Amstutz C. et al.

in 2016 IEEE-NPSS Real Time Conference, RT 2016 (2016), 7543110. DOI:10.1109/RTC.2016.7543110

Abstract

© 2016 IEEE.The CMS collaboration is preparing a major upgrade of its detector, so it can operate during the high luminosity run of the LHC from 2026. The upgraded tracker electronics will reconstruct the trajectories of charged particles within a latency of a few microseconds, so that they can be used by the level-1 trigger. An emulation framework, CIDAF, has been developed to provide a reference for a proposed FPGA-based implementation of this track finder, which employs a Time-Multiplexed (TM) technique for data processing.

Rota L., Balzer M., Caselle M., Kudella S., Weber M., Mozzanica A., Hiller N., Nasse M.J., Niehues G., Schonfeldt P., Gerth C., Steffen B., Walther S., Makowski D., Mielczarek A.

in 2016 IEEE-NPSS Real Time Conference, RT 2016 (2016), 7543157. DOI:10.1109/RTC.2016.7543157

Abstract

© 2016 IEEE. We developed a fast linear array detector to improve the acquisition rate and the resolution of Electro-Optical Spectral Decoding (EOSD) experimental setups currently installed at several light sources. The system consists of a detector board, an FPGA readout board and a high-Throughput data link. InGaAs or Si sensors are used to detect near-infrared (NIR) or visible light. The data acquisition, the operation of the detector board and its synchronization with synchrotron machines are handled by the FPGA. The readout architecture is based on a high-Throughput PCI-Express data link. In this paper we describe the system and we present preliminary measurements taken at the ANKA storage ring. A line-rate of 2.7 Mlps (lines per second) has been demonstrated.

Hahn S., Muller Y., Hofmann R., Moosmann J., Oktem O., Helfen L., Guigay J.-P., Van De Kamp T., Baumbach T.

in Physical Review A – Atomic, Molecular, and Optical Physics, 93 (2016), 053834. DOI:10.1103/PhysRevA.93.053834

Abstract

© 2016 American Physical Society. ©2016 American Physical Society. We analyze theoretically and investigate experimentally the transfer of phase to intensity power spectra of spatial frequencies through free-space Fresnel diffraction. Depending on λz (where λ is the wavelength and z is the free-space propagation distance) and the phase-modulation strength S, we demonstrate that for multiscale and broad phase spectra critical behavior transmutes a quasilinear to a nonlinear diffractogram except for low frequencies. On the contrary, a single-scale and broad phase spectrum induces a critical transition in the diffractogram at low frequencies. In both cases, identifying critical behavior encoded in the intensity power spectra is of fundamental interest because it exhibits the limits of perturbative power counting but also guides resolution and contrast optimization in propagation-based, single-distance, phase-contrast imaging, given certain dose and coherence constraints.

T. Baumbach, V. Altapova, D. Hänschke, T. dos Santos Rolo, A. Ershov, L. Helfen, T. van de Kamp, J.-T. Reszat, M. Weber, M. Caselle, M. Balzer, S. Chilingaryan, A. Kopmann, I. Dalinger, A. Myagotin, V. Asadchikov, A. Buzmakov, S. Tsapko, I. Tsapko, V. Vichugov, M. Sukhodoev, UFO collaboration

Final report, BMBF Programme: “Development and Use of Accelerator-Based Photon Sources”, 2016

Executive summary

Recent progress in X-ray optics, detector technology, and the tremendous increase of processing speed of commodity computational architectures gave rise to a paradigm shift in synchrotron X-ray imaging. In order to explore these technologies within the two UFO projects the UFO experimental station for ultra-fast X-ray imaging has been developed. Key components, an intelligent detector system, vast computational power, and sophisticated algorithms have been designed, optimized and integrated for best overall performance. New methods like 4D cine-tomography for in-vivo measurements have been established. This online assessment of sample dynamics not only made active image-based control possible, but also resulted in unprecedented image quality and largely increased throughput. Typically 400-500 high-quality datasets with 3D images and image sequences are recorded with the UFO experimental station during a beam time of about 3-4 days.

A flexible and fully automated sample environment and a detector system for a set of up to three complementary cameras has been realized. It can be equipped with commercial available scientific visible-light cameras or a custom UFO camera. To support academic sensor development a novel platform for scientific cameras, the UFO camera framework, has been developed. It is a unique rapid-prototyping environment to turn scientific image sensors into intelligent smart camera systems. All beamline components, sample environment, detector station and the computing infrastructure are seamlessly integrates into the high-level control system “Concert” designed for online data evaluation and feedback control.

As a new element computing nodes for online data assessment have been introduced in UFO. A powerful computing infrastructure based on GPUs and real-time storage has been developed. Optimized reconstruction algorithms reach a throughput of several GB/s with a single GPU server. For scalability also clusters are supported. Highly optimized reconstruction and image processing algorithms are key for real-time monitoring and efficient data analysis. In order to manage these algorithms the UFO parallel computing framework has been designed. It supports the implementation of efficient algorithms as well as the development of data processing workflows based on these. The library of optimized algorithms supports all modalities of operation at the UFO experimental station: tomography laminography and diffraction imaging as well as numerous pre- and post-processing steps.

The results of the UFO project have been reported at several national and international workshops and conferences. The UFO project contributes with developments like the UFO- camera framework or its GPU computing environment to other hard- and software projects in the synchrotron community (e.g. Tango Control System, High Data Rate Processing and Analysis Initiative, Nexus data format, Helmholtz Detector Technology and Systems Initiative DTS). Further follow-up projects base on the UFO results and improve imaging methods (like STROBOS-CODE) or add sophisticated analysis environments (like ASTOR).

The UFO project has successfully developed key components for ultra-fast X-ray imaging and serves as an example for future data intense applications. It demonstrates KIT’s role as technology center for novel synchrotron instrumentation.

Koenig T., Zuber M., Trimborn B., Farago T., Meyer P., Kunka D., Albrecht F., Kreuer S., Volk T., Fiederle M., Baumbach T.

in Physics in Medicine and Biology, 61 (2016) 3427-3442, 3427. DOI:10.1088/0031-9155/61/9/3427

Abstract

© 2016 Institute of Physics and Engineering in Medicine. The x-ray dark-field contrast accessible via grating interferometry is sensitive to features at length scales well below what is resolvable by a detector system. It is commonly explained as arising from small-angle x-ray scattering (SAXS), and can be implemented both at synchrotron beamlines and with low-brilliance sources such as x-ray tubes. Here, we demonstrate that for tube based setups the underlying process of image formation can be fundamentally different. For focal spots or detector pixels that comprise multiple grating periods, we show that dark-field images contain a strong artificial and system-specific component not arising from SAXS. Based on experiments carried out with a nanofocus x-ray tube and the example of an excised rat lung, we demonstrate that the dark-field contrast observed for porous media transforms into a differential phase contrast for large geometric magnifications. Using a photon counting detector with an adjustable point spread function, we confirm that a dark-field image can indeed be formed by an intra-pixel differential phase contrast that cannot be resolved as such due to a dephasing between the periodicities of the absorption grating and the Talbot carpet. Our findings are further corroborated by a link between the strength of this pseudo-dark-field contrast and our x-ray tube’s focal spot size in a three-grating setup. These results must not be ignored when measurements are intended to be reproducible across systems.

Huang D.-Y., Bechly G., Nel P., Engel M.S., Prokop J., Azar D., Cai C.-Y., Van De Kamp T., Staniczek A.H., Garrouste R., Krogmann L., Dos Santos Rolo T., Baumbach T., Ohlhoff R., Shmakov A.S., Bourgoin T., Nel A.

in Scientific Reports, 6 (2016), 23004. DOI:10.1038/srep23004

Abstract

With nearly 100,000 species, the Acercaria (lice, plant lices, thrips, bugs) including number of economically important species is one of the most successful insect lineages. However, its phylogeny and evolution of mouthparts among other issues remain debatable. Here new methods of preparation permitted the comprehensive anatomical description of insect inclusions from mid-Cretaceous Burmese amber in astonishing detail. These “missing links” fossils, attributed to a new order Permopsocida, provide crucial evidence for reconstructing the phylogenetic relationships in the Acercaria, supporting its monophyly, and questioning the position of Psocodea as sister group of holometabolans in the most recent phylogenomic study. Permopsocida resolves as sister group of Thripida + Hemiptera and represents an evolutionary link documenting the transition from chewing to piercing mouthparts in relation to suction feeding. Identification of gut contents as angiosperm pollen documents an ecological role of Permopsocida as early pollen feeders with relatively unspecialized mouthparts. This group existed for 185 million years, but has never been diverse and was superseded by new pollenivorous pollinators during the Cretaceous co-evolution of insects and flowers. The key innovation of suction feeding with piercing mouthparts is identified as main event that triggered the huge post-Carboniferous radiation of hemipterans, and facilitated the spreading of pathogenic vectors.

Rota L., Vogelgesang M., Perez L.E.A., Caselle M., Chilingaryan S., Dritschler T., Zilio N., Kopmann A., Balzer M., Weber M.

in Journal of Instrumentation, 11 (2016), P02007. DOI:10.1088/1748-0221/11/02/P02007

Abstract

© 2016 IOP Publishing Ltd and Sissa Medialab srl.Modern physics experiments produce multi-GB/s data rates. Fast data links and high performance computing stages are required for continuous data acquisition and processing. Because of their intrinsic parallelism and computational power, GPUs emerged as an ideal solution to process this data in high performance computing applications. In this paper we present a high-throughput platform based on direct FPGA-GPU communication. The architecture consists of a Direct Memory Access (DMA) engine compatible with the Xilinx PCI-Express core, a Linux driver for register access, and high- level software to manage direct memory transfers using AMD’s DirectGMA technology. Measurements with a Gen3 x8 link show a throughput of 6.4 GB/s for transfers to GPU memory and 6.6 GB/s to system memory. We also assess the possibility of using the architecture in low latency systems: preliminary measurements show a round-trip latency as low as 1 μs for data transfers to system memory, while the additional latency introduced by OpenCL scheduling is the current limitation for GPU based systems. Our implementation is suitable for real-time DAQ system applications ranging from photon science and medical imaging to High Energy Physics (HEP) systems.

Schwermann A.H., dos Santos Rolo T., Caterino M.S., Bechly G., Schmied H., Baumbach T., van de Kamp T.

in eLife, 5 (2016), e12129. DOI:10.7554/eLife.12129

Abstract

© Schwermann et al. External and internal morphological characters of extant and fossil organisms are crucial to establishing their systematic position, ecological role and evolutionary trends. The lack of internal characters and soft-tissue preservation in many arthropod fossils, however, impedes comprehensive phylogenetic analyses and species descriptions according to taxonomic standards for Recent organisms. We found well-preserved three-dimensional anatomy in mineralized arthropods from Paleogene fissure fillings and demonstrate the value of these fossils by utilizing digitally reconstructed anatomical structure of a hister beetle. The new anatomical data facilitate a refinement of the species diagnosis and allowed us to reject a previous hypothesis of close phylogenetic relationship to an extant congeneric species. Our findings suggest that mineralized fossils, even those of macroscopically poor preservation, constitute a rich but yet largely unexploited source of anatomical data for fossil arthropods.

Caselle M., Blank T., Colombo F., Dierlamm A., Husemann U., Kudella S., Weber M.

in Journal of Instrumentation, 11 (2016), C01050. DOI:10.1088/1748-0221/11/01/C01050

Abstract

© 2016 IOP Publishing Ltd and Sissa Medialab srl.In the next generation of collider experiments detectors will be challenged by unprecedented particle fluxes. Thus large detector arrays of highly pixelated detectors with minimal dead area will be required at reasonable costs. Bump-bonding of pixel detectors has been shown to be a major cost-driver. KIT is one of five production centers of the CMS barrel pixel detector for the Phase I Upgrade. In this contribution the SnPb bump-bonding process and the production yield is reported. In parallel to the production of the new CMS pixel detector, several alternatives to the expensive photolithography electroplating/electroless metal deposition technologies are developing. Recent progress and challenges faced in the development of bump-bonding technology based on gold-stud bonding by thin (15 μm) gold wire is presented. This technique allows producing metal bumps with diameters down to 30 μm without using photolithography processes, which are typically required to provide suitable under bump metallization. The short setup time for the bumping process makes gold-stud bump-bonding highly attractive (and affordable) for the flip-chipping of single prototype ICs, which is the main limitation of the current photolithography processes.

Briceno R.D., Eberhard W.G., Chinea-Cano E., Wegrzynek D., Dos Santos Rolo T.

in Ethology Ecology and Evolution, 28 (2016) 53-76. DOI:10.1080/03949370.2014.1002114

Abstract

© 2015 Dipartimento di Biologia, Università di Firenze, Italia. A long-standing question in morphological evolution is why male genitalia tend to diverge more rapidly than other structures. One possible explanation is that male genitalia are under sexual selection to function as internal courtship devices. Males of closely related species may provide divergent stimulation using different genital morphologies and behaviors. Testing this hypothesis has been difficult, however, because the presumed genital courtship behavior is often hidden from view inside the female, and because studies of how the males genitalia interact with those of the female are nearly always limited to a single species in a given group, thus restricting opportunities for comparison of closely related species. We present new morphological and behavioral data for portions of the male genitalia that are hidden in the female during copulation in five species in the tsetse fly genus Glossina using data from dissections of pairs frozen in copula, artificially stimulated males, and from copulating pairs viewed with a new X-ray technique that allows events inside the female to be recorded in real time. These data almost certainly give only an incomplete view of this complex, previously hidden world. But even so they clearly reveal that, as predicted by sexual selection theory, the male genitalia of Glossina flies perform dramatic, stereotyped, rhythmic movements deep within the females reproductive tract and in inward folds of her external surface, and that many of these movements probably differ among closely related species. Most of the movements are not explicable as means by which the male anchors himself more securely to the female; all are likely to result in stimulation of the female. A female Glossina can be stimulated tactilely at a given moment during copulation at up to 8-10 or more different sites on her body.