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  • 401.
    Winchen, T.
    et al.
    Vrije Universiteit Brussel, Belgium.
    Bonardi, A.
    Radboud University, The Netherlands.
    Buitink, S.
    Vrije Universiteit Brussel, Belgium.
    Corstanje, A.
    Radboud University, The Netherlands.
    Falcke, H.
    Radboud University, The Netherlands;Science Park Amsterdam, The Netherlands;Netherlands Institute of Radio Astronomy (ASTRON), The Netherlands.
    Hare, B. M.
    University Groningen, Germany.
    Hörandel, J. R.
    Radboud University, The Netherlands;NIKHEF, Science Park Amsterdam, The Netherlands.
    Mitra, P.
    Vrije Universiteit Brussel, Belgium.
    Mulrey, K.
    Vrije Universiteit Brussel, Belgium.
    Nelles, A.
    Humboldt-Universität zu Berlin, Germany.
    Rachen, J. P.
    Radboud University, The Netherlands.
    Rossetto, L.
    Radboud University, The Netherlands.
    Schellart, P.
    Radboud University, The Netherlands;Princeton University, Princeton, USA.
    Scholten, O.
    University Groningen, Germany;Vrije Universiteit Brussel, Belgium.
    Ter Veen, S.
    Radboud University, The Netherlands; Netherlands Institute of Radio Astronomy (ASTRON), The Netherlands.
    Thoudam, Satyendra
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering. Radboud University, The Netherlands.
    Trinh, T. N. G.
    University Groningen, Germany.
    Status of the lunar detection mode for cosmic particles of LOFAR2019In: Journal of Physics: Conference Series, Institute of Physics (IOP), 2019, no 1, article id 012077Conference paper (Refereed)
    Abstract [en]

    Cosmic particles hitting Earth's moon produce radio emission via the Askaryan effect. If the resulting radio ns-pulse can be detected by radio telescopes, this technique potentially increases the available collective area for ZeV scale particles by several orders of magnitude compared to current experiments. The LOw Frequency ARray (LOFAR) is the largest radio telescope operating in the optimum frequency regime for this technique. In this contribution, we report on the status of the implementation of the lunar detection mode at LOFAR. © Published under licence by IOP Publishing Ltd.

  • 402.
    Winchen, Tobias
    et al.
    Vrije Universiteit Brussel, Belgium.
    Bonardi, Antonio
    Radboud University, Netherlands.
    Buitink, Stijn
    Vrije Universiteit Brussel, Belgium.
    Corstanje, Arthur
    Radboud University, Netherlands.
    Falcke, Heino
    Radboud University, Netherlands;Nikhef, Netherlands;Netherlands Institute of Radio Astronomy (ASTRON), Netherlands.
    Hare, Brian M.
    University of Groningen, Netherlands.
    Hörandel, Jörg R.
    Radboud University, Netherlands;Nikhef, Netherlands.
    Mitra, Pragati
    Vrije Universiteit Brussel, Belgium.
    Mulrey, Katharine
    Vrije Universiteit Brussel, Belgium.
    Nelles, Anna
    Radboud University, Netherlands;University of California Irvine, USA.
    Rachen, J. P.
    Rossetto, L.
    Radboud University, Netherlands.
    Schellart, P.
    Radboud University, Netherlands; Princeton University, United States.
    Scholten, O.
    University Groningen, Netherlands;Vrije Universiteit Brussel, Belgium.
    Ter Veen, S.
    Radboud University, Netherlands;Netherlands Institute of Radio Astronomy (ASTRON), Netherlands.
    Thoudam, Satyendra
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering. Radboud University, Netherlands.
    Trinh, T. N. G.
    University Groningen, Netherlands.
    Overview and status of the lunar detection of cosmic particles with LOFAR2018In: Proceedings of Science: 35th International Cosmic Ray Conference, ICRC 2017; Bexco, Busan; South Korea; 10-20 July 2017, Sissa Medialab Srl , 2018Conference paper (Refereed)
    Abstract [en]

    When a cosmic particle hits matter it produces radio emission via the Askaryan effect. This allows to use Earth's moon as detector for cosmic particles by searching for these ns-pulses with radio telescopes. This technique potentially increases the available collective area by several orders of magnitude compared to current experiments. The LOw Frequency ARray (LOFAR) is the largest radio telescope operating in the optimum frequency regime for corresponding searches. In this contribution, we report on the design and status of the implementation of the lunar detection mode at LOFAR. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).

  • 403.
    Xie, Zhiyuan
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    The design of the optical touchpointer system for brain tumorresections: The electrical system design2014Independent thesis Advanced level (degree of Master (Two Years)), 10 credits / 15 HE creditsStudent thesis
    Abstract [en]

    Glioblastoma multiforme (GBM) is the most common and aggressive form of brain malignancy. The morphological similarities of the malignant and the surrounding tissue cause difficulties in distinguishing the tumors during surgery. Improved methods for precise tumor resection have long been investigated, with the aim to improve the results in resecting malignant brain tumors. Real time diagnostics is obvioulsy crucial for assisting neurosurgical tumor resection. An optical fiber based system is developed in this project. For this electronics is developed for amplifying the weak photocurrent  from the photon detectors, modulating the light sources and supplying power for all the parts of the system. The electronics is controlled by LabView (National Instruments) program. This LabView program also performs signal processing for extracting the diagnostic information from the detected light intensity signals.

  • 404.
    Xing, Hanwen
    et al.
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Liu, Xin
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    A Lithium-ion Battery Charger2015Independent thesis Basic level (degree of Bachelor), 10 credits / 15 HE creditsStudent thesis
    Abstract [en]

       Nowadays personal small electronic devices like cellphones are more and more popular, but the various batteries in need of charging become a problem. This thesis aims to explain a Lithium-ion charger which can control the current and voltage so that it can charge most kinds of popular batteries. More specifically, Li-ion battery charging is presented. The charging circuit design, simulation and the measurements will also be included.

  • 405.
    Xu, F.
    et al.
    Univ Konstanz, Germany.
    Holmqvist, Cecilia
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Rastelli, G.
    Univ Konstanz, Germany.
    Belzig, W.
    Univ Konstanz, Germany.
    Dynamical Coulomb blockade theory of plasmon-mediated light emission from a tunnel junction2016In: Physical Review B, ISSN 2469-9950, E-ISSN 2469-9969, Vol. 94, no 24, article id 245111Article in journal (Refereed)
    Abstract [en]

    Inelastic tunneling of electrons can generate the emission of photons with energies intuitively limited by the applied bias voltage. However, experiments indicate that more complex processes involving the interaction of electrons with plasmon polaritons lead to photon emission with overbias energies. We recently proposed a model of this observation in Phys. Rev. Lett. 113, 066801 (2014), in analogy to the dynamical Coulomb blockade, originally developed for treating the electromagnetic environment in mesoscopic circuits. This model describes the correlated tunneling of two electrons interacting with a local plasmon-polariton mode, represented by a resonant circuit, and shows that the overbias emission is due to the non-Gaussian fluctuations. Here we extend our model to study the overbias emission at finite temperature. We find that the thermal smearing strongly masks the overbias emission. Hence, the detection of the correlated tunneling processes requires temperatures k(B)T much lower than the bias energy eV and the plasmon energy h omega(0), a condition which is fortunately realized experimentally.

  • 406.
    Zacharias, M.
    et al.
    Heidelberg Univ, Germany ; North West Univ, South Africa.
    Bottcher, M.
    North West Univ, South Africa.
    Chakraborty, N.
    Max Planck Inst Kernphys, Germany.
    Cologna, G.
    Heidelberg Univ, Germany.
    Jankowsky, F.
    Heidelberg Univ, Germany.
    Lenain, J. -P
    Mohamed, M.
    Heidelberg Univ, Germany.
    Prokoph, Heike
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Wagner, S.
    Heidelberg Univ, Germany.
    Wierzcholska, A.
    Inst Fizyki Jadrowej PAN, Poland.
    Zaborov, D.
    Ecole Polytech, CNRS, France.
    The Complex VHE And Multiwavelength Flaring Activity Of The FSRQ PKS 1510-089 In May 20152017In: HIGH ENERGY GAMMA-RAY ASTRONOMY / [ed] Aharonian, FA Hofmann, W Rieger, FM, American Institute of Physics (AIP), 2017, article id UNSP 050023Conference paper (Refereed)
    Abstract [en]

    The blazar PKS 1510-089 was the first of the flat spectrum radio quasar type, which had been detected simultaneously by a ground based Cherenkov telescope (H.E.S.S.) and the LAT instrument on board the Fermi satellite. Given the strong broad line region emission defining this blazar class, and the resulting high optical depth for VHE (E > 100 GeV) gamma-rays, it was surprising to detect VHE emission from such an object. In May 2015, PKS 1510-089 exhibited high states throughout the electromagnetic spectrum. Target of Opportunity observations with the H.E.S.S. experiment revealed strong and unprecedented variability of this source. Comparison with the lightcurves obtained with the Fermi-LAT in HE gamma-rays (100 MeV < E < 100 GeV) and ATOM in the optical band shows a complex relationship between these energy bands. This points to a complex structure of the emission region, since the one-zone model has difficulties to reproduce the source behavior even when taking into account absorption by ambient soft photon fields. It will be shown that the presented results have important consequences for the explanation of FSRQ spectra and lightcurves, since the emission region cannot be located deep inside the broad line region as is typically assumed. Additionally, acceleration and cooling processes must be strongly time-dependent in order to account for the observed variability patterns.

  • 407.
    Zheng, Rongpeng
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    An FPGA Based MPPT and Monitoring System: suitable for a photovoltaic based microgrid2019Independent thesis Basic level (degree of Bachelor), 180 HE creditsStudent thesis
    Abstract [en]

    Microgrids containing photovoltaic (PV) cells and wind power gain more and more interest. These microgrids may work in stand-alone mode ("islanding") or be conncted to the main grid. In both modes of operation, power quality must be monitored and controlled.

    This report focuses on microgrids and aims to implement a monitoring system based on FPGA. In the monitoring system, two applications can be achieved, firstly a PAS-MPPT algorithm in a DC-DC boost converter to improve the maximun power point tracking of a PV unit, and secondly a detection and switching system of the grid mode - stand-alone or connected to the main grid. Simulation results prove the Verilog programs in FPGA are suitable to be used in microgrids.

  • 408.
    Zhu, Qizhao
    et al.
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Wang, Yaqi
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    FMCW radar implemented with GNU Radio Companion2016Independent thesis Advanced level (degree of Master (Two Years)), 20 credits / 30 HE creditsStudent thesis
    Abstract [en]

    Continuous-wave frequency-modulated radar, or FMCW radar, is simple in design, small in size and weight and uses low transmitting power. The range resolution depends on the bandwidth. FMCWradar is used in applications ranging from guided weapons systems to vehicle collision avoidance systems. Measuring the distance to the target is the essential feature of FMCW radar. Firstly, this thesis introduces the basic structure of the FMCW radar and the principle formeasuring distance. Secondly, by using software-dened radio (SDR),FMCW radar can be implemented and congured with a reduced costand complexity. In this report, the radar is implemented by means ofthe software GNU Radio Companion with a test signal. HackRF may be used in future work with an osmocom source instead of the testsignal.

  • 409.
    Ziegenbein, Lena
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Lärarens yrkeskunnande: Ett kluvet uppdrag2014Independent thesis Advanced level (degree of Master (One Year)), 10 credits / 15 HE creditsStudent thesis
    Abstract [sv]

    Uppsatsen belyser och beskriver en del av yrkeslärarens många kompetenser och dagliga verksamhet, men den handlar också hur en utveckling av dessa kompetenser skulle kunna ske. Min egen bildningsresa inom frisöryrket skildras med några trevande försök att klippa hår till att numera jobba som frisörlärare. I vårt arbetslag på den gymnasieskola där jag jobbar, som lärare och programansvarig för Hantverksprogrammet, avsattes arbetsplatsträffar under läsåret 2013-2014 för att bland annat få tid till diskussion om begreppet formativ bedömningen, men även för att skapa en plattform för ett kollegialt lärande. Uppsatsen är en del i magisterutbildningen ”yrkeskunnande och professionsutveckling”. 

  • 410.
    Zucca, P.
    et al.
    ASTRON, Netherlands.
    Morosan, D. E.
    Trinity Coll Dublin, Ireland.
    Rouillard, A. P.
    Inst Rech Astrophys & Planetol, France.
    Fallows, R.
    ASTRON, Netherlands.
    Gallagher, P. T.
    Trinity Coll Dublin, Ireland.
    Magdalenic, J.
    Royal Observ Belgium, Belgium.
    Klein, K-L
    Observ Paris, France.
    Mann, G.
    Leibniz Inst Astrophys Potsdam AIP, Germany.
    Vocks, C.
    Leibniz Inst Astrophys Potsdam AIP, Germany.
    Carley, E. P.
    Trinity Coll Dublin, Ireland.
    Bisi, M. M.
    RAL Space, UK.
    Kontar, E. P.
    Univ Glasgow, UK.
    Rothkaehl, H.
    Polish Acad Sci, Poland.
    Dabrowski, B.
    Univ Warmia & Mazury, Poland.
    Krankowski, A.
    Univ Warmia & Mazury, Poland.
    Anderson, J.
    Helmholtz Zentrum Potsdam, Germany.
    Asgekar, A.
    ASTRON, Netherlands;Shell Technol Ctr, India.
    Bell, M. E.
    Univ Technol Sydney, Australia.
    Bentum, M. J.
    ASTRON, Netherlands;Eindhoven Univ Technol, Netherlands.
    Best, P.
    Univ Edinburgh, UK.
    Blaauw, R.
    ASTRON, Netherlands.
    Breitling, F.
    Leibniz Inst Astrophys Potsdam AIP, Germany.
    Broderick, J. W.
    ASTRON, Netherlands.
    Brouw, W. N.
    ASTRON, Netherlands;Kapteyn Astron Inst, Netherlands.
    Brueggen, M.
    Univ Hamburg, Germany.
    Butcher, H. R.
    Australian Natl Univ, Australia.
    Ciardi, B.
    Max Planck Inst Astrophys, Germany.
    de Geus, E.
    ASTRON, Netherlands;SmarterVision BV, Netherlands.
    Deller, A.
    ASTRON, Netherlands;Swinburne Univ Technol, Australia.
    Duscha, S.
    ASTRON, Netherlands.
    Eisloeffel, J.
    Thuringer Landessternwarte,Germany.
    Garrett, M. A.
    Univ Manchester, UK;Leiden Univ, Netherlands.
    Griessmeier, J. M.
    Univ Orleans, France;CNRS, France.
    Gunst, A. W.
    ASTRON, Netherlands.
    Heald, G.
    ASTRON, Netherlands;CSIRO Astron & Space Sci, Australia.
    Hoeft, M.
    Eindhoven Univ Technol, Netherlands.
    Horandel, J.
    Radboud Univ Nijmegen, Netherlands.
    Iacobelli, M.
    ASTRON, Netherlands.
    Juette, E.
    Ruhr Univ Bochum, Germany.
    Karastergiou, A.
    Univ Oxford, UK.
    van Leeuwen, J.
    Trinity Coll Dublin, Ireland;Univ Amsterdam, Netherlands.
    McKay-Bukowski, D.
    Univ Tromso, Norway;STFC Rutherford Appleton Lab, UK.
    Mulder, H.
    ASTRON, Netherlands.
    Munk, H.
    ASTRON, Netherlands;Radboud Univ Nijmegen, Netherlands.
    Nelles, A.
    Univ Calif Irvine, USA.
    Orru, E.
    ASTRON, Netherlands.
    Paas, H.
    Univ Groningen, Netherlands.
    Pandey, V. N.
    ASTRON, Netherlands;Observ Paris, France.
    Pekal, R.
    Poznan Supercomp & Networking Ctr PCSS, Poland.
    Pizzo, R.
    ASTRON, Netherlands.
    Polatidis, A. G.
    ASTRON, Netherlands.
    Reich, W.
    Max Planck Inst Radioastron, Germany.
    Rowlinson, A.
    ASTRON, Netherlands.
    Schwarz, D. J.
    Univ Bielefeld, Germany.
    Shulevski, A.
    Kapteyn Astron Inst, Netherlands.
    Sluman, J.
    ASTRON, Netherlands.
    Smirnov, O.
    Rhodes Univ, South Africa;SKA South Africa, South Africa.
    Sobey, C.
    Curtin Univ, Australia.
    Soida, M.
    Jagiellonian Univ, Poland.
    Thoudam, Satyendra
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Toribio, M. C.
    ASTRON, Netherlands;Kapteyn Astron Inst, Netherlands.
    Vermeulen, R.
    ASTRON, Netherlands.
    van Weeren, R. J.
    Kapteyn Astron Inst, Netherlands.
    Wucknitz, O.
    Max Planck Inst Radioastron, Germany.
    Zarka, P.
    Observ Paris, France.
    Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR2018In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 615, article id A89Article in journal (Refereed)
    Abstract [en]

    Context. Type II radio bursts are evidence of shocks in the solar atmosphere and inner heliosphere that emit radio waves ranging from sub-meter to kilometer lengths. These shocks may be associated with coronal mass ejections (CMEs) and reach speeds higher than the local magnetosonic speed. Radio imaging of decameter wavelengths (20-90 MHz) is now possible with the Low Frequency Array (LOFAR), opening a new radio window in which to study coronal shocks that leave the inner solar corona and enter the interplanetary medium and to understand their association with CMEs. Aims. To this end, we study a coronal shock associated with a CME and type II radio burst to determine the locations at which the radio emission is generated, and we investigate the origin of the band-splitting phenomenon. Methods. The type II shock source-positions and spectra were obtained using 91 simultaneous tied-array beams of LOFAR, and the CME was observed by the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) and by the COR2A coronagraph of the SECCHI instruments on board the Solar Terrestrial Relation Observatory (STEREO). The 3D structure was inferred using triangulation of the coronographic observations. Coronal magnetic fields were obtained from a 3D magnetohydrodynamics (MHD) polytropic model using the photospheric fields measured by the Heliospheric Imager (HMI) on board the Solar Dynamic Observatory (SDO) as lower boundary. Results. The type II radio source of the coronal shock observed between 50 and 70 MHz was found to be located at the expanding flank of the CME, where the shock geometry is quasi-perpendicular with theta(Bn)similar to 70 degrees. The type II radio burst showed first and second harmonic emission; the second harmonic source was cospatial with the first harmonic source to within the observational uncertainty. This suggests that radio wave propagation does not alter the apparent location of the harmonic source. The sources of the two split bands were also found to be cospatial within the observational uncertainty, in agreement with the interpretation that split bands are simultaneous radio emission from upstream and downstream of the shock front. The fast magnetosonic Mach number derived from this interpretation was found to lie in the range 1.3-1.5. The fast magnetosonic Mach numbers derived from modelling the CME and the coronal magnetic field around the type II source were found to lie in the range 1.4-1.6.

  • 411.
    Åhman, Niclas
    et al.
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Gunnarsson, Gunilla
    Linnaeus University, Faculty of Social Sciences, Department of Education.
    Edfors, Inger
    Linnaeus University, Faculty of Health and Life Sciences, Department of Chemistry and Biomedical Sciences.
    In-service science teacher professional development2015In: NorDiNa: Nordic Studies in Science Education, ISSN 1504-4556, E-ISSN 1894-1257, Vol. 11, no 2, p. 207-219Article in journal (Refereed)
    Abstract [en]

    The aim of the present study was to explore teachers’ professional development when using the tool Content Representations (CoRe) to plan a learning study in chemistry, which they also implemented and analysed. The work of six experienced science teachers, all teaching at the 6th to 9th year (age 13 to 16 years), was followed at eight group meetings during one year. The teachers’ discussions during the group meetings were audio and/or video recorded. Recordings were transcribed and a thematic analysis was performed. The results show that two main approaches to teaching emerged in the teachers’ discussions, a pragmatic and a reflective approach, respectively. During the investigation period, the focus of the teachers’ discussions changed, from a predominantly pragmatic approach to a predominantly reflective approach. The results indicate that the work with CoRe and learning study stimulated the teachers to express and discuss their knowledge, beliefs and attitudes towards teaching, i.e. promoted their professional development.

  • 412.
    Åhman, Niclas
    et al.
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Gunnarsson, Gunilla
    Linnaeus University, Faculty of Social Sciences, Department of Education.
    Edfors, Inger
    Linnaeus University, Faculty of Health and Life Sciences, Department of Chemistry and Biomedical Sciences.
    In-service science teachers’ professional development2014Conference paper (Refereed)
  • 413.
    Östergren, Linus
    Linnaeus University, Faculty of Technology, Department of Physics and Electrical Engineering.
    Vätgas som energilagringsmedium för energi från förnyelsebara energikällor2019Independent thesis Basic level (university diploma), 10 credits / 15 HE creditsStudent thesis
    Abstract [sv]

    En omställning till ett mer hållbart samhälle pågår både nationellt och internationellt. Arbete läggs på att öka andelen förnyelsebara energikällor där solceller är en populär produkt. När effekttopparna och de förnyelsebara energikällorna ökar i det svenska stamnätet så skapas ett behov av att lagra stora mängder energi. Att lagra den mängden energi i batterier skulle bli kostsamt. Resultatet från utredningen tyder på att vätgas är ett lämpligt alternativ då omvandlingsprocesserna genererar både elektrisk och termisk energi. Komponenterna som används är ursprungligen från industrin vilket gör dom överdimensionerade för vanliga hushåll. Optimalt används vätgassystem i flerfarmilsbostäder där både den termiska energin och elektriska energin kan nyttjas.   

6789 401 - 413 of 413
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