and current developments in Tier1 networking, as well as extrapolating where we anticipate things are heading.

Overview of storage operations at CERN 25m. CASTOR also evolved during this time with major improvements in critical areas - notably the internal scheduling of requests, the simplifications of the database structure and a complete overhaul of the tape subsystem.

The talk will compare the two systems from an operation's perspective setup, day-by-day user support, upgrades, resilience to common failures while taking into account their different scope. In the case of CASTOR we will analyse the impact of the improvements on delivering Tier0 services, while for EOS we will focus on the steps to achieve to a production-quality service. For both systems, the upcoming changes will be discussed in relation with the evolution of the LHC programme and computing models data volumes, access patterns, relations among computing sites.

CMS experiment possesses distributed computing infrastructure and its performance heavily depends on the fast and smooth distribution of data between different CMS sites.

At the same time, processed data has to be distributed from Tier-1 sites to all Tier-2 sites for physics analysis while MonteCarlo simulations synchronized back to Tier-1 sites for further archival. It is very important to ensure reliable operation of the system, and the operational tasks comprise monitoring and debugging all transfer issues. Based on transfer quality information Site Readiness tool is used to create plans for resources utilization in the future.

We review the operational procedures created to enforce reliable data delivery to CMS distributed sites all over the world. Additionally, we need to keep data consistent at all sites and both on disk and on tape. It provides all the components that are needed to manage the distributed resources. AliEn is used for all the computing workflows of the experiment: Montecarlo production, data replication and reconstruction and organixed or chaotic user analysis.

The main components of AliEn are a centralized file and metadata catalogue, a job execution model and file replication model. These three components have been evolving over the last 10 years to make sure that the satisfy the computing requirements of the experiment, which keep increasing every year.

The DQ2 system has over time rapidly evolved to assist the ATLAS collaboration management to properly manage the data, as well as provide an effective interface allowing physicists easy access to this data. Numerous new requirements and operational experience of ATLAS' use cases have necessitated the need for a next generation data management system, called Rucio, which will re-engineer the current system to cover new high-level use cases and workflows such as the management of data for physics groups.

In this talk, we will describe the state of the current of DQ2, and present an overview of the upcoming Rucio system, covering it's architecture, new innovative features, and preliminary benchmarks. The CMS workload management system 25m. CMS has started the process of rolling out a new workload management system. This system is currently used for reprocessing and monte carlo production with tests under way using it for user analysis.

This system now includes central request submission and management Request Manager ; a task queue for parcelling up and distributing work WorkQueue and agents which process requests by interfacing with disparate batch and storage resources WMAgent.

Datasets are defined as sets of files corresponding to a given query in the Bookkeeping system. Datasets can be manipulated by CLI tools as well as by automatic transformations removal, replication, processing.

A dynamic handling of dataset replication is performed, based on disk space usage at the sites and dataset popularity. For custodial storage, an on-demand recall of files from tape is performed, driven by the requests of the jobs, including disk cache handling. We shall describe all the tools that are available for Data Management, from handling of large datasets to basic tools for users as well as for monitoring the dynamic behaviour of LHCb Storage capacity.

Such solutions allow us not only to optimize development manpower but also offer lower long-term maintenance and support costs. This talk focuses primarily on the strategic aspects of providing such common solutions and how this relates to the overall goals of long-term sustainability and the relationship to the various WLCG Technical Evolution Groups.

ALICE moves into warp drive. Since its successful start-up in , the LHC has been performing outstandingly, providing to the experiments long periods of stable collisions and an integrated luminosity that greatly exceeds the planned targets. To fully explore these privileged conditions, we aim at maximizing the experiment's data taking productivity during stable collisions.

We present in this paper the evolution of the online systems in order to spot reasons of inefficiency and address new requirements. This paper describes the features added to the ALICE Electronic Logbook eLogbook to allow the Run Coordination team to identify, prioritize, fix and follow causes of inefficiency in the experiment.

Thorough monitoring of the data taking efficiency provides reports for the collaboration to portray its evolution and evaluate the measures fixes and new features taken to increase it. In particular, the eLogbook helps decision making by providing quantitative input, which can be used to better balance risks of changes in the production environment against potential gains in quantity and quality of physics data.


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The special R label denotes that additional resources e. Skip to main content. Search: Search. School of Physics and Astronomy. Contact us. Note that individual archives are also available for each of our event or seminar categories: General interest seminar archive Higgs Centre Colloquia archive Particle Physics Theory seminar archive UK Centre for Astrobiology seminar archive Condensed Matter lunchtime seminar archive Condensed Matter journal club archive Statistical Physics and Complexity Group meeting archive Entrepreneurship event archive General event archive The special R label denotes that additional resources e.

By searching the web, I came accross these speakers: a) Marten Coltrane Supreme b) German Physiks "The Gaudi".

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Architect: Antoni Gaudi. A postcard from my first academic conference, ACL Saif M. He received his Ph. His team developed a sentiment analysis system which ranked first in shared task competitions. His word--emotion resources, such as the NRC Emotion Lexicon , are used for analyzing affect in text. You can watch a video of the talk at the Alan Turing Institute London, March summarizing recent work. Detailed CV How my name is pronounced: Photo. Oct

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german physics gaudi speakers platform

Gable, Clark — American film star. His casual and debonair charm, edged sometimes with a cynical aplomb, made him a box-office star. Gabo, Naum Neemia originally Pevsner — Russian-American sculptor, born in Bryansk.

The German Physiks line is comprehensive, stretching from the comparatively humble Troubadour and Unlimited models, right up to the wardrobe-sized, cost no object Gaudi Mk II, but all share a common driver unique to the brand.

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Although physically smaller than the Gaudi, the Emperor is still a big loudspeaker, with all the advantages that brings. Its massive bass system produces well-controlled and clean bass all the way down to 18Hz, but is agile enough to integrate perfectly with the speed of the DDD drivers. The coherence of the DDD drivers allows the Emperor to generate very detailed and life like stereo images. This is fitted to a telescopic arm, which is driven by linear actuators, allowing it to be precisely positioned in relation to the bass enclosures for optimal phasing. The user can adjust each side from their seat using a wireless remote control.

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Contemporary automotive market demand has led to a wealth of new applications requiring strong performance in cost-effective optical systems. Requirements for these systems require modern software capability for both optical design and engineering Optical based biomedical systems can span a wide range of applications from wearables, pulse oximeters, absorption spectroscopy, fluorescence microscopy, and many, many others. These systems use light sources of varying types and wavelength ranges, including UV, visible, and infrared. Optical des. As the leading provider of materials reference data Key to Metals AG will present the key aspects of how the Total Materia database can support and improve the accuracy of simulation results whilst reducing cost, optimizing material usage and elim The Georgia Tech Institute of Technology Georgia Tech took the lead in collaborating with five Universities to develop a senior-level capstone design course that would give engineering students collaborative design experience using state-of the AAM has been providing mechanical drivelines to automotive customers for more than 25 years.

German Physiks Emperor Preamplifier review. exploit the exceptional dynamic range of the German Physiks Gaudi and Loreley loudspeakers.

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Boarding time is PM with departure at 7 PM. Shuttle buses will depart from Kimmel Center at PM. Buses will provide a return trip to various points in Manhattan within walking distance of conference hotels. Photo ID is required for boarding.

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During the conference, there will be held the Round table "Modern IT technologies and education". Boarding starts at Departure at From the pier on the Komsomolskaya embankment. All events within the conference will be held in compliance with the sanitary and epidemiological requirements to prevent the spread of the coronavirus infection COVID Conference languages - Russian and English. The "Fawkes" procedure is discussed as a method of protection against unauthorized use and recognition of facial images from social networks.

During that period, he founded Eurolab European Federation of Measurement, Testing and Analytical Laboratories and served as its first President from to He began his career in metrology, notably with the USA's National Bureau of Standards today the National Institute of Standards and Technology and has a strong background in the fields of quality and the rational use of energy.

German Physiks The Emperor MK II Referencia omnidirekcionális ultra high-end hangsugárzó

Hello, i am a newbie in the audiophile society and i would like to ask a question that bothers me for the last few weeks. By searching the web, I came accross these speakers: a Marten Coltrane Supreme b German Physiks "The Gaudi" The first ones, have two towers per channel, one for the bass and another one separately for the midrange and tweeters. So they need two 2 monoblock power-amplifiers per channel, one for each tower. The second ones, they need three 3 monoblock power amplifiers per channel, one for each section DDD, Woofer, Subwoofer. So, my question is how on earth they should be configured in order to create a stereo system?

Author : Edward D. Pages : pages. Publisher : Stanford University Press.




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