264 results on '"M Wieser"'
Search Results
2. Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission
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S. Orsini, A. Milillo, H. Lichtenegger, A. Varsani, S. Barabash, S. Livi, E. De Angelis, T. Alberti, G. Laky, H. Nilsson, M. Phillips, A. Aronica, E. Kallio, P. Wurz, A. Olivieri, C. Plainaki, J. A. Slavin, I. Dandouras, J. M. Raines, J. Benkhoff, J. Zender, J.-J. Berthelier, M. Dosa, G. C. Ho, R. M. Killen, S. McKenna-Lawlor, K. Torkar, O. Vaisberg, F. Allegrini, I. A. Daglis, C. Dong, C. P. Escoubet, S. Fatemi, M. Fränz, S. Ivanovski, N. Krupp, H. Lammer, François Leblanc, V. Mangano, A. Mura, R. Rispoli, M. Sarantos, H. T. Smith, M. Wieser, F. Camozzi, A. M. Di Lellis, G. Fremuth, F. Giner, R. Gurnee, J. Hayes, H. Jeszenszky, B. Trantham, J. Balaz, W. Baumjohann, M. Cantatore, D. Delcourt, M. Delva, M. Desai, H. Fischer, A. Galli, M. Grande, M. Holmström, I. Horvath, K. C. Hsieh, R. Jarvinen, R. E. Johnson, A. Kazakov, K. Kecskemety, H. Krüger, C. Kürbisch, Frederic Leblanc, M. Leichtfried, E. Mangraviti, S. Massetti, D. Moissenko, M. Moroni, R. Noschese, F. Nuccilli, N. Paschalidis, J. Ryno, K. Seki, A. Shestakov, S. Shuvalov, R. Sordini, F. Stenbeck, J. Svensson, S. Szalai, K. Szego, D. Toublanc, N. Vertolli, R. Wallner, and A. Vorburger
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Science - Abstract
Abstract Mercury’s southern inner magnetosphere is an unexplored region as it was not observed by earlier space missions. In October 2021, BepiColombo mission has passed through this region during its first Mercury flyby. Here, we describe the observations of SERENA ion sensors nearby and inside Mercury’s magnetosphere. An intermittent high-energy signal, possibly due to an interplanetary magnetic flux rope, has been observed downstream Mercury, together with low energy solar wind. Low energy ions, possibly due to satellite outgassing, were detected outside the magnetosphere. The dayside magnetopause and bow-shock crossing were much closer to the planet than expected, signature of a highly eroded magnetosphere. Different ion populations have been observed inside the magnetosphere, like low latitude boundary layer at magnetopause inbound and partial ring current at dawn close to the planet. These observations are important for understanding the weak magnetosphere behavior so close to the Sun, revealing details never reached before.
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- 2022
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3. PROJECT INDIGO – DOCUMENT, DISSEMINATE & ANALYSE A GRAFFITI-SCAPE
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G. Verhoeven, B. Wild, J. Schlegel, M. Wieser, N. Pfeifer, S. Wogrin, L. Eysn, M. Carloni, B. Koschiček-Krombholz, A. Molada-Tebar, J. Otepka-Schremmer, C. Ressl, M. Trognitz, and A. Watzinger
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Technology ,Engineering (General). Civil engineering (General) ,TA1-2040 ,Applied optics. Photonics ,TA1501-1820 - Abstract
Graffiti is a short-lived form of heritage balancing between tangible and intangible, offensive and pleasant. Graffiti makes people laugh, wonder, angry, think. These conflicting traits are all present along Vienna's Donaukanal (Eng. Danube Canal), a recreational hotspot – located in the city's heart – famous for its endless display of graffiti. The graffiti-focused heritage science project INDIGO aims to build the basis to systematically document, monitor, and analyse circa 13 km of Donaukanal graffiti in the next decade. The first part of this paper details INDIGO's goals and overarching methodological framework, simultaneously placing it into the broader landscape of graffiti research. The second part of the text concentrates on INDIGO's graffiti documentation activities. Given the project's aim to create a spatially, spectrally, and temporally accurate record of all possible mark-makings attached in (il)legal ways to the public urban surfaces of the Donaukanal, it seems appropriate to provide insights on the photographic plus image-based modelling activities that form the foundation of INDIGO's graffiti recording strategy. The text ends with some envisioned strategies to streamline image acquisition and process the anticipated hundreds of thousands of images.
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- 2022
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4. Neutralized solar energetic particles for SEP forecasting: Feasibility study of an innovative technique for space weather applications
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Xiao-Dong Wang, B. Klecker, G. Nicolaou, S. Barabash, M. Wieser, P. Wurz, A. Galli, F. Cipriani, and Y. Futaana
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solar energetic particles ,energetic neutral atoms ,space weather ,numerical simulation ,Science ,Geophysics. Cosmic physics ,QC801-809 ,Environmental sciences ,GE1-350 - Abstract
Energetic neutral atoms (ENAs) are produced by the neutralization of energetic ions formed by shock-accelerated gradual solar energetic particle events (SEP). These high-energy ENAs (HENAs) can reach the Earth earlier than the associated SEPs and thus can provide information about the SEPs at the lower corona. The HENA properties observed at Earth depend on the properties of the coronal mass ejection (CME)-driven shocks that accelerate the SEPs. Using a model of HENA production in a shock-accelerated SEP event, we semi-quantitatively investigate the energy-time spectrum of HENAs depending on the width, propagation speed, and direction of the shock, as well as the density and ion abundances of the lower corona. Compared to the baseline model parameters, the cases with a wider shock width angle or a higher coronal density would increase the HENA flux observed at the Earth, while the case with an Earth-propagating shock shows a softened HENA spectrum. The comparison of expected HENA fluxes in different cases with a flight-proven ENA instrument suggests that solar HENAs can feasibly be monitored with current technologies, which could provide a lead time of 2−3 hours for SEPs at a few MeV. We propose that monitoring of solar HENAs could provide a new method to forecast shock-driven SEP events that are capable of significant space weather impacts on the near-Earth environment.
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- 2022
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5. Simulations of Energetic Neutral Atom Sputtering From Ganymede in Preparation for the JUICE Mission
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A. Pontoni, M. Shimoyama, Y. Futaana, S. Fatemi, A. R. Poppe, M. Wieser, and S. Barabash
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- 2022
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6. SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo
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S. Orsini, S.A. Livi, H. Lichtenegger, S. Barabash, A. Milillo, E. De Angelis, M. Phillips, G. Laky, M. Wieser, A. Olivieri, C. Plainaki, G. Ho, R.M. Killen, J.A. Slavin, P. Wurz, J.-J. Berthelier, I. Dandouras, E. Kallio, S. McKenna-Lawlor, S. Szalai, K. Torkar, O. Vaisberg, F. Allegrini, I.A. Daglis, C. Dong, C.P. Escoubet, S. Fatemi, M. Fränz, S. Ivanovski, N. Krupp, H. Lammer, François Leblanc, V. Mangano, A. Mura, H. Nilsson, J.M. Raines, R. Rispoli, M. Sarantos, H.T. Smith, K. Szego, A. Aronica, F. Camozzi, A.M. Di Lellis, G. Fremuth, F. Giner, R. Gurnee, J. Hayes, H. Jeszenszky, F. Tominetti, B. Trantham, J. Balaz, W. Baumjohann, D. Brienza, U. Bührke, M.D. Bush, M. Cantatore, S. Cibella, L. Colasanti, G. Cremonese, L. Cremonesi, M. D’Alessandro, D. Delcourt, M. Delva, M. Desai, M. Fama, M. Ferris, H. Fischer, A. Gaggero, D. Gamborino, P. Garnier, W.C. Gibson, R. Goldstein, M. Grande, V. Grishin, D. Haggerty, M. Holmström, I. Horvath, K.-C. Hsieh, A. Jacques, R.E. Johnson, A. Kazakov, K. Kecskemety, H. Krüger, C. Kürbisch, F. Lazzarotto, Frederic Leblanc, M. Leichtfried, R. Leoni, A. Loose, D. Maschietti, S. Massetti, F. Mattioli, G. Miller, D. Moissenko, A. Morbidini, R. Noschese, F. Nuccilli, C. Nunez, N. Paschalidis, S. Persyn, D. Piazza, M. Oja, J. Ryno, W. Schmidt, J.A. Scheer, A. Shestakov, S. Shuvalov, K. Seki, S. Selci, K. Smith, R. Sordini, J. Svensson, L. Szalai, D. Toublanc, C. Urdiales, A. Varsani, N. Vertolli, R. Wallner, P. Wahlstroem, P. Wilson, and S. Zampieri
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Space Sciences (General) - Abstract
The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase.
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- 2021
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7. EVALUATION OF A NOVEL UAV-BORNE TOPO-BATHYMETRIC LASER PROFILER
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G. Mandlburger, M. Pfennigbauer, M. Wieser, U. Riegl, and N. Pfeifer
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Technology ,Engineering (General). Civil engineering (General) ,TA1-2040 ,Applied optics. Photonics ,TA1501-1820 - Abstract
We present a novel topo-bathymetric laser profiler. The sensor system (RIEGL BathyCopter) comprises a laser range finder, an Inertial Measurement Unit (IMU), a Global Navigation Satellite System (GNSS) receiver, a control unit, and digital cameras mounted on an octocopter UAV (RiCOPTER). The range finder operates on the time-of-flight measurement principle and utilizes very short laser pulses (
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- 2016
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8. ULS LiDAR SUPPORTED ANALYSES OF LASER BEAM PENETRATION FROM DIFFERENT ALS SYSTEMS INTO VEGETATION
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M. Wieser, M. Hollaus, G. Mandlburger, P. Glira, and N. Pfeifer
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Technology ,Engineering (General). Civil engineering (General) ,TA1-2040 ,Applied optics. Photonics ,TA1501-1820 - Abstract
This study analyses the underestimation of tree and shrub heights for different airborne laser scanner systems and point cloud distribution within the vegetation column. Reference data was produced by a novel UAV-borne laser scanning (ULS) with a high point density in the complete vegetation column. With its physical parameters (e.g. footprint) and its relative accuracy within the block as stated in Section 2.2 the reference data is supposed to be highly suitable to detect the highest point of the vegetation. An airborne topographic (ALS) and topo-bathymetric (ALB) system were investigated. All data was collected in a period of one month in leaf-off condition, while the dominant tree species in the study area are deciduous trees. By robustly estimating the highest 3d vegetation point of each laser system the underestimation of the vegetation height was examined in respect to the ULS reference data. This resulted in a higher under-estimation of the airborne topographic system with 0.60 m (trees) and 0.55 m (shrubs) than for the topo-bathymetric system 0.30 m (trees) and 0.40 m (shrubs). The degree of the underestimation depends on structural characteristics of the vegetation itself and physical specification of the laser system.
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- 2016
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9. Cyclic Lateral Load Test of a Wall with Timber Frame Structure and Lightearth Envelope
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G. Becerra, S. Onnis, G. Meli, M. Wieser, and J. Vargas-Neumann
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- 2023
10. Traitement chirurgical d’une fistule recto-vésicale selon la technique de York Mason (avec vidéo)
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B. Romain, M. Wieser, and S. Rohr
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Surgery - Published
- 2022
11. Moonraker -- Enceladus Multiple Flyby Mission
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O. Mousis, A. Bouquet, Y. Langevin, N. André, H. Boithias, G. Durry, F. Faye, P. Hartogh, J. Helbert, L. Iess, S. Kempf, A. Masters, F. Postberg, J.-B. Renard, P. Vernazza, A. Vorburger, P. Wurz, D. H. Atkinson, S. Barabash, M. Berthomier, J. Brucato, M. Cable, J. Carter, S. Cazaux, A. Coustenis, G. Danger, V. Dehant, T. Fornaro, P. Garnier, T. Gautier, O. Groussin, L. Z. Hadid, J.-C. Ize, I. Kolmasova, J.-P. Lebreton, S. Le Maistre, E. Lellouch, J. I. Lunine, K. E. Mandt, Z. Martins, D. Mimoun, Q. Nenon, G. M. Muñoz Caro, P. Rannou, H. Rauer, P. Schmitt-Kopplin, A. Schneeberger, M. Simons, K. Stephan, T. Van Hoolst, J. Vaverka, M. Wieser, L. Wörner, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Physique des interactions ioniques et moléculaires (PIIM), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), UCL - SST/ELI/ELIC - Earth & Climate, Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Institut d'astrophysique spatiale (IAS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Airbus Defence and Space [Les Mureaux], ASTRIUM, Groupe de spectrométrie moléculaire et atmosphérique (GSMA), Université de Reims Champagne-Ardenne (URCA)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Max-Planck-Gesellschaft, DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR), Dipartimento di Ingegneria Meccanica e Aerospaziale [Roma La Sapienza] (DIMA), Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Laboratory for Atmospheric and Space Physics [Boulder] (LASP), University of Colorado [Boulder], Imperial College London, Institute of Geological Sciences [Berlin], Department of Earth Sciences [Berlin], Free University of Berlin (FU)-Free University of Berlin (FU), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Physics Institute [Bern], University of Bern, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Swedish Institute of Space Physics [Kiruna] (IRF), Laboratoire de Physique des Plasmas (LPP), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École polytechnique (X)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Faculty of Aerospace Engineering [Delft], Delft University of Technology (TU Delft), Leiden Observatory [Leiden], Universiteit Leiden, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Royal Observatory of Belgium [Brussels] (ROB), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institute of Atmospheric Physics [Prague] (IAP), Czech Academy of Sciences [Prague] (CAS), Faculty of Mathematics and Physics [Praha/Prague], Charles University [Prague] (CU), Department of Astronomy [Ithaca], Cornell University [New York], Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), Centro de Quimica Estrutural (CQE), Instituto Superior Técnico, Universidade Técnica de Lisboa (IST), Institut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Centro de Astrobiologia [Madrid] (CAB), Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Max-Planck-Institut für Extraterrestrische Physik (MPE), Seismological Laboratory, California Institute of Technology, California Institute of Technology (CALTECH), and DLR Institute of Quantum Technologies
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530 Physics ,ISOTOPOLOGUES ,MU-M ,FOS: Physical sciences ,Saturnian satellites ,Astronomy & Astrophysics ,moon ,Enceladus ,[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology ,Earth and Planetary Sciences (miscellaneous) ,Interdisciplinary astronomy ,INTERIOR STRUCTURE ,ION ,Habitable planets ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,CALIBRATION ,Earth and Planetary Astrophysics (astro-ph.EP) ,Science & Technology ,SPECTROSCOPY ,GRAVITY-FIELD ,520 Astronomy ,500 Naturwissenschaften und Mathematik::520 Astronomie::520 Astronomie und zugeordnete Wissenschaften ,Astronomy and Astrophysics ,CASSINI ,Astrobiology ,620 Engineering ,PLUME ,Geophysics ,Saturn ,[SDU]Sciences of the Universe [physics] ,Space and Planetary Science ,MASS-SPECTROMETER ,Physical Sciences ,Ocean planets ,Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Earth and Planetary Astrophysics - Abstract
Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could be a habitable environment having a complex interaction with the rocky core. Further investigation of the composition of the plume formed by the jets is necessary to fully understand the ocean, its potential habitability, and what it tells us about Enceladus' origin. Moonraker has been proposed as an ESA M-class mission designed to orbit Saturn and perform multiple flybys of Enceladus, focusing on traversals of the plume. The proposed Moonraker mission consists of an ESA-provided platform, with strong heritage from JUICE and Mars Sample Return, and carrying a suite of instruments dedicated to plume and surface analysis. The nominal Moonraker mission has a duration of 13.5 years. It includes a 23-flyby segment with 189 days allocated for the science phase, and can be expanded with additional segments if resources allow. The mission concept consists in investigating: i) the habitability conditions of present-day Enceladus and its internal ocean, ii) the mechanisms at play for the communication between the internal ocean and the surface of the South Polar Terrain, and iii) the formation conditions of the moon. Moonraker, thanks to state-of-the-art instruments representing a significant improvement over Cassini's payload, would quantify the abundance of key species in the plume, isotopic ratios, and physical parameters of the plume and the surface. Such a mission would pave the way for a possible future landed mission., Accepted for publication in The Planetary Science Journal
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- 2022
12. New Models of PADI, an Ultrafast Preamplifier–Discriminator ASIC for Time-of-Flight Measurements
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J. Frühauf, H. Deppe, S. Lochner, H. Flemming, Octav Marghitu, Vlad Constantinescu, N. Herrmann, H. Andersson, P.-A. Loizeau, M. Wieser, I. M. Deppner, and M. Ciobanu
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Physics ,Nuclear and High Energy Physics ,Discriminator ,Preamplifier ,business.industry ,Detector ,Electrical engineering ,Integrated circuit ,Chip ,law.invention ,Nuclear Energy and Engineering ,CMOS ,Application-specific integrated circuit ,law ,Facility for Antiproton and Ion Research ,Electrical and Electronic Engineering ,business - Abstract
The general-purpose PreAmplifier–DIscriminator application-specific integrated circuit (ASIC) chip, PADI, was originally designed to be used as front-end electronics (FEE) for reading out the timing resistive plate chambers in the time-of-flight (TOF) wall of the compressed baryonic matter (CBM) experiment of the future Facility for Antiproton and Ion Research (FAIR) facility in Darmstadt, Germany. Here, we present the last models of this 0.18- $\mu \text{m}$ CMOS technology—PADI-X, PADI-XI, and PADI-XII—as well as their key features and test results. While the PADI series was originally developed for high-energy physics experiments carried out at ground facilities, it turned out that PADI is also suitable for space experiments and PADI-X was selected for one sensor of the European Space Agency, JUpiter ICy moons Explore (JUICE) mission. Currently, the most recent model of the series, PADI-XII, has been tuned for space applications and the prototype batch is currently under production.
- Published
- 2021
13. Chapter 6 Using isotopic abundances to follow anthropogenic emissions: an example of sulfur, oxygen and boron isotopes in a Canadian watershed
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A. L. Norman, J Xie, C. Kruschel, and M Wieser
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- 2022
14. Analysing the suitability of radiometrically calibrated full-waveform lidar data for delineating Alpine rock glaciers
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A. Roncat, M. Wieser, C. Briese, E. Bollmann, R. Sailer, C. Klug, and N. Pfeifer
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Technology ,Engineering (General). Civil engineering (General) ,TA1-2040 ,Applied optics. Photonics ,TA1501-1820 - Abstract
With full-waveform (FWF) lidar systems becoming increasingly available from different commercial manufacturers, the possibility for extracting physical parameters of the scanned surfaces in an area-wide sense, as addendum to their geometric representation, has risen as well. The mentioned FWF systems digitize the temporal profiles of the transmitted laser pulse and of its backscattered echoes, allowing for a reliable determination of the target distance to the instrument and of physical target quantities by means of radiometric calibration, one of such quantities being the diffuse Lambertian reflectance. The delineation of glaciers is a time-consuming task, commonly performed manually by experts and involving field trips as well as image interpretation of orthophotos, digital terrain models and shaded reliefs. In this study, the diffuse Lambertian reflectance was compared to the glacier outlines mapped by experts. We start the presentation with the workflow for analysis of FWF data, their direct georeferencing and the calculation of the diffuse Lambertian reflectance by radiometric calibration; this workflow is illustrated for a large FWF lidar campaign in the Ötztal Alps (Tyrol, Austria), operated with an Optech ALTM 3100 system. The geometric performance of the presented procedure was evaluated by means of a relative and an absolute accuracy assessment using strip differences and orthophotos, resp. The diffuse Lambertian reflectance was evaluated at two rock glaciers within the mentioned lidar campaign. This feature showed good performance for the delineation of the rock glacier boundaries, especially at their lower parts.
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- 2013
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15. POSITIONING IN TIME AND SPACE – COST-EFFECTIVE EXTERIOR ORIENTATION FOR AIRBORNE ARCHAEOLOGICAL PHOTOGRAPHS
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G. Verhoeven, M. Wieser, C. Briese, and M. Doneus
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Technology ,Engineering (General). Civil engineering (General) ,TA1-2040 ,Applied optics. Photonics ,TA1501-1820 - Abstract
Since manned, airborne aerial reconnaissance for archaeological purposes is often characterised by more-or-less random photographing of archaeological features on the Earth, the exact position and orientation of the camera during image acquisition becomes very important in an effective inventorying and interpretation workflow of these aerial photographs. Although the positioning is generally achieved by simultaneously logging the flight path or directly recording the camera's position with a GNSS receiver, this approach does not allow to record the necessary roll, pitch and yaw angles of the camera. The latter are essential elements for the complete exterior orientation of the camera, which allows – together with the inner orientation of the camera – to accurately define the portion of the Earth recorded in the photograph. This paper proposes a cost-effective, accurate and precise GNSS/IMU solution (image position: 2.5 m and orientation: 2°, both at 1σ) to record all essential exterior orientation parameters for the direct georeferencing of the images. After the introduction of the utilised hardware, this paper presents the developed software that allows recording and estimating these parameters. Furthermore, this direct georeferencing information can be embedded into the image's metadata. Subsequently, the first results of the estimation of the mounting calibration (i.e. the misalignment between the camera and GNSS/IMU coordinate frame) are provided. Furthermore, a comparison with a dedicated commercial photographic GNSS/IMU solution will prove the superiority of the introduced solution. Finally, an outlook on future tests and improvements finalises this article.
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- 2013
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16. Cure de hernie inguinale selon la technique de Lichtenstein sous anesthésie locale (avec vidéo)
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M. Wieser, S. Rohr, and B. Romain
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business.industry ,Medicine ,Surgery ,business - Published
- 2021
17. Inguinal hernia repair using the Lichtenstein technique under local anesthesia (with video)
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S. Rohr, B. Romain, and M. Wieser
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medicine.medical_specialty ,business.industry ,General surgery ,Hernia, Inguinal ,General Medicine ,Surgical Mesh ,medicine.disease ,Inguinal hernia ,Recurrence ,Humans ,Medicine ,Local anesthesia ,business ,Herniorrhaphy ,Anesthesia, Local - Published
- 2021
18. Surgical treatment of a recto-urinary fistula using the York Mason procedure (with video)
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B. Romain, M. Wieser, and S. Rohr
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Urinary Fistula ,Urethral Diseases ,Rectum ,Humans ,Rectal Fistula ,General Medicine - Published
- 2022
19. Neutralized Solar Energetic Particles for SEP Forecasting: Feasibility Study of an Innovative Technique for Space Weather Applications
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M. Wieser, Peter Wurz, F. Cipriani, and Y. Futaana, André Galli, S. Barabash, X. Wang, Berndt Klecker, and Georgios Nicolaou
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Physics ,Atmospheric Science ,Solar energetic particles ,Energetic neutral atom ,Astrophysics::High Energy Astrophysical Phenomena ,520 Astronomy ,Astronomy and Astrophysics ,Space weather ,620 Engineering ,Corona ,Shock (mechanics) ,Computational physics ,Ion ,Space and Planetary Science ,Physics::Space Physics ,Coronal mass ejection ,Astrophysics::Solar and Stellar Astrophysics ,Event (particle physics) - Abstract
Energetic neutral atoms (ENAs) are produced by the neutralization of energetic ions formed by shock-accelerated gradual solar energetic particle events (SEP). These high-energy ENAs (HENAs) can reach the Earth earlier than the associated SEPs and provide information about the SEPs at the lower corona. The HENA properties observed at Earth depend on the properties of the coronal mass ejection (CME)-driven shocks that accelerate the SEPs. With a model of HENA production in a shock-accelerated SEP event, we semi-quantitatively investigate the energy-time spectrum of HENAs depending on the width, propagation speed, and direction of the shock, as well as the density and ion abundances of the lower corona. Compared to the baseline model parameters, the cases with a wider shock width angle or a higher coronal density would increase the HENA flux observed at the Earth, while the case with an Earth-propagating shock shows a softened HENA spectrum. The comparison of expected HENA fluxes in different cases with a flight-proven ENA instrument suggests that solar HENAs can feasibly be monitored with current technologies, which could provide a lead time of 2-3 hours for SEPs at a few MeV. We propose that monitoring of solar HENAs could provide a new method to forecast shock-driven SEP events that could have significant space weather impacts on the near-Earth environment.
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- 2022
- Full Text
- View/download PDF
20. Correction to: SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo
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Raffaella Noschese, A. Loose, S. Barabash, A. Varsani, Markus Fränz, Diana Gamborino, Sándor Szalai, François Leblanc, Roberto Leoni, John Hayes, Stefano Livi, J. A. Scheer, A. Olivieri, F. Tominetti, Jim M. Raines, C. Kürbisch, Peter Wurz, Jean-Jacques Berthelier, Mats Holmström, Chuanfei Dong, Klaus Torkar, D. Toublanc, M. Ferris, G. Cremonese, Robert E. Johnson, Norbert Krupp, Menelaos Sarantos, M. D. Bush, Istvan Dr Horvath, George C. Ho, Magda Delva, G. Fremuth, A. M. Di Lellis, Raymond Goldstein, A. Aronica, Rosanna Rispoli, M. I. Desai, N. Vertolli, Stavro Ivanovski, Philippe Garnier, G. Laky, K. C. Hsieh, Nikolaos Paschalidis, L. Cremonesi, D. Brienza, Dominique Delcourt, B. Trantham, Kanako Seki, Ioannis A. Daglis, Iannis Dandouras, Harald Krüger, M. Leichtfried, Alessandro Gaggero, Karoly Szego, P. Wahlstroem, Frederic Allegrini, M. Cantatore, F. Giner, H. Jeszenszky, Manuel Grande, Wolfgang Baumjohann, F. Leblanc, Fabrizio Nuccilli, R. Wallner, A. D. Jacques, D. Maschietti, M. Wieser, Stefano Massetti, Walter Schmidt, Esa Kallio, Karoly Kecskemety, Dennis Haggerty, S. Zampieri, Anna Milillo, Greg Miller, S. Shuvalov, Helmut Lammer, H. Fischer, Francesco Lazzarotto, M. Oja, A. Shestakov, C. P. Escoubet, Shahab Fatemi, Roberto Sordini, J. Ryno, O. L. Vaisberg, V. Grishin, V. Mangano, Fabio Camozzi, L. Colasanti, W. C. Gibson, Adrian Kazakov, Alessandro Mura, D. Moissenko, Stefano Selci, Rosemary M. Killen, Kerrington D. Smith, Howard Smith, L. Szalai, Francesco Mattioli, Johan Svensson, S. M. P. McKenna-Lawlor, Hans Nilsson, R. S. Gurnee, C. Nunez, Mark Phillips, E. De Angelis, M. Famá, S. Persyn, P. Wilson, Daniele Piazza, Marco D'Alessandro, Alfredo Morbidini, U. Bührke, C. Urdiales, Herbert Lichtenegger, Christina Plainaki, J. Balaz, James A. Slavin, Sara Cibella, Stefano Orsini, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)
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010504 meteorology & atmospheric sciences ,Suite ,chemistry.chemical_element ,Astronomy and Astrophysics ,01 natural sciences ,Mercury (element) ,Astrobiology ,Planetary science ,chemistry ,[SDU]Sciences of the Universe [physics] ,Space and Planetary Science ,0103 physical sciences ,Environmental science ,Particle ,010303 astronomy & astrophysics ,ComputingMilieux_MISCELLANEOUS ,0105 earth and related environmental sciences - Abstract
International audience
- Published
- 2021
21. SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo
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Hans Nilsson, R. S. Gurnee, Wolfgang Baumjohann, Howard Smith, Menelaos Sarantos, Mark Phillips, Iannis Dandouras, S. Shuvalov, V. Grishin, D. Moissenko, Stavro Ivanovski, Johan Svensson, John Hayes, Markus Fränz, Stefano Orsini, Francesco Lazzarotto, S. Persyn, Stefano Selci, Rosemary M. Killen, S. M. P. McKenna-Lawlor, V. Mangano, Diana Gamborino, Sándor Szalai, B. Trantham, P. Wilson, M. Oja, M. Cantatore, François Leblanc, Peter Wurz, H. Jeszenszky, Dominique Delcourt, Chuanfei Dong, Helmut Lammer, A. Shestakov, A. Aronica, A. Loose, S. Barabash, H. Fischer, E. De Angelis, M. Famá, M. Wieser, C. Nunez, Harald Krüger, Kerrington D. Smith, George C. Ho, G. Laky, L. Cremonesi, Mats Holmström, Manuel Grande, C. Kürbisch, Raffaella Noschese, D. Toublanc, Fabio Camozzi, C. P. Escoubet, L. Szalai, Francesco Mattioli, P. Wahlstroem, D. Maschietti, James A. Slavin, N. Vertolli, L. Colasanti, Frederic Allegrini, F. Giner, Jean-Jacques Berthelier, W. C. Gibson, Roberto Leoni, Dennis Haggerty, Stefano Massetti, Fabrizio Nuccilli, R. Wallner, S. Zampieri, Anna Milillo, Magda Delva, G. Fremuth, A. M. Di Lellis, Raymond Goldstein, Sara Cibella, Esa Kallio, Greg Miller, Walter Schmidt, Alessandro Gaggero, J. A. Scheer, M. I. Desai, Philippe Garnier, U. Bührke, Shahab Fatemi, Karoly Kecskemety, D. Brienza, Marco D'Alessandro, Adrian Kazakov, M. Leichtfried, Karoly Szego, Stefano Livi, A. Olivieri, F. Tominetti, A. D. Jacques, Alfredo Morbidini, Istvan Dr Horvath, Nikolaos Paschalidis, Daniele Piazza, Ioannis A. Daglis, Alessandro Mura, C. Urdiales, Herbert Lichtenegger, Christina Plainaki, Jim M. Raines, J. Balaz, Rosanna Rispoli, K. C. Hsieh, Kanako Seki, F. Leblanc, Roberto Sordini, J. Ryno, O. L. Vaisberg, A. Varsani, M. D. Bush, Klaus Torkar, M. Ferris, G. Cremonese, Robert E. Johnson, Norbert Krupp, Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Southwest Research Institute [San Antonio] (SwRI), Department of Climate and Space Sciences and Engineering (CLaSP), University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Space Research Institute of Austrian Academy of Sciences (IWF), Austrian Academy of Sciences (OeAW), Swedish Institute of Space Physics [Kiruna] (IRF), Italian Space Agency, Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), NASA Goddard Space Flight Center (GSFC), Physics Institute [Bern], University of Bern, HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Department of Electronics and Nanoengineering [Espoo], School of Electrical Engineering [Aalto Univ], Aalto University-Aalto University, Space Technology Ireland Limited, Wigner Research Centre for Physics [Budapest], Hungarian Academy of Sciences (MTA), Space Research Institute of the Russian Academy of Sciences (IKI), Russian Academy of Sciences [Moscow] (RAS), Department of Physics [Athens], National and Kapodistrian University of Athens (NKUA), Princeton Plasma Physics Laboratory (PPPL), Princeton University, Research and Scientific Support Department, ESTEC (RSSD), European Space Research and Technology Centre (ESTEC), Agence Spatiale Européenne = European Space Agency (ESA)-Agence Spatiale Européenne = European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Max-Planck-Gesellschaft, INAF - Osservatorio Astronomico di Trieste (OAT), Institut für Weltraumforschung = Space Research institute [Graz] (IWF), Osterreichische Akademie der Wissenschaften (ÖAW), Laboratory for Atmospheric and Space Physics [Boulder] (LASP), University of Colorado [Boulder], CNR Institute for Photonics and Nanotechnologies (IFN), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), INAF - Osservatorio Astronomico di Padova (OAPD), Istituto di Struttura della Materia (CNR-ISM), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Comisión Nacional de Energía Atómica [ARGENTINA] (CNEA), Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Institute of Mathematical and Physical Sciences [Aberystwyth], University of Wales, University of Arizona, Department of Materials Science and Engineering [Charlottesville] (MS), University of Virginia, Laboratoire de Physique des Plasmas (LPP), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École polytechnique (X)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Finnish Meteorological Institute (FMI), Department of Earth and Planetary Science [Tokyo], Graduate School of Science [Tokyo], The University of Tokyo (UTokyo)-The University of Tokyo (UTokyo), EISCAT Scientific Association [Sweden], Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), European Space Agency (ESA)-European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung (MPS), Institut für Weltraumforschung [Graz] (IWF), Consiglio Nazionale delle Ricerche [Roma] (CNR), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National d’Études Spatiales [Paris] (CNES), Universität Bern [Bern], University of Virginia [Charlottesville], The University of Tokyo (UTokyo), National Institute for Astrophysics, Southwest Research Institute, Austrian Academy of Sciences, Uppsala University, Agenzia Spaziale Italiana, Johns Hopkins Applied Physics Laboratory, NASA Goddard Space Flight Center, University of Michigan, Ann Arbor, UMR7095, IRAP, Department of Electronics and Nanoengineering, Space Technology Ireland, Hungarian Academy of Sciences, Space Research Institute of the Russian Academy of Sciences, National and Kapodistrian University of Athens, United States Department of Energy, European Space Research and Technology Centre, Max Planck Institute for Solar System Research, Osservatorio Astronomico di Trieste, AMDL Srl, University of Colorado Boulder, Slovak Academy of Sciences, National Research Council of Italy, INAF - Osservatorio Astronomico di Padova, Université d'Orléans, Comisión Nacional de Energía Atómica, Aberystwyth University, Université Paris-Saclay, Finnish Meteorological Institute, Tofwerk AG, The University of Tokyo, EISCAT Headquarters, Aalto-yliopisto, and Aalto University
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010504 meteorology & atmospheric sciences ,chemistry.chemical_element ,7. Clean energy ,01 natural sciences ,Article ,Astrobiology ,law.invention ,Particle instrumentation ,Mercury’s environment ,Orbiter ,Interplanetary dust cloud ,law ,0103 physical sciences ,Calibration ,BepiColombo space mission ,Neutral particle ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Spacecraft ,business.industry ,520 Astronomy ,Astronomy and Astrophysics ,620 Engineering ,Mercury (element) ,Solar wind ,Planetary science ,chemistry ,Space and Planetary Science ,[SDU]Sciences of the Universe [physics] ,Physics::Space Physics ,Environmental science ,Astrophysics::Earth and Planetary Astrophysics ,business - Abstract
The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase.
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- 2021
22. Assessment of aging state of bitumen based on peak-area evaluation in infrared spectroscopy: Influence of data processing and modeling
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M. Wieser, R. Traxl, S.H. Unterberger, and R. Lackner
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General Materials Science ,Building and Construction ,Civil and Structural Engineering - Published
- 2022
23. Sperm quality biomarkers complement reproductive and endocrine parameters in investigating environmental contaminants in common carp (Cyprinus carpio) from the Lake Mead National Recreation Area
- Author
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Constance A. Kersten, Steven L. Goodbred, Kathy R. Echols, Jill A. Jenkins, Carla M. Wieser, Rassa O. Draugelis-Dale, Michael R. Rosen, and Leticia Torres
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Male ,0301 basic medicine ,Carps ,Zoology ,010501 environmental sciences ,01 natural sciences ,Biochemistry ,Cyprinus ,Vitellogenins ,03 medical and health sciences ,chemistry.chemical_compound ,Vitellogenin ,Common carp ,Southwestern United States ,Animals ,Carp ,Sperm motility ,0105 earth and related environmental sciences ,General Environmental Science ,biology ,Hexachlorobenzene ,biology.organism_classification ,Spermatozoa ,Lakes ,Gonadosomatic Index ,030104 developmental biology ,chemistry ,Sperm Motility ,biology.protein ,Recreation ,Biomarkers ,Water Pollutants, Chemical ,Hormone - Abstract
Lake Mead National Recreational Area (LMNRA) serves as critical habitat for several federally listed species and supplies water for municipal, domestic, and agricultural use in the Southwestern U.S. Contaminant sources and concentrations vary among the sub-basins within LMNRA. To investigate whether exposure to environmental contaminants is associated with alterations in male common carp (Cyprinus carpio) gamete quality and endocrine- and reproductive parameters, data were collected among sub-basins over 7 years (1999–2006). Endpoints included sperm quality parameters of motility, viability, mitochondrial membrane potential, count, morphology, and DNA fragmentation; plasma components were vitellogenin (VTG), 17s-estradiol, 11-keto-testosterone, triiodothyronine, and thyroxine. Fish condition factor, gonadosomatic index, and gonadal histology parameters were also measured. Diminished biomarker effects were noted in 2006, and sub-basin differences were indicated by the irregular occurrences of contaminants and by several associations between chemicals (e.g., polychlorinated biphenyls, hexachlorobenzene, galaxolide, and methyl triclosan) and biomarkers (e.g., plasma thyroxine, sperm motility and DNA fragmentation). By 2006, sex steroid hormone and VTG levels decreased with subsequent reduced endocrine disrupting effects. The sperm quality bioassays developed and applied with carp complemented endocrine and reproductive data, and can be adapted for use with other species.
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- 2018
24. Energetic Neutral Atom Distribution on the Lunar Surface and Its Relationship with Solar Wind Conditions
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H. Z. Wang, C. Xiao, Q. Q. Shi, R. L. Guo, C. Yue, L. H. Xie, J. Zhang, A. B. Zhang, M. Wieser, Y. Saito, M. N. Nishino, M. Nowada, Q. G. Zong, A. W. Degeling, A. M. Tian, S. Y. Fu, H. Zhang, J. Chen, T. X. Zhang, J. Liu, C. Y. Han, W. S. Shang, and S. C. Bai
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Space and Planetary Science ,Astrophysics::High Energy Astrophysical Phenomena ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Astronomy and Astrophysics ,Astrophysics::Earth and Planetary Astrophysics - Abstract
The Advanced Small Analyzer for Neutrals (ASAN) on board the Chang’E-4 Yutu-2 rover first detected energetic neutral atoms (ENAs) originating from the lunar surface at various lunar local times on the lunar farside. In this work, we examine the ENA energy spectra, obtained in the first 23 lunar days from 2019 January 11 to 2020 October 12, and find a higher ENA differential flux on the lunar dawnside than on the duskside. Combined with Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon’s Interaction with the Sun (ARTEMIS) data, we analyze the correlation between the ENA differential flux and solar wind parameters, such as flux, density, dynamic pressure, and velocity, for each ASAN energy channel on the dawnside and duskside. The results show that ENA differential flux is positively correlated with solar wind flux, density, and dynamic pressure and relatively lower on the duskside than on the dawnside. To determine the relationship between solar wind energy and ENA energy, we analyze the correlation between solar wind energy and ENA cutoff energy and temperature on the dawnside and duskside. The results show that the ENA cutoff energy and temperature are lower on the duskside than on the dawnside at the same solar wind energy. The difference between the ENA–solar wind observation on the dawnside and duskside is possibly caused by solar wind deflection and deceleration on the duskside, which can be attributed to the interaction between solar wind and the lunar magnetic anomalies located nearby in the northwestern direction of the Chang’E-4 landing site.
- Published
- 2021
25. Surgical treatment of a rectovaginal fistula using the Martius Flap procedure (with video)
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M. Wieser, B. Romain, and D. Charleux-Muller
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medicine.medical_specialty ,Rectovaginal fistula ,business.industry ,medicine ,medicine.disease ,Surgical treatment ,business ,Surgery - Published
- 2021
26. Determination of cyclic volatile methylsiloxanes in personal care products by gas chromatography
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H. M. Brothers, T. Boehmer, R. A. Campbell, S. Dorn, J. J. Kerbleski, S. Lewis, C. Mund, D. Pero, K. Saito, M. Wieser, and W. Zoller
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Aging ,Chromatography, Gas ,Siloxanes ,Sample (material) ,Pharmaceutical Science ,Cosmetics ,Dermatology ,010501 environmental sciences ,Quechers ,01 natural sciences ,Colloid and Surface Chemistry ,Drug Discovery ,False positive paradox ,Process engineering ,Reliability (statistics) ,0105 earth and related environmental sciences ,Personal care ,Chromatography ,Chemistry ,business.industry ,010401 analytical chemistry ,Reproducibility of Results ,0104 chemical sciences ,Chemistry (miscellaneous) ,Gas chromatography ,Volatilization ,business - Abstract
Objective Organosiloxanes are prevalent in personal care products (PCPs) due to the desired properties they impart in the usage and application of such products. However, the European Chemical Agency (ECHA) has recently published restriction proposals on the amount of two cyclic siloxanes, octamethylcyclotetrasiloxane (D4) and decamethylcyclotetrasiloxane (D5) allowed in wash off products such as shampoos and conditioners which are discharged down the drain during consumer use. This legislation will require that reliable analytical methods are available for manufacturers and government agencies to use in documenting compliance with the restrictions. This paper proposes a simple analytical method to enable accurate measurement of these compounds down to the circa 0.1 weight percent level in PCPs. Methods While gas chromatography methods are reported in the literature for quantitation of D4 and D5 in several matrices including PCPs, the potential for generation of false positives due to contamination, co-elution, and in-situ generation of cyclic volatile methylsiloxanes (cVMS) is always present and needs to be controlled. This report demonstrates the applicability of using a combination of emulsion break, liquid-liquid extraction and silylation sample preparation followed by GC-FID analysis as a suitable means of analyzing PCPs for specific cVMS. Results The reliability and limitations of such methodology was demonstrated through several round robin studies conducted in the laboratories of a consortium of silicone manufacturers. In addition, this report presents examples of false positives encountered during development of the method and presents a comparative analysis between this method and a published QuEChERS sample preparation procedure to illustrate the potential for generation of false positives when an inappropriate approach is applied to determination of cVMS in personal care products. Conclusion This report demonstrates that an approach to determine cVMS levels in personal care products is to perform an emulsion break on the sample, isolate the nonpolar phase from the emulsion break and treat with a silylation reagent to abate potential in situ formation of cyclics during the course of GC-FID analysis. Round robin studies conducted in laboratories representing multiple siloxane manufacturers demonstrated the reliability of the GC-FID method when measuring cVMS in PCPs down to circa 0.1%. This article is protected by copyright. All rights reserved.
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- 2017
27. SAS-6 engineering reveals interdependence between cartwheel and microtubules in determining centriole architecture
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Michel O. Steinmetz, Pierre Gönczy, Virginie Hamel, Rolf Jaussi, Isabelle Flückiger, Masafumi Hirono, Sebastian H. W. Kraatz, Sarah Hosner, Daniel Frey, Katherine M. Thieltges, Xavier Deupi, Paul Guichard, Daniel J. Müller, Moritz Pfreundschuh, Akira Noga, Mara M. Wieser, Richard A. Kammerer, and Manuel Hilbert
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Models, Molecular ,0301 basic medicine ,Centriole ,Blotting, Western ,Green Fluorescent Proteins ,Mutant ,Molecular Conformation ,Chlamydomonas reinhardtii ,Cell Cycle Proteins ,Flagellum ,Crystallography, X-Ray ,Microscopy, Atomic Force ,medicine.disease_cause ,Microtubules ,03 medical and health sciences ,Microtubule ,Cell Line, Tumor ,medicine ,Humans ,Centrioles ,Mutation ,biology ,Cilium ,Algal Proteins ,Cell Biology ,biology.organism_classification ,Protein Structure, Tertiary ,Cell biology ,Microscopy, Electron ,030104 developmental biology ,Microscopy, Fluorescence ,Centrosome ,RNA Interference ,Protein Multimerization - Abstract
Centrioles are critical for the formation of centrosomes, cilia and flagella in eukaryotes. They are thought to assemble around a nine-fold symmetric cartwheel structure established by SAS-6 proteins. Here, we have engineered Chlamydomonas reinhardtii SAS-6-based oligomers with symmetries ranging from five- to ten-fold. Expression of a SAS-6 mutant that forms six-fold symmetric cartwheel structures in vitro resulted in cartwheels and centrioles with eight- or nine-fold symmetries in vivo. In combination with Bld10 mutants that weaken cartwheel-microtubule interactions, this SAS-6 mutant produced six- to eight-fold symmetric cartwheels. Concurrently, the microtubule wall maintained eight- and nine-fold symmetries. Expressing SAS-6 with analogous mutations in human cells resulted in nine-fold symmetric centrioles that exhibited impaired length and organization. Together, our data suggest that the self-assembly properties of SAS-6 instruct cartwheel symmetry, and lead us to propose a model in which the cartwheel and the microtubule wall assemble in an interdependent manner to establish the native architecture of centrioles.
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- 2016
28. Structure of the BoNT/A1 – receptor complex
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Mara M. Wieser, Richard A. Kammerer, Katherine M. Thieltges, Guido Capitani, Roger Benoit, Rolf Jaussi, and Daniel Frey
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Neurons ,Membrane Glycoproteins ,Molecular Structure ,Neuronal protein ,Biology ,Crystallography, X-Ray ,Toxicology ,medicine.disease ,Virology ,Botulinum neurotoxin ,Adenosine A1 receptor ,medicine ,Animals ,Humans ,Botulism ,Botulinum Toxins, Type A ,Neuroscience ,Protein Binding - Abstract
Botulinum neurotoxin A causes botulism but is also used for medical and cosmetic applications. A detailed molecular understanding of BoNT/A--host receptor interactions is therefore fundamental for improving current clinical applications and for developing new medical strategies targeting human disorders. Towards this end, we recently solved an X-ray crystal structure of BoNT/A1 in complex with its neuronal protein receptor SV2C. Based on our findings, we discuss the potential implications for BoNT/A function.
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- 2015
29. Software-type Wave-Particle Interaction Analyzer (S-WPIA) by RPWI for JUICE: Science objectives and implementation
- Author
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Hirotsugu Kojima, Tomoki Kimura, Hiroaki Misawa, Mitsuru Hikishima, Masafumi Shoji, Keigo Ishisaka, Satoshi Yagitani, Atsushi Kumamoto, W. Schmidt, Yoshizumi Miyoshi, Jan-Erik Wahlund, Yasumasa Kasaba, M. Kitahara, Tomohiko Imachi, Fuminori Tsuchiya, W. Puccio, Yoshiya Kasahara, M. Wieser, Kazushi Asamura, S. Barabash, Yuto Katoh, R. Gill, and Santolik, O., Bergman, J.
- Subjects
Jupiter ,Physics ,Spectrum analyzer ,Software ,Wave–particle duality ,business.industry ,Instrumentation (computer programming) ,Aerospace engineering ,business - Published
- 2018
30. PLATO: the ESA mission for exo-planets discovery
- Author
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Mario Salatti, Simonetta Chinellato, C. Catala, Willy Benz, Matteo Burresi, Enrico Battistelli, Steve Rockstein, Giordano Bruno, Matteo Munari, Giampaolo Piotto, Federico Biondi, M. Marinai, Maria Bergomi, Maximilian Klebor, Stefano Basso, Elisa Portaluri, Daniele Piazza, Martin Pertenais, Valerio Nascimbeni, T. Bandy, Riccardo Bardazzi, Anders Erikson, Emanuele Capuano, Anko Börner, Virginie Cessa, Simone Pirrotta, Andrea Novi, Mauro Ghigo, Isabella Pagano, Filippo Marliani, Marco Dima, Flavia Calderone, Daniela Sicilia, Juan Cabrera, Heike Rauer, Alexis Brandeker, Ana M. Heras, Mathias Brändli, M. Schweitzer, Roberto Ragazzoni, Davide Greggio, Valery Mogulsky, Martin Rieder, Luca Marafatto, Valentina Viotto, M. Wieser, Gisbert Peter, Thierry De Roche, E. Tommasi, Mauro Brotini, Demetrio Magrin, Gabriele Umbriaco, Jacopo Farinato, and Francesco Borsa
- Subjects
Cosmic Vision ,010504 meteorology & atmospheric sciences ,Aperture ,Field of view ,ESA medium size mission ,01 natural sciences ,Asteroseismology ,Transits ,law.invention ,Telescope ,law ,Planet ,0103 physical sciences ,Electronic ,Optical and Magnetic Materials ,ESA medium class mission ,Exoplanets ,PLATO ,Refractive design ,Electronic, Optical and Magnetic Materials ,Condensed Matter Physics ,Applied Mathematics ,Electrical and Electronic Engineering ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Physics ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Exoplanet ,Stars ,Astrophysics::Earth and Planetary Astrophysics - Abstract
PLATO (PLAnetary Transits and Oscillation of stars) is the ESA Medium size dedicated to exo-planets discovery, adopted in the framework of the Cosmic Vision program. The PLATO launch is planned in 2026 and the mission will last at least 4 years in the Lagrangian point L2. The primary scientific goal of PLATO is to discover and characterize a large amount of exo-planets hosted by bright nearby stars, constraining with unprecedented precision their radii by mean of transits technique and the age of the stars through by asteroseismology. By coupling the radius information with the mass knowledge, provided by a dedicated ground-based spectroscopy radial velocity measurements campaign, it would be possible to determine the planet density. Ultimately, PLATO will deliver the largest samples ever of well characterized exo-planets, discriminating among their ‘zoology’. The large amount of required b right stars can be achieved by a relatively small aperture telescope (about 1 meter class) with a wide Field of View (about 1000 square degrees). The PLATO strategy is to split the collecting area into 24 identical 120 mm aperture diameter fully refractive cameras with partially overlapped Field of View delivering an overall instantaneous sky covered area of about 2232square degrees. The opto-mechanical sub-system of each camera, namely Telescope Optical Unit, is basically composed by a 6 lenses fully refractive optical system, presenting one aspheric surface on the front lens, and by a mechanical structure made in AlBeMet.
- Published
- 2018
31. Crystal structure of the BoNT/A2 receptor-binding domain in complex with the luminal domain of its neuronal receptor SV2C
- Author
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Roger M. Benoit, Martin A. Schärer, Mara M. Wieser, Xiaodan Li, Daniel Frey, and Richard A. Kammerer
- Published
- 2017
- Full Text
- View/download PDF
32. Vor-Turbine-Katalysatoren in PKW-Dieselmotoren/Pre-Turbine-Catalysts for Passenger Car Diesel Engines
- Author
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G. Kellermayr, F. Jayat, H. Eichlseder, M. Bonifer, P. Rumplmayr, M. Wieser, and R. Ratzberger
- Published
- 2017
33. Dose matters! Optimisation of guideline adherence is associated with lower mortality in stable patients with chronic heart failure
- Author
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C Dornaus, Friedrich Fruhwald, Reiter S, Andreas Winter, D Keroe, A Boehmer, Hanno Ulmer, Richard Steinacher, Martin Huelsmann, Christian Ebner, K. Ablasser, Richard Pacher, V Eder, Gerhard Poelzl, M Wieser, G Jakl, Michael Ess, A Hallas, Johann Auer, Groebner H, Ehmsen U, Johann Altenberger, and L Pilgersdorfer
- Subjects
Male ,medicine.medical_specialty ,Nyha class ,Medication Adherence ,Internal medicine ,medicine ,Humans ,In patient ,Registries ,cardiovascular diseases ,Mortality ,Intensive care medicine ,Aged ,Heart Failure ,Ejection fraction ,business.industry ,Guideline adherence ,Australia ,Cardiovascular Agents ,Middle Aged ,medicine.disease ,Heart failure ,Censoring (clinical trials) ,Chronic Disease ,Ambulatory ,Female ,Guideline Adherence ,Cardiology and Cardiovascular Medicine ,business ,Lower mortality ,Follow-Up Studies - Abstract
Guidelines have been published for improving management of chronic heart failure (CHF). We examined the association between improved guideline adherence and risk for all-cause death in patients with stable systolic HF.Data on ambulatory patients (2006-2010) with CHF and reduced ejection fraction (HF-REF) from the Austrian Heart Failure Registry (HIR Austria) were analysed. One-year clinical data and long-term follow-up data until all-cause death or data censoring were available for 1014 patients (age 65 [55-73], male 75%, NYHA class I 14%, NYHA II 56%, NYHA III/IV 30%). A guideline adherence indicator (GAI [0-100%]) was calculated for each patient at baseline and after 12 ± 3 months that considered indications and contraindications for ACE-I/ARB, beta blockers, and MRA. Patients were considered ΔGAI-positive if GAI improved to or remained at high levels (≥ 80%). ΔGAI50+ positivity was ascribed to patients achieving a dose of ≥ 50% of suggested target dose.Improvements in GAI and GAI50+ were associated with significant improvements in NYHA class and NT-proBNP (1728 [740-3636] to 970 [405-2348]) (p0.001). Improvements in GAI50+, but not GAI, were independently predictive of lower mortality risk (HR 0.55 [95% CI 0.34-0.87; p=0.01]) after adjustment for a large variety of baseline parameters and hospitalisation for heart failure during follow-up.Improvement in guideline adherence with particular emphasis on dose escalation is associated with a decrease in long-term mortality in ambulatory HF-REF subjects surviving one year after registration.
- Published
- 2014
34. Novel compounds for therapy: antibiotics and alternative therapies
- Author
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Kimberly D.P. Hammer, Tze Shien Lo, Catherine M. Wieser, and Melissa A Rohrich
- Subjects
medicine.medical_specialty ,medicine.drug_class ,business.industry ,Antibiotics ,medicine ,Intensive care medicine ,business - Published
- 2014
35. Synthesis and Evaluation of Biphenyl Compounds as Kinesin Spindle Protein Inhibitors
- Author
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Richard A. Kammerer, Svetlana V. Selivanova, Selena Milicevic Sephton, Rolf Jaussi, Jason P. Holland, Mara M. Wieser, Albert Kang, Roger Schibli, Susan Cohrs, Daniel Frey, Eliane Fischer, and Thomas Betzel
- Subjects
Kinesins ,Cell Cycle Proteins ,Bioengineering ,Antimitotic Agents ,Biochemistry ,Structure-Activity Relationship ,Adenosine Triphosphate ,Cell Line, Tumor ,Humans ,Structure–activity relationship ,Enzyme Inhibitors ,Molecular Biology ,Mitosis ,Cell Proliferation ,Chemistry ,Biphenyl Compounds ,Thiourea ,General Chemistry ,General Medicine ,Cell sorting ,HCT116 Cells ,In vitro ,Biphenyl compound ,Cell culture ,MCF-7 Cells ,M Phase Cell Cycle Checkpoints ,Molecular Medicine ,Kinesin ,Antimitotic Agent - Abstract
Kinesin spindle protein (KSP), an ATP-dependent motor protein, plays an essential role in bipolar spindle formation during the mitotic phase (M phase) of the normal cell cycle. KSP has emerged as a novel target for antimitotic anticancer drug development. In this work, we synthesized a range of new biphenyl compounds and investigated their properties in vitro as potential antimitotic agents targeting KSP expression. Antiproliferation (MTT (=3-(4,5-dimethylthiazol-2-yl)-2,5-diphenyl-2H-tetrazolium bromide)) assays, combined with fluorescence-assisted cell sorting (FACS) and Western blot studies analyzing cell-cycle arrest confirmed the mechanism and potency of these biphenyl compounds in a range of human cancer cell lines. Structural variants revealed that functionalization of biphenyl compounds with bulky aliphatic or aromatic groups led to a loss of activity. However, replacement of the urea group with a thiourea led to an increase in antiproliferative activity in selected cell lines. Further studies using confocal fluorescence microscopy confirmed that the most potent biphenyl derivative identified thus far, compound 7, exerts its pharmacologic effect specifically in the M phase and induces monoaster formation. These studies confirm that chemical scope remains for improving the potency and treatment efficacy of antimitotic KSP inhibition in this class of biphenyl compounds.
- Published
- 2013
36. Structural basis of tubulin tyrosination by tubulin tyrosine ligase
- Author
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Maria M. Magiera, Richard A. Kammerer, Marijn Kuijpers, Katja Bargsten, Carsten Janke, Mara M. Wieser, Rolf Jaussi, Casper C. Hoogenraad, Daniel Frey, Andrea E. Prota, and Michel O. Steinmetz
- Subjects
Models, Molecular ,Tubulin—tyrosine ligase ,Dimer ,Sus scrofa ,macromolecular substances ,Hippocampus ,Models, Biological ,Article ,Structure-Activity Relationship ,03 medical and health sciences ,chemistry.chemical_compound ,0302 clinical medicine ,Protein structure ,Tubulin ,Animals ,Structure–activity relationship ,Peptide Synthases ,Tyrosine ,Research Articles ,030304 developmental biology ,Neurons ,chemistry.chemical_classification ,0303 health sciences ,biology ,Cell Biology ,Cell cycle ,Protein Structure, Tertiary ,Rats ,Enzyme ,Biochemistry ,chemistry ,biology.protein ,Cattle ,Chickens ,030217 neurology & neurosurgery - Abstract
Structural analysis of a complex of tubulin and tubulin tyrosine ligase (TTL) reveals insights into TTL’s enzymatic mechanism, how it discriminates between α- and β-tubulin, and its possible evolutionary origin., Tubulin tyrosine ligase (TTL) catalyzes the post-translational retyrosination of detyrosinated α-tubulin. Despite the indispensable role of TTL in cell and organism development, its molecular mechanism of action is poorly understood. By solving crystal structures of TTL in complex with tubulin, we here demonstrate that TTL binds to the α and β subunits of tubulin and recognizes the curved conformation of the dimer. Biochemical and cellular assays revealed that specific tubulin dimer recognition controls the activity of the enzyme, and as a consequence, neuronal development. The TTL–tubulin structure further illustrates how the enzyme binds the functionally crucial C-terminal tail sequence of α-tubulin and how this interaction catalyzes the tyrosination reaction. It also reveals how TTL discriminates between α- and β-tubulin, and between different post-translationally modified forms of α-tubulin. Together, our data suggest that TTL has specifically evolved to recognize and modify tubulin, thus highlighting a fundamental role of the evolutionary conserved tubulin tyrosination cycle in regulating the microtubule cytoskeleton.
- Published
- 2013
- Full Text
- View/download PDF
37. Implementation and Outcome Assessment of an Inpatient Antimicrobial Stewardship Program
- Author
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Catherine M. Wieser, Brandie L. Hagert, Tze Shien Lo, William P. Newman, Melissa Rohrich, Ji M. Koo, and Cristin Williams
- Subjects
Pharmacology ,medicine.medical_specialty ,business.industry ,Psychological intervention ,Retrospective cohort study ,Pharmacy ,Outcome assessment ,Antimicrobial ,Antibiotic resistance ,Health care ,Emergency medicine ,medicine ,Antimicrobial stewardship ,Pharmacology (medical) ,business ,Intensive care medicine ,Veterans Affairs - Abstract
Background An antimicrobial stewardship program (ASP), aiming to optimize antimicrobial usage, was implemented at a Veterans Affairs Health Care System (VA HCS). Objective The main objective of this study was to compare antimicrobial usage before and after implementation of an ASP and to assess ASP interventions. Method This retrospective study was conducted at the Fargo VA HCS. A total of 1,017 inpatient charts were reviewed for 2 distinct time periods, February through September 2008 (pre ASP) and February through September 2010 (post ASP). The data that were collected and analyzed included the number of hospitalized patients prescribed antimicrobials, antimicrobial therapy duration, duration of hospital stay, and inpatient antimicrobial costs. Subgroup analyses were performed on the top 5 antimicrobials and the top 6 indications. The number, types of, and overall acceptance rate of ASP interventions were also assessed. Results When the pre- to post-ASP periods were compared, the percentage of patients on antimicrobial therapy decreased from 36.8% to 25% ( P < .001), the median duration of antimicrobial therapy significantly decreased ( P = .02), and the defined daily dose (DDD) per 1,000 patient bed days was reduced for piperacillin/tazobactam, vancomycin, and ciprofloxacin. In addition, the total inpatient antimicrobial costs decreased by $48,044 (25%). The overall ASP intervention acceptance rate was 81.6% (315 out of 386 total interventions). Conclusion The results of this study show that ASP implementation has been highly accepted by providers and has been associated with a reduction in the number of patients prescribed antimicrobials, median duration of antimicrobial therapy, and antimicrobial inpatient costs.
- Published
- 2012
38. Crystal structure of the BoNT/A2 receptor-binding domain in complex with the luminal domain of its neuronal receptor SV2C
- Author
-
Roger M, Benoit, Martin A, Schärer, Mara M, Wieser, Xiaodan, Li, Daniel, Frey, and Richard A, Kammerer
- Subjects
Models, Molecular ,Binding Sites ,Membrane Glycoproteins ,Protein Conformation ,Amino Acid Motifs ,Humans ,Nerve Tissue Proteins ,Protein Interaction Domains and Motifs ,Amino Acid Sequence ,Botulinum Toxins, Type A ,Article ,Protein Binding - Abstract
A detailed molecular understanding of botulinum neurotoxin (BoNT)/host-cell-receptor interactions is fundamental both for developing strategies against botulism and for generating improved BoNT variants for medical applications. The X-ray crystal structure of the receptor-binding domain (HC) of BoNT/A1 in complex with the luminal domain (LD) of its neuronal receptor SV2C revealed only few specific side-chain – side-chain interactions that are important for binding. Notably, two BoNT/A1 residues, Arg 1156 and Arg 1294, that are crucial for the interaction with SV2, are not conserved among subtypes. Because it has been suggested that differential receptor binding of subtypes might explain their differences in biological activity, we determined the crystal structure of BoNT/A2-HC in complex with SV2C-LD. Although only few side-chain interactions are conserved between the two BoNT/A subtypes, the overall binding mode of subtypes A1 and A2 is virtually identical. In the BoNT/A2-HC – SV2C complex structure, a missing cation-π stacking is compensated for by an additional salt bridge and an anion-π stacking interaction, which explains why the binding of BoNT/A subtypes to SV2C tolerates variable side chains. These findings suggest that motif extensions and a shallow binding cleft in BoNT/A-HC contribute to binding specificity.
- Published
- 2016
39. Thermal effects on PLATO point spread function
- Author
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Demetrio Magrin, Simonetta Chinellato, Giordano Bruno, Isabella Pagano, M. Schweitzer, Roberto Ragazzoni, Marco Gullieuszik, Davide Greggio, Alexis Brandeker, Luca Marafatto, Valerio Nascimbeni, Daniele Spiga, Daniela Sicilia, Mathias Brändli, Mauro Ghigo, Valery Mogulsky, Daniele Piazza, Matteo Munari, Maximilian Klebor, Stefano Basso, Maria Bergomi, Marco Dima, Anders Erikson, Federico Biondi, Willy Benz, Martin Rieder, Heike Rauer, M. Wieser, Thierry De Roche, Valentina Viotto, Thimoty Bandy, Francesco Borsa, and Jacopo Farinato
- Subjects
Point spread function ,Extrasolare Planeten und Atmosphären ,Field of view ,01 natural sciences ,Instrumentation: photometers ,law.invention ,Telescope ,Photometry (optics) ,Optics ,Photometric calibration ,law ,0103 physical sciences ,Thermal ,Electronic ,Optical and Magnetic Materials ,Electrical and Electronic Engineering ,010303 astronomy & astrophysics ,planetary systems ,Physics ,Planetary systems ,Telescopes ,Electronic, Optical and Magnetic Materials ,Condensed Matter Physics ,Computer Science Applications ,Computer Vision and Pattern Recognition ,Applied Mathematics ,010308 nuclear & particles physics ,business.industry ,Astrophysics::Instrumentation and Methods for Astrophysics ,Centroid ,Physics::History of Physics ,Exoplanet ,Telescopes ,Astrophysics::Earth and Planetary Astrophysics ,business - Abstract
Thermal effects in PLATO are analyzed in terms of uniform temperature variations, longitudinal and lateral temperature gradients. We characterize these effects by evaluating the PSF centroid shifts and the Enclosed Energy variations across the whole FoV. These patterns can then be used to gauge the thermal behavior of each individual telescope in order to improve the local photometric calibration across the PLATO field of view.
- Published
- 2016
40. PLATO: a multiple telescope spacecraft for exo-planets hunting
- Author
-
M. Wieser, Simonetta Chinellato, Gisbert Peter, Valentina Viotto, Daniela Sicilia, Demetrio Magrin, Giordano Bruno, P. Bodin, Martin Rieder, T. Bandy, Valerio Nascimbeni, Luca Marafatto, Maximilian Klebor, Stefano Basso, Anko Boerner, Ana M. Heras, Isabella Pagano, Mauro Ghigo, M. Schweitzer, C. Catala, Roberto Ragazzoni, Matteo Munari, Francesco Borsa, Federico Biondi, Jacopo Farinato, Daniele Spiga, Maria Bergomi, Anders Erikson, Patrick Levacher, Heike Rauer, Willy Benz, Marco Dima, Marco Gullieuszik, Thierry De Roche, Daniele Piazza, Valery Mogulsky, Juan Cabrera, Alexis Brandeker, Davide Greggio, Philippe Gondoin, Mathias Brändli, Giampaolo Piotto, and ITA
- Subjects
Extrasolare Planeten und Atmosphären ,Cosmic Vision ,Lagrangian point ,extra-solar planetary system ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Asteroseismology ,law.invention ,010309 optics ,Telescope ,law ,Planet ,Space telescope ,0103 physical sciences ,Electronic ,Astrophysics::Solar and Stellar Astrophysics ,Optical and Magnetic Materials ,Electrical and Electronic Engineering ,010303 astronomy & astrophysics ,Physics ,Applied Mathematics ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Extra-solar planetary system ,Space telescope ,Electronic, Optical and Magnetic Materials ,Condensed Matter Physics ,Exoplanet ,Radial velocity ,Stars ,Astrophysics::Earth and Planetary Astrophysics - Abstract
PLATO stands for PLAnetary Transits and Oscillation of stars and is a Medium sized mission selected as M3 by the European Space Agency as part of the Cosmic Vision program. The strategy behind is to scrutinize a large fraction of the sky collecting lightcurves of a large number of stars and detecting transits of exo-planets whose apparent orbit allow for the transit to be visible from the Earth. Furthermore, as the transit is basically able to provide the ratio of the size of the transiting planet to the host star, the latter is being characterized by asteroseismology, allowing to provide accurate masses, radii and hence density of a large sample of extra solar bodies. In order to be able to then follow up from the ground via spectroscopy radial velocity measurements these candidates the search must be confined to rather bright stars. To comply with the statistical rate of the occurrence of such transits around these kind of stars one needs a telescope with a moderate aperture of the order of one meter but with a Field of View that is of the order of 50 degrees in diameter. This is achieved by splitting the optical aperture into a few dozens identical telescopes with partially overlapping Field of View to build up a mixed ensemble of differently covered area of the sky to comply with various classes of magnitude stars. The single telescopes are refractive optical systems with an internally located pupil defined by a CaF2 lens, and comprising an aspheric front lens and a strong field flattener optical element close to the detectors mosaic. In order to continuously monitor for a few years with the aim to detect planetary transits similar to an hypothetical twin of the Earth, with the same revolution period, the spacecraft is going to be operated while orbiting around the L2 Lagrangian point of the Earth-Sun system so that the Earth disk is no longer a constraints potentially interfering with such a wide field continuous uninterrupted survey.
- Published
- 2016
41. Radiation, Thermal Gradient and Weight: a threefold dilemma for PLATO
- Author
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Heike Rauer, Marco Gullieuszik, Simonetta Chinellato, Francesco Borsa, Giordano Bruno, Mathias Brändli, Martin Rieder, Luca Marafatto, Daniele Piazza, Matteo Munari, Jacopo Farinato, Willy Benz, Anders Erikson, Maximilian Klebor, Stefano Basso, M. Wieser, Alexis Brandeker, Demetrio Magrin, Valentina Viotto, Valery Mogulsky, M. Schweitzer, Roberto Ragazzoni, Thierry De Roche, Maria Bergomi, Mauro Ghigo, T. Bandy, Daniela Sicilia, Marco Dima, Federico Biondi, Daniele Spiga, Isabella Pagano, Davide Greggio, and ITA
- Subjects
Extrasolare Planeten und Atmosphären ,Cosmic Vision ,extra-solar planetary system ,01 natural sciences ,law.invention ,010309 optics ,Telescope ,Optics ,Spitzer Space Telescope ,law ,0103 physical sciences ,Electronic ,asteroseismology ,Optical and Magnetic Materials ,Electrical and Electronic Engineering ,010303 astronomy & astrophysics ,Physics ,Asteroseismology ,Extra-solar planetary system ,Radiation ,Space telescope ,Thermal gradient ,Wide field camera ,Electronic, Optical and Magnetic Materials ,Condensed Matter Physics ,Applied Mathematics ,business.industry ,Payload ,Astrophysics::Instrumentation and Methods for Astrophysics ,Window (computing) ,Planetary system ,radiation ,Temperature gradient ,Astrophysics::Earth and Planetary Astrophysics ,pace telescope ,thermal gradient ,wide field camera ,business ,Space environment - Abstract
The project PLAnetary Transits and Oscillations of stars (PLATO) is one of the selected medium class (M class) missions in the framework of the ESA Cosmic Vision 2015-2025 program. The mean scientific goal of PLATO is the discovery and study of extrasolar planetary systems by means of planetary transits detection. The opto mechanical subsystem of the payload is made of 32 normal telescope optical units (N-TOUs) and 2 fast telescope optical units (FTOUs). The optical configuration of each TOU is an all refractive design based on six properly optimized lenses. In the current baseline, in front of each TOU a Suprasil window is foreseen. The main purposes of the entrance window are to shield the following lenses from possible damaging high energy radiation and to mitigate the thermal gradient that the first optical element will experience during the launch from ground to space environment. In contrast, the presence of the window increases the overall mass by a non-negligible quantity. We describe here the radiation and thermal analysis and their impact on the quality and risks assessment, summarizing the trade-off process with pro and cons on having or dropping the entrance window in the optical train.
- Published
- 2016
42. Manufacturing and alignment tolerance analysis through Montecarlo approach for PLATO
- Author
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Jacopo Farinato, Daniele Spiga, Simonetta Chinellato, Willy Benz, Marco Gullieuszik, Marco Dima, Federico Biondi, Heike Rauer, Mauro Ghigo, Alexis Brandeker, Daniela Sicilia, Luca Marafatto, T. Bandy, Isabella Pagano, M. Schweitzer, Roberto Ragazzoni, Daniele Piazza, Giordano Bruno, Maximilian Klebor, Stefano Basso, Matteo Munari, Anders Erikson, Mathias Brändli, Maria Bergomi, Valery Mogulsky, Davide Greggio, Martin Rieder, Thierry De Roche, Valentina Viotto, M. Wieser, Demetrio Magrin, Francesco Borsa, and ITA
- Subjects
Extrasolare Planeten und Atmosphären ,Depth of focus ,Cosmic Vision ,Tolerance analysis ,Field of view ,extra-solar planetary system ,asteroseismology ,01 natural sciences ,010309 optics ,Optics ,Spitzer Space Telescope ,Asteroseismology ,Extra-solar planetary system ,Space telescope ,Wide field camera ,Electronic, Optical and Magnetic Materials ,Condensed Matter Physics ,Applied Mathematics ,Electrical and Electronic Engineering ,0103 physical sciences ,Electronic ,Optical and Magnetic Materials ,Aerospace engineering ,010303 astronomy & astrophysics ,Physics ,Pixel ,business.industry ,Payload ,tolerance analysis ,Astrophysics::Instrumentation and Methods for Astrophysics ,Planetary system ,Astrophysics::Earth and Planetary Astrophysics ,wide field camera ,business - Abstract
The project PLAnetary Transits and Oscillations of stars (PLATO) is one of the selected medium class (M class) missions in the framework of the ESA Cosmic Vision 2015-2025 program. The main scientific goal of PLATO is the discovery and study of extrasolar planetary systems by means of planetary transits detection. According to the current baseline, the scientific payload consists of 34 all refractive telescopes having small aperture (120mm) and wide field of view (diameter greater than 37 degrees) observing over 0.5-1 micron wavelength band. The telescopes are mounted on a common optical bench and are divided in four families of eight telescopes with an overlapping line-of-sight in order to maximize the science return. Remaining two telescopes will be dedicated to support on-board star-tracking system and will be specialized on two different photometric bands for science purposes. The performance requirement, adopted as merit function during the analysis, is specified as 90% enclosed energy contained in a square having size 2 pixels over the whole field of view with a depth of focus of +/-20 micron. Given the complexity of the system, we have followed a Montecarlo analysis approach for manufacturing and alignment tolerances. We will describe here the tolerance method and the preliminary results, speculating on the assumed risks and expected performances.
- Published
- 2016
43. Arthroskopie des Ellenbogengelenks in der Unfallchirurgie
- Author
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Sven Yves Vetter, C. Frank, M. Wieser, S. Englert, and Paul-Alfred Grützner
- Subjects
Public Health, Environmental and Occupational Health ,Emergency Medicine - Abstract
Die Arthroskopie des Ellenbogengelenkes gewinnt zunehmend an Bedeutung. Eine umfassende Untersuchung und praoperative Diagnostik sind fur eine korrekte Indikationsstellung entscheidend. Neben den haufigen Eingriffen an Gelenkhaut und Knorpel konnen bei zunehmender Expertise auch Instabilitaten sowie Bewegungseinschrankungen arthroskopisch therapiert werden. Eine Ausweitung der Indikationsstellung auf die Frakturversorgung des Ellenbogengelenkes stellt aktuell noch eine Ausnahme dar.
- Published
- 2011
44. Schulterarthroskopie
- Author
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Paul Alfred Grützner, M. Münzberg, M. Wieser, and S. Studier-Fischer
- Subjects
Public Health, Environmental and Occupational Health ,Emergency Medicine - Abstract
In den letzten Jahren gewannen die diagnostische und die operative Arthroskopie der Schulter zunehmend an Bedeutung. Die Arthroskopie ergibt im Vergleich zu anderen Diagnostikverfahren die zuverlassigsten und meisten Informationen bei Schultergelenklasionen. Vor allem die arthroskopische Versorgung von Weichteilverletzungen drangte die offenen Verfahren immer mehr in den Hintergrund. Labrumlasionen nach traumatischen Schulterluxationen, Lasionen der langen Bizepssehne, Rotatorenmanschettenlasionen und das subakromiale Impingementsyndrom sind Indikationen fur arthroskopische Operationsverfahren. Durch die Weiterentwicklung von Instrumenten und speziellen Ankersystemen werden die Operationstechniken immer effektiver und schneller und somit letztlich auch sicherer fur den Patienten.
- Published
- 2011
45. Effects of vegetation and fertilizer on metal and Sb plant uptake in a calcareous shooting range soil
- Author
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Héctor M. Conesa, Björn Studer, Rainer Schulin, and M. Wieser
- Subjects
Environmental Engineering ,biology ,Chemistry ,Extraction (chemistry) ,Management, Monitoring, Policy and Law ,engineering.material ,biology.organism_classification ,Lolium perenne ,Metal ,Agronomy ,visual_art ,Environmental chemistry ,Shoot ,Soil water ,Dissolved organic carbon ,engineering ,visual_art.visual_art_medium ,Fertilizer ,Calcareous ,Nature and Landscape Conservation - Abstract
Shooting range soils frequently contain anomalous concentrations of metals (e.g. Pb, Zn, Mn) and Sb coming from bullets which may be released into the environment. In a pot experiment, we investigated metal and Sb uptake by three plant species (Plantago lanceolata, Lolium perenne and Triticum aestivum) growing on a calcareous shooting range soil (pH 7.8; 500 mg kg−1 Pb, 21 mg kg−1 Sb) and the uptake changes when an acidic fertilizer solution was applied to the soil. Metal and Sb solubility in the soil was determined by extraction with 0.1 M NaNO3. In addition, we measured pH, electrical conductivity and dissolved organic carbon in drainage samples. The results showed significant increase over time of pH (from 7.8 to 8.3) and decrease of electrical conductivity and dissolved organic carbon (from 230 to ∼130 mg L−1). Fertilizer application increased NaNO3-extractable Pb and Sb and root:shoot biomass ratio but not plant metal uptake. In T. aestivum spikes accumulated more Zn, Ni and Cu than shoots and grains. Mn and Zb uptake was correlated in L. perenne shoots. P. lanceolata, a Sb-bioindicator, did not accumulate high amounts of Sb (
- Published
- 2011
46. Effects of three amendments on extractability and fractionation of Pb, Cu, Ni and Sb in two shooting range soils
- Author
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Björn Studer, M. Gasser, Michael W.H. Evangelou, M. Wieser, Kerstin Hockmann, Rainer Schulin, and Héctor M. Conesa
- Subjects
Antimony ,Total organic carbon ,Firearms ,Environmental Engineering ,Chemistry ,Health, Toxicology and Mutagenesis ,Soil classification ,Fractionation ,Chemical Fractionation ,Pollution ,Soil contamination ,Soil conditioner ,Lead ,Nickel ,Metals, Heavy ,Environmental chemistry ,Soil water ,Soil Pollutants ,Environmental Chemistry ,Leaching (agriculture) ,Waste Management and Disposal ,Calcareous ,Copper - Abstract
Contamination of shooting range soils with toxic trace elements, in particular Pb and Sb, is of increasing environmental concern worldwide. We studied the extractability of Sb, and other metals in two shooting range soils: a calcareous soil (pH 8) with low organic carbon (0.5%) and a non-calcareous soil (pH 6.3) with elevated organic carbon content (5%). Both soils contained total concentrations of around 500 mg kg(-1) Pb, 65 mg kg(-1) Cu, 100 mg kg(-1) Zn and 20 mg kg(-1) Sb. We tested the effects of Ca(OH)(2), phosphate and sodium humate amendments on metals and Sb extractability. Extracts with H(2)O and NaNO(3) contained 0.02-0.05% of the total Zn and Pb; 0.1-0.5% of total Ni and Cu and approximately 1% of total Sb. Sequential extraction procedure of Zeien and Brümmer resulted in similar percentages for the sum of the two most labile fractions (F1+F2) in two soils: 10% Pb, and 15-20% Sb. Water and NaNO(3)-extractable Sb concentrations increased after phosphate addition, but were not affected by the addition of sodium humate. The results show that leaching of Sb from shooting ranges into ground and surface waters may generate a serious environmental risk under widely different soils conditions.
- Published
- 2010
47. S3-Leitlinie 'Kolorektales Karzinom' – Aktualisierung 2008
- Author
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Christian Pox, Hans-Joachim Schmoll, W. Schmitt, Ullrich Graeven, Volker Heinemann, Rainer Porschen, Thomas Seufferlein, Dirk Arnold, Wolff Schmiegel, Anke Reinacher-Schick, I. Kopp, J. Riemann, M. Wieser, Claus Rödel, and Rolf Sauer
- Subjects
medicine.medical_specialty ,medicine.diagnostic_test ,business.industry ,Colorectal cancer ,General surgery ,Gastroenterology ,MEDLINE ,Salvage therapy ,Sigmoidoscopy ,Evidence-based medicine ,Guideline ,medicine.disease ,Text mining ,Medicine ,Combined Modality Therapy ,business - Published
- 2008
48. Chemical contaminants, health indicators, and reproductive biomarker responses in fish from rivers in the Southeastern United States
- Author
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Carla M. Wieser, Mark R. Ellersieck, Robert W. Gale, Vicki S. Blazer, Nancy D. Denslow, James J. Coyle, Jo Ellen Hinck, Donald E. Tillitt, Thomas W. May, and Kathy R. Echols
- Subjects
Male ,Carps ,Environmental Engineering ,food.ingredient ,Zoology ,Micropterus ,Dioxins ,Fish Diseases ,Selenium ,Vitellogenins ,Bass (fish) ,chemistry.chemical_compound ,Common carp ,Dieldrin ,food ,Rivers ,Metals, Heavy ,Cytochrome P-450 CYP1A1 ,Hydrocarbons, Chlorinated ,Animals ,Environmental Chemistry ,Testosterone ,Pesticides ,Gonads ,Carp ,Waste Management and Disposal ,Estradiol ,biology ,Ecology ,Methoxychlor ,Hexachlorobenzene ,biology.organism_classification ,Lipids ,Pollution ,Southeastern United States ,chemistry ,Endrin ,Bass ,Female ,Water Pollutants, Chemical - Abstract
Largemouth bass (Micropterus salmoides) and common carp (Cyprinus carpio) were collected from 13 sites located in the Mobile (MRB), Apalachicola–Flint–Chattahoochee (ARB), Savannah (SRB), and Pee Dee (PRB) River Basins to document spatial trends in accumulative chemical contaminants, health indicators, and reproductive biomarkers. Organochlorine residues, 2,3,7,8-tetrachlorodibenzo-p-dioxin-like activity (TCDD-EQ), and elemental contaminants were measured in composite samples of whole fish, grouped by species and gender, from each site. Mercury (Hg) and polychlorinated biphenyls (PCBs) were the primary contaminants of concern. Concentrations of Hg in bass samples from all basins exceeded toxicity thresholds for piscivorous mammals (> 0.1 μg/g ww), juvenile and adult fish (> 0.2 μg/g ww), and piscivorous birds (> 0.3 μg/g ww). Total PCB concentrations in samples from the MRB, ARB, and PRB were > 480 ng/g ww and may be a risk to piscivorous wildlife. Selenium concentrations also exceeded toxicity thresholds (> 0.75 μg/g ww) in MRB and ARB fish. Concentrations of other formerly used (total chlordanes, dieldrin, endrin, aldrin, mirex, and hexachlorobenzene) and currently used (pentachlorobenzene, pentachloroanisole, dacthal, endosulfan, γ-hexachlorocyclohexane, and methoxychlor) organochlorine residues were generally low or did not exceed toxicity thresholds for fish and piscivorous wildlife. TCDD-EQs exceeded wildlife dietary guidelines (> 5 pg/g ww) in MRB and PRB fish. Hepatic ethoxyresorufin O-deethylase (EROD) activity was generally greatest in MRB bass and carp. Altered fish health indicators and reproductive biomarker were noted in individual fish, but mean responses were similar among basins. The field necropsy and histopathological examination determined that MRB fish were generally in poorer health than those from the other basins, primarily due to parasitic infestations. Tumors were found in few fish (n = 5; 0.01%); ovarian tumors of smooth muscle origin were found in two ARB carp from the same site. Intersex gonads were identified in 47 male bass (42%) representing 12 sites and may indicate exposure to potential endocrine disrupting compounds. Comparatively high vitellogenin concentrations (> 0.35 mg/mL) in male fish from the MRB, SRB, and PRB indicate exposure to estrogenic or anti-androgenic chemicals.
- Published
- 2008
49. Reproductive and biochemical biomarkers in largemouth bass sampled downstream of a pulp and paper mill in Florida
- Author
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Maria S. Sepúlveda, Timothy S. Gross, Evan P. Gallagher, and Carla M. Wieser
- Subjects
Male ,Paper ,Health, Toxicology and Mutagenesis ,Industrial Waste ,Zoology ,Vitellogenins ,Vitellogenin ,Cytochrome P-450 CYP1A1 ,Animals ,Ecotoxicology ,Gonadal Steroid Hormones ,Gonads ,Centrarchidae ,Reproductive success ,biology ,business.industry ,Ecology ,Public Health, Environmental and Occupational Health ,Paper mill ,General Medicine ,Biochemical biomarkers ,biology.organism_classification ,Pollution ,Gonadosomatic Index ,Florida ,biology.protein ,Bass ,Female ,sense organs ,business ,Biomarkers ,Water Pollutants, Chemical ,Florida largemouth bass ,Environmental Monitoring - Abstract
The objective of this study was to evaluate the effects of bleached/unbleached kraft mill effluents (B/UKME) on the reproductive parameters of free-ranging Florida largemouth bass (Micropterus salmoides floridanus). The reproductive parameters measured included gonadosomatic index (GSI), histological evaluation of gonads, and plasma concentrations of vitellogenin (VTG), 17beta-estradiol, and 11-ketotestosterone (11-KT). Hepatic ethoxyresorufin-O-deethylase (EROD) activity was measured as a marker of exposure to cytochrome P450-inducing agents in these effluents. Endpoints were compared among adult bass sampled from tributary and mainstream effluent-contaminated and reference sites. Females sampled from the site closest to the mill outfall had a significant five-fold increase in EROD activity compared to bass sampled from reference streams. Although sex hormones were significantly reduced in bass from exposed sites, there were no differences in VTG and GSI across sites. The absence of organism-level responses was probably not related to a lack of sensitivity, as previous studies in our laboratory have shown that bass exposed to these effluents exhibit changes in GSI and in other measures associated with reproductive success. In females, inverse relationships were observed between VTG and GSI and EROD activity. These relationship, however, were not consistent within all of the sites studied. Collectively, our findings indicate that hepatic EROD induction is an effective marker of B/UKME exposure in largemouth bass and that it might be associated with antiestrogenic effects in this species.
- Published
- 2004
50. A EUROPEAN GLOBAL NAVIGATION SATELLITE SYSTEM — THE GERMAN MARKET AND VALUE ADDING CHAIN EFFECTS
- Author
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A. Vollerthun and M. Wieser
- Subjects
Finance ,Factor market ,Engineering ,Market research ,Market segmentation ,business.industry ,Forecast period ,Market share analysis ,Aerospace Engineering ,Satellite navigation ,Market share ,business ,Domestic market - Abstract
Since Europe is considering to establish a “market-driven” European Global Navigation Satellite System, the German Center of Aerospace initiated a market research to justify a German investment in such a European project. The market research performed included the following market segments: aviation, railway, road traffic, shipping, surveying, farming, military, space applications, leisure, and sport. In these market segments, the forementioned inputs were determined for satellite navigation hardware (receivers) as well as satellite navigation services. The forecast period was from year 2007 to 2017. For the considered period, the market amounts to a total of DM 83.0 billion (approx. US $50 billion), whereas the satellite navigation equipment market makes up DM 39.8 billion, and charges for value-added-services amount to DM 43.2 billion. On closer examination road traffic can be identified as the dominant market share, both in the receiver-market and service-market. With a share of 96% for receivers and 73% for services the significance of the road traffic segment becomes obvious. The second part of this paper investigates the effects the market potential has on the Value-Adding-Chain. Therefore, all participants in the Value-Adding-Chain are identified, using industrial cost structure models the employment effect is analyzed, and possible tax revenues for the state are examined.
- Published
- 2002
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