TY - THES A1 - Nickelt-Czycykowski, Iliya Peter T1 - Aktive Regionen der Sonnenoberfläche und ihre zeitliche Variation in zweidimensionaler Spektro-Polarimetrie T1 - Active regions on the solar surface and their temporal variation in two-dimensional spectropolarimetry N2 - Die Arbeit beschreibt die Analyse von Beobachtungen zweier Sonnenflecken in zweidimensionaler Spektro-Polarimetrie. Die Daten wurden mit dem Fabry-Pérot-Interferometer der Universität Göttingen am Vakuum-Turm-Teleskop auf Teneriffa erfasst. Von der aktiven Region NOAA 9516 wurde der volle Stokes-Vektor des polarisierten Lichts in der Absorptionslinie bei 630,249 nm in Einzelaufnahmen beobachtet, und von der aktiven Region NOAA 9036 wurde bei 617,3 nm Wellenlänge eine 90-minütige Zeitserie des zirkular polarisierten Lichts aufgezeichnet. Aus den reduzierten Daten werden Ergebniswerte für Intensität, Geschwindigkeit in Beobachtungsrichtung, magnetische Feldstärke sowie verschiedene weitere Plasmaparameter abgeleitet. Mehrere Ansätze zur Inversion solarer Modellatmosphären werden angewendet und verglichen. Die teilweise erheblichen Fehlereinflüsse werden ausführlich diskutiert. Das Frequenzverhalten der Ergebnisse und Abhängigkeiten nach Ort und Zeit werden mit Hilfe der Fourier- und Wavelet-Transformation weiter analysiert. Als Resultat lässt sich die Existenz eines hochfrequenten Bandes für Geschwindigkeitsoszillationen mit einer zentralen Frequenz von 75 Sekunden (13 mHz) bestätigen. In größeren photosphärischen Höhen von etwa 500 km entstammt die Mehrheit der damit zusammenhängenden Schockwellen den dunklen Anteilen der Granulen, im Unterschied zu anderen Frequenzbereichen. Die 75-Sekunden-Oszillationen werden ebenfalls in der aktiven Region beobachtet, vor allem in der Lichtbrücke. In den identifizierten Bändern oszillatorischer Power der Geschwindigkeit sind in einer dunklen, penumbralen Struktur sowie in der Lichtbrücke ausgeprägte Strukturen erkennbar, die sich mit einer Horizontalgeschwindigkeit von 5-8 km/s in die ruhige Sonne bewegen. Diese zeigen einen deutlichen Anstieg der Power, vor allem im 5-Minuten-Band, und stehen möglicherweise in Zusammenhang mit dem Phänomen der „Evershed-clouds“. Eingeschränkt durch ein sehr geringes Signal-Rausch-Verhältnis und hohe Fehlereinflüsse werden auch Magnetfeldvariationen mit einer Periode von sechs Minuten am Übergang von Umbra zu Penumbra in der Nähe einer Lichtbrücke beobachtet. Um die beschriebenen Resultate zu erzielen, wurden bestehende Visualisierungsverfahren der Frequenzanalyse verbessert oder neu entwickelt, insbesondere für Ergebnisse der Wavelet-Transformation. N2 - The publication describes the analysis of two sunspot observations in two-dimensional spectropolarimetry. The data was obtained with the Fabry-Pérot-interferometer of Göttingen University at the German Vacuum Tower Telescope on Tenerife. Of the active region NOAA 9516 the full Stokes vector of polarised light was observed in the absorption line at 630.249 nm in single scans. A ninety minute time series of circular polarised light of the active region NOAA 9036 was observed at 617.3 nm wavelength. From the reduced data results for intensity, line-of-sight velocity, magnetic field strength as well as several other plasma parameters are inferred. Different approaches to solar atmosphere model inversion are applied and compared. The significant influence of errors is discussed in detail. The frequency behaviour of the results and spatial and temporal dependencies are further analysed by Fourier and wavelet transformation. As a result the existence of a high frequency band of velocity oscillations with a central frequency of about 75-seconds (13 mHz) can be confirmed. In greater heights of about 500 km the majority of the corresponding shock waves are derived from darker parts of the granules in contrast to the dominant five-minute-oscillations. 75-second-oscillations can also be observed in the active region, especially in the light bridge. In the identified bands of oscillatory velocity power, distinct structures become visible in a penumbral dark structure as well as in the light bridge that move into the quiet sun with a horizontal speed of 5-8 km/s. They show an increase in power, mostly 5-minute-band, and may be related to the Evershed cloud phenomenon. Under the constraint of a very low signal-to-noise ratio and high error influence, magnetic field variations of a 6-minute period are also observed in an umbral-penumbral transition area close to a light bridge. To derive these results, existing visualisation methods for frequency analysis where improved or newly developed, especially so for wavelet transform results. KW - Sonne: Oszillationen KW - Sonne: Sonnenflecken KW - Instrumente: Polarimeter KW - Instrumente: Spektrographen KW - Frequenzanalyse KW - Sun: oszillations KW - Sun: sunspots KW - instrumentation: polarimeters KW - instrumentation: spectrographs KW - frequency analysis Y1 - 2008 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus-25524 ER - TY - JOUR A1 - Thieken, Annegret A1 - Apel, Heiko A1 - Merz, Bruno T1 - Assessing the probability of large-scale flood loss events: a case study for the river Rhine, Germany JF - Journal of flood risk management N2 - Flood risk analyses are often estimated assuming the same flood intensity along the river reach under study, i.e. discharges are calculated for a number of return periods T, e.g. 10 or 100 years, at several streamflow gauges. T-year discharges are regionalised and then transferred into T-year water levels, inundated areas and impacts. This approach assumes that (1) flood scenarios are homogeneous throughout a river basin, and (2) the T-year damage corresponds to the T-year discharge. Using a reach at the river Rhine, this homogeneous approach is compared with an approach that is based on four flood types with different spatial discharge patterns. For each type, a regression model was created and used in a Monte-Carlo framework to derive heterogeneous scenarios. Per scenario, four cumulative impact indicators were calculated: (1) the total inundated area, (2) the exposed settlement and industrial areas, (3) the exposed population and 4) the potential building loss. Their frequency curves were used to establish a ranking of eight past flood events according to their severity. The investigation revealed that the two assumptions of the homogeneous approach do not hold. It tends to overestimate event probabilities in large areas. Therefore, the generation of heterogeneous scenarios should receive more attention. KW - damage estimation KW - discharge pattern KW - exposure KW - flood risk analysis KW - frequency analysis KW - land-use KW - population density Y1 - 2015 U6 - https://doi.org/10.1111/jfr3.12091 SN - 1753-318X VL - 8 IS - 3 SP - 247 EP - 262 PB - Wiley-Blackwell CY - Hoboken ER - TY - JOUR A1 - Kellermann, Patric A1 - Bubeck, Philip A1 - Kundela, Guenther A1 - Dosio, Alessandro A1 - Thieken, Annegret T1 - Frequency Analysis of Critical Meteorological Conditions in a Changing ClimateAssessing Future Implications for Railway Transportation in Austria JF - Climate : open access journal N2 - Meteorological extreme events have great potential for damaging railway infrastructure and posing risks to the safety of train passengers. In the future, climate change will presumably have serious implications on meteorological hazards in the Alpine region. Hence, attaining insights on future frequencies of meteorological extremes with relevance for the railway operation in Austria is required in the context of a comprehensive and sustainable natural hazard management plan of the railway operator. In this study, possible impacts of climate change on the frequencies of so-called critical meteorological conditions (CMCs) between the periods 1961-1990 and 2011-2040 are analyzed. Thresholds for such CMCs have been defined by the railway operator and used in its weather monitoring and early warning system. First, the seasonal climate change signals for air temperature and precipitation in Austria are described on the basis of an ensemble of high-resolution Regional Climate Model (RCM) simulations for Europe. Subsequently, the RCM-ensemble was used to investigate changes in the frequency of CMCs. Finally, the sensitivity of results is analyzed with varying threshold values for the CMCs. Results give robust indications for an all-season air temperature rise, but show no clear tendency in average precipitation. The frequency analyses reveal an increase in intense rainfall events and heat waves, whereas heavy snowfall and cold days are likely to decrease. Furthermore, results indicate that frequencies of CMCs are rather sensitive to changes of thresholds. It thus emphasizes the importance to carefully define, validate, andif neededto adapt the thresholds that are used in the weather monitoring and warning system of the railway operator. For this, continuous and standardized documentation of damaging events and near-misses is a pre-requisite. KW - climate change KW - critical meteorological condition KW - frequency analysis KW - natural hazard management KW - railway transportation Y1 - 2016 U6 - https://doi.org/10.3390/cli4020025 SN - 2225-1154 VL - 4 SP - 914 EP - 931 PB - MDPI CY - Basel ER - TY - GEN A1 - Kellermann, Patric A1 - Bubeck, Philip A1 - Kundela, Günther A1 - Dosio, Alessandro A1 - Thieken, Annegret T1 - Frequency analysis of critical meteorological conditions in a changing climate BT - assessing future implications for railway transportation in Austria N2 - Meteorological extreme events have great potential for damaging railway infrastructure and posing risks to the safety of train passengers. In the future, climate change will presumably have serious implications on meteorological hazards in the Alpine region. Hence, attaining insights on future frequencies of meteorological extremes with relevance for the railway operation in Austria is required in the context of a comprehensive and sustainable natural hazard management plan of the railway operator. In this study, possible impacts of climate change on the frequencies of so-called critical meteorological conditions (CMCs) between the periods 1961-1990 and 2011-2040 are analyzed. Thresholds for such CMCs have been defined by the railway operator and used in its weather monitoring and early warning system. First, the seasonal climate change signals for air temperature and precipitation in Austria are described on the basis of an ensemble of high-resolution Regional Climate Model (RCM) simulations for Europe. Subsequently, the RCM-ensemble was used to investigate changes in the frequency of CMCs. Finally, the sensitivity of results is analyzed with varying threshold values for the CMCs. Results give robust indications for an all-season air temperature rise, but show no clear tendency in average precipitation. The frequency analyses reveal an increase in intense rainfall events and heat waves, whereas heavy snowfall and cold days are likely to decrease. Furthermore, results indicate that frequencies of CMCs are rather sensitive to changes of thresholds. It thus emphasizes the importance to carefully define, validate, andif neededto adapt the thresholds that are used in the weather monitoring and warning system of the railway operator. For this, continuous and standardized documentation of damaging events and near-misses is a pre-requisite. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 358 KW - climate change KW - critical meteorological condition KW - frequency analysis KW - natural hazard management KW - railway transportation Y1 - 2017 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-400505 ER -