New Observations of Balmer Continuum Flux in Solar Flares, Instrument Description and First Results

Increase in the Balmer continuum radiation during solar flares was predicted by various authors but never firmly confirmed observationally using ground-based slit spectrographs. Here we describe a new post-focal instrument - Image Selector - enabling to measure the Balmer continuum flux from the whole flare area, in analogy of successful detections of flaring dMe stars. The system was developed and put into operation at the horizontal solar telescope HSFA-2 of the Ond\v{r}ejov Observatory. We measure the total flux by a fast spectrometer from a limited but well defined region on the solar disk. Using a system of diaphragms, the disturbing contribution of a bright solar disk can be eliminated as much as possible. Light curves of the measured flux in the spectral range 350 - 440 nm are processed, together with the H{\alpha} images of the flaring area delimited by the appropriate diaphragm. The spectral flux data are flat-fielded, calibrated and processed to be compared with model predictions. Our analysis of the data proves that the described device is sufficiently sensitive to detect variations in the Balmer continuum during solar flares. Assuming that the Balmer-continuum kernels have at least a similar size as those visible in H\alpha, we find the flux increase in the Balmer continuum to reach 230 % - 550 % of the quiet continuum during the observed X-class flare. We also found temporal changes in the Balmer continuum flux starting well before the onset of the flare in H{\alpha}.Comment: 12 pages, 4 figure

Three-port beam splitters-combiners for interferometer applications

We derive generic phase and amplitude coupling relations for beam splitters-combiners that couple a single port with three output ports or input ports, respectively. We apply the coupling relations to a reflection grating that serves as a coupler to a single-ended Fabry-Perot ring cavity. In the impedance-matched case such an interferometer can act as an all-reflective ring mode cleaner. It is further shown that in the highly undercoupled case almost complete separation of carrier power and phase signal from a cavity strain can be achieved

Highly Integrated Steam Reforming Fuel Processor with Condensing Burner Technology for Maximised Electrical Efficiency of CHP-PEMFC Systems

AbstractCompact fuel processors using natural gas, LPG and biogas for μCHP fuel cell systems have been developed at ZBT for over 10 years. The technology, based on steam reforming, includes a reformer and a WGS reactor, a water evaporator, heat exchangers and a fuel/anodic offgas burner integrated in an insulated housing. For coupling with a LT-PEMFC today an external preferential oxidation or methanation is added. A HT-PEMFC can be coupled directly to the fuel processor at a temperature level of 160°C. It is discussed that HT-PEMFC systems can exceed the electrical efficiency of LT-PEMFC systems up to five percentage points because of the integration of high quality heat from the fuel cell cooling cycle. In process simulations with AspenPlus® this efficiency advantage could be confirmed. But further investigations concerning heat integration showed for both systems the advantage of using the condensation enthalpy of the flue gas provided by the system burner. This gain in energy offers the opportunity to realise burner operation only with anodic offgas, without additional fuel firing. This study shows the use of condensing burner technology in the fuel processor in comparison of integrating HT-PEMFC heat and/or the use of conventional low-temperature burner technology. For comparison the system boundaries and efficiencies were clearly determined. Heat sources and sinks were identified and quantified along the process chain of steam reforming. A pinch analysis illustrates the requirement of additional heat flows concerning their power and temperature levels

Erratum: Laser-Frequency Stabilization via a Quasimonolithic Mach-Zehnder Interferometer with Arms of Unequal Length and Balanced dc Readout [Phys. Rev. Applied 7, 024027 (2017)]

Low frequency high precision laser interferometry is subject to excess laser frequency noise coupling via arm-length differences which is commonly mitigated by locking the frequency to a stable reference system. This is crucial to achieve picometer level sensitivities in the 0.1 mHz to 1 Hz regime, where laser frequency noise is usually high and couples into the measurement phase via arm-length mismatches in the interferometers. Here we describe the results achieved by frequency stabilising an external cavity diode laser to a quasi-monolithic unequal arm-length Mach-Zehnder interferometer read out at mid-fringe via balanced detection. This stabilisation scheme has been found to be an elegant solution combining a minimal number of optical components, no additional laser modulations and relatively low frequency noise levels. The Mach-Zehnder interferometer has been designed and constructed to minimise the influence of thermal couplings and to reduce undesired stray light using the optical simulation tool IfoCAD. We achieve frequency noise levels corresponding to LISA-like (laser interferometer space antenna) displacement sensitivities below 1 pm/$\sqrt{\textrm{Hz}}$ and are able to demonstrate the LISA frequency pre-stabilisation requirement of 300 Hz/$\sqrt{\textrm{Hz}}$ down to frequencies of 100 mHz by beating the stabilised laser with an Iodine locked reference

Modelling background charge rearrangements near single-electron transistors as a Poisson process

Background charge rearrangements in metallic single-electron transistors are modelled in two-level tunnelling systems as a Poisson process with a scale parameter as only variable. The model explains the recent observation of asymmetric Coulomb blockade peak spacing distributions in metallic single-electron transistors. From the scale parameter we estimate the average size of the tunnelling systems, their density of states, and the height of their energy barrier. We conclude that the observed background charge rearrangements predominantly take place in the substrate of the single-electron transistor.Comment: 7 pages, 2 eps figures, used epl.cls macro include

Towards a FPGA-controlled deep phase modulation interferometer

Deep phase modulation interferometry was proposed as a method to enhance homodyne interferometers to work over many fringes. In this scheme, a sinusoidal phase modulation is applied in one arm while the demodulation takes place as a post-processing step. In this contribution we report on the development to implement this scheme in a fiber coupled interferometer controlled by means of a FPGA, which includes a LEON3 soft-core processor. The latter acts as a CPU and executes a custom made application to communicate with a host PC. In contrast to usual FPGA-based designs, this implementation allows a real-time fine tuning of the parameters involved in the setup, from the control to the post-processing parameters.Comment: Proceedings of the X LISA Symposium, Gainesville, May 18-23, 201

The Ly<alpha> and Ly<beta> profiles in solar prominences and prominence fine structure

We present the first combined Ly and Ly profiles in solar prominences obtained by the SOHO/SUMER instrument and discuss their important spatial variability with respect to predictions from 1D and multithread models.Comment: Accepted in Solar Physics, 14 pages with 9 figures and 3 Table

Kindersimulation heute und morgen: Perspektiven und Konzepte

Zusammenfassung: Die Konfrontation mit kritisch kranken Neugeborenen, Säuglingen und Kleinkindern ist selten und stellt ein Behandlungsteam vor besondere Herausforderungen. Für eine erfolgreiche Notfallbehandlung sind sichere technische und nichttechnische Fertigkeiten essenziell. Kindersimulatoren ermöglichen die Schaffung einer didaktischen Infrastruktur zur Vernetzung von Lehrbuchtheorie mit erfahrungsaktiver Praxis. Zur Erfassung des aktuellen Status der Kindersimulation in Deutschland, Österreich und der Schweiz wurde eine Onlinebefragung aller entsprechend aktiven Zentren durchgeführt. Derzeit wird Kindersimulation in 24Zentren betrieben. Diese verfügen über 39 pädiatrische Simulatoren: 8 für Neugeborene, 26 für Säuglinge und 5 für Kinder. Eine gewisse Kongruenz im Standard ist unter den Zentren feststellbar. Die meisten Instruktoren verfügen über eine spezialisierte Instruktorenausbildung. Von den Instruktoren sind 26% Pflegefachkräfte und 67% Ärzte, davon haben Pädiater und Anästhesisten den größten Anteil. Viele Zentren (38%) funktionieren lediglich durch das spezielle Engagement ihrer Mitarbeiter, die diverse Aktivitäten in ihrer Freizeit organisieren. Videogestützte Nachbesprechungen gelten als Grundlage für ein effektives Training. Einen besonderen inhaltlichen Schwerpunkt legen fast alle Zentren (92%) auf die Vermittlung von nichttechnischen Fertigkeiten (interpersonelle Aspekte des Zwischenfallmanagements). Im Rahmen des kürzlich etablierten PaedSim-Projekts sollen die Curricula von Kindersimulationskursen noch klarer strukturiert sowie international standardisiert werden, um dadurch Trainingseffektivität und -nachhaltigkeit zu erhöhe

The influence of laser relative intensity noise in the Laser Interferometer Space Antenna

LISA is an upcoming ESA mission that will detect gravitational waves in spaceby interferometrically measuring the separation between free-falling testmasses at picometer precision. To reach the desired performance, LISA willemploy the noise reduction technique time-delay interferometry (TDI), in whichmultiple raw interferometric readouts are time shifted and combined into thefinal scientific observables. Evaluating the performance in terms of these TDIvariables requires careful tracking of how different noise sources propagatethrough TDI, as noise correlations might affect the performance in unexpectedways. One example of such potentially correlated noise is the relativeintensity noise (RIN) of the six lasers aboard the three LISA satellites, whichwill couple into the interferometric phase measurements. In this article, wecalculate the expected RIN levels based on the current mission architecture andthe envisaged mitigation strategies. We find that strict requirements on thetechnical design reduce the effect from approximately 8.7 pm/rtHz perinter-spacecraft interferometer to that of a much lower sub-1 pm/rtHz noise,with typical characteristics of an uncorrelated readout noise after TDI. Ourinvestigations underline the importance of sufficient balanced detection of theinterferometric measurements.<br