Entwicklung eines Konzeptes für die Optimierung von Produktentwicklungsprojekten auf Basis eines integrierten Produktdaten- und Projektmanagements

Eine Analyse der gegenwärtigen EDV-Unterstützung der Produktentwicklung zeigt, dass dieser Prozess im Wesentlichen durch Produktdatenmanagement (PDM) und Projektmanagement (PM) assistiert werden. Aufgrund von unterschiedlichen Datenmodellen, redundanter Datenhaltung und des Fehlens einer zentralen Arbeitsoberfläche können diese Systeme den Anforderungen an eine wettbewerbsfähige Produktentwicklung lediglich partiell gerecht werden. Obwohl zu beiden Systemtypen zahlreiche Anwendungen existieren, fehlt bislang ein konsistentes Gesamtkonzept, welches die beiden Systemtypen zu einer durchgängigen EDV-Lösung vereinigt. In dieser Dissertation wird ein neuartiges Konzept für eine ganzheitliche EDV-Unterstützung von Produktentwicklungsprojekten erarbeitet. Der dargelegte Lösungsansatz besteht aus einer neu entwickelten Projektmanagementkomponente und der Erweiterung eines kommerziellen PDM-Systems. Die Beschreibung des Konzeptes wird in zwei Teilschritten vollzogen. Einleitend wird die Projektmanagementkomponente vorgestellt. Diese ist im Gegensatz zu herkömmlichen PM-Systemen auf die Anforderungen von Produktentwicklungsprojekten ausgelegt. Weiterhin werden bei ihrer Entwicklung Benutzerfreundlichkeit und Anpassungsfähigkeit als zentrale Randbedingungen berücksichtigt. In einem zweiten Schritt erfolgt die Integration der Projektmanagementkomponente in ein exemplarisches PDM-System. Dieses bildet die funktionale Basis für den erarbeiteten Lösungsansatz. Das PDM-System wird zu diesem Zweck über seine Programmierschnittstellen an die Anforderungen einer durchgängigen EDV-Unterstützung angepasst. Dabei bleibt durch die Systemarchitektur des entwickelten Lösungskonzeptes gewährleistet, dass die PM-Komponente unter geringem Anpassungsaufwand mit einem beliebigen PDM-System kombiniert werden kann. Abschließend werden anhand einer prototypenhaften Implementierung die Realisierbarkeit und der Nutzen des dargelegten Konzeptes nachgewiesen

Phase-locked multi-terahertz electric fields exceed 13 MV/cm at 190 kHz repetition rate

We demonstrate a compact source of energetic and phase-locked multi-terahertz pulses at a repetition rate of 190 kHz. Difference frequency mixing of the fundamental output of an Yb:KGW amplifier with the idler of an optical parametric amplifier in GaSe and LiGaS2 crystals yields a passively phase-locked train of waveforms tunable between 12 and 42 THz. The shortest multi-terahertz pulses contain 1.8 oscillation cycles within the intensity full width at half-maximum. Pulse energies of up to 0.16 mu J and peak electric fields of 13 MV/cm are achieved. Electro-optic sampling reveals a phase stability better than 0.1 pi over multiple hours, combined with free carrier-envelope phase tunability. The scalable scheme opens the door to strong-field terahertz optics at unprecedented repetition rates. (C) 2017 Optical Society of Americ

Visibility in Information Spaces and in Geographic Environments. Post-Proceedings of the KI'11 Workshop (October 4th, 2011, TU Berlin, Germany)

In the post-proceedings of the Workshop "Visibility in Information Spaces and in Geographic Environments" a selection of research papers is presented where the topic of visibility is addressed in different contexts. Visibility governs information selection in geographic environments as well as in information spaces and in cognition. The users of social media navigate in information spaces and at the same time, as embodied agents, they move in geographic environments. Both activities follow a similar type of information economy in which decisions by individuals or groups require a highly selective filtering to avoid information overload. In this context, visibility refers to the fact that in social processes some actors, topics or places are more salient than others. Formal notions of visibility include the centrality measures from social network analysis or the plethora of web page ranking methods. Recently, comparable approaches have been proposed to analyse activities in geographic environments: Place Rank, for instance, describes the social visibility of urban places based on the temporal sequence of tourist visit patterns. The workshop aimed to bring together researchers from AI, Geographic Information Science, Cognitive Science, and other disciplines who are interested in understanding how the different forms of visibility in information spaces and geographic environments relate to one another and how the results from basic research can be used to improve spatial search engines, geo-recommender systems or location-based social networks

Segmented flow generator for serial crystallography at the European X-ray free electron laser

Serial femtosecond crystallography (SFX) with X-ray free electron lasers (XFELs) allows structure determination of membrane proteins and time-resolved crystallography. Common liquid sample delivery continuously jets the protein crystal suspension into the path of the XFEL, wasting a vast amount of sample due to the pulsed nature of all current XFEL sources. The European XFEL (EuXFEL) delivers femtosecond (fs) X-ray pulses in trains spaced 100 ms apart whereas pulses within trains are currently separated by 889 ns. Therefore, continuous sample delivery via fast jets wastes >99% of sample. Here, we introduce a microfluidic device delivering crystal laden droplets segmented with an immiscible oil reducing sample waste and demonstrate droplet injection at the EuXFEL compatible with high pressure liquid delivery of an SFX experiment. While achieving ~60% reduction in sample waste, we determine the structure of the enzyme 3-deoxy-D-manno-octulosonate-8-phosphate synthase from microcrystals delivered in droplets revealing distinct structural features not previously reported

TXS 0506+056 with Updated IceCube Data

Past results from the IceCube Collaboration have suggested that the blazar TXS 0506+056 is a potential source of astrophysical neutrinos. However, in the years since there have been numerous updates to event processing and reconstruction, as well as improvements to the statistical methods used to search for astrophysical neutrino sources. These improvements in combination with additional years of data have resulted in the identification of NGC 1068 as a second neutrino source candidate. This talk will re-examine time-dependent neutrino emission from TXS 0506+056 using the most recent northern-sky data sample that was used in the analysis of NGC 1068. The results of using this updated data sample to obtain a significance and flux fit for the 2014 TXS 0506+056 "untriggered" neutrino flare are reported

Galactic Core-Collapse Supernovae at IceCube: “Fire Drill” Data Challenges and follow-up

The next Galactic core-collapse supernova (CCSN) presents a once-in-a-lifetime opportunity to make astrophysical measurements using neutrinos, gravitational waves, and electromagnetic radiation. CCSNe local to the Milky Way are extremely rare, so it is paramount that detectors are prepared to observe the signal when it arrives. The IceCube Neutrino Observatory, a gigaton water Cherenkov detector below the South Pole, is sensitive to the burst of neutrinos released by a Galactic CCSN at a level >10σ. This burst of neutrinos precedes optical emission by hours to days, enabling neutrinos to serve as an early warning for follow-up observation. IceCube\u27s detection capabilities make it a cornerstone of the global network of neutrino detectors monitoring for Galactic CCSNe, the SuperNova Early Warning System (SNEWS 2.0). In this contribution, we describe IceCube\u27s sensitivity to Galactic CCSNe and strategies for operational readiness, including "fire drill" data challenges. We also discuss coordination with SNEWS 2.0

All-Energy Search for Solar Atmospheric Neutrinos with IceCube

The interaction of cosmic rays with the solar atmosphere generates a secondary flux of mesons that decay into photons and neutrinos – the so-called solar atmospheric flux. Although the gamma-ray component of this flux has been observed in Fermi-LAT and HAWC Observatory data, the neutrino component remains undetected. The energy distribution of those neutrinos follows a soft spectrum that extends from the GeV to the multi-TeV range, making large Cherenkov neutrino telescopes a suitable for probing this flux. In this contribution, we will discuss current progress of a search for the solar neutrino flux by the IceCube Neutrino Observatory using all available data since 2011. Compared to the previous analysis which considered only high-energy muon neutrino tracks, we will additionally consider events produced by all flavors of neutrinos down to GeV-scale energies. These new events should improve our analysis sensitivity since the flux falls quickly with energy. Determining the magnitude of the neutrino flux is essential, since it is an irreducible background to indirect solar dark matter searches