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Reflexion wird in diesem Artikel als Rückmeldung (Feedback) zu einem Sprachlernstand begriffen. Es soll anhand eines Fallbeispiels (IRF-Sequenz) aus dem Unterricht Deutsch als Zweitsprache (DaZ) der Frage nachgegangen werden, wie sich die Feedback-Interaktion gestaltet und inwiefern sich ihr Gelingen oder Misslingen erklären lässt. Dazu wird die evidenzbasierte Forschung zum effektiven Feedback nach Hattie (u. a. Hattie 2020; Hattie & Zierer 2020; Wisniewski & Zierer 2018) in die Analyse einbezogen. Zu wissen, welche Wirkung Feedbacks erzielen, hilft (angehenden) Lehrer:innen, das eigene Handeln zu reflektieren.
Sprache hat im Unterricht verschiedene Funktionen. Sie ist das Instrument zur Vermittlung von Lehrinhalten, das Medium im Unterrichtsgespräch und in Prüfungen. Sprache ist gleichzeitig auch ein Werkzeug des Denkens und damit des Lernens: beim Nachvollziehen von Prozessen, beim Aufbau innerer Vorstellungsbilder und bei der Verknüpfung von neuem Wissen mit altem. Das an der Universität Würzburg durchgeführte interdisziplinäre, praxisorientierte Projektseminar „Sprachsensibles Unterrichtsgeschehen gestalten“ sollte Studierende unter Bezugnahme auf linguistische Theorien zur Mehrsprachigkeitsforschung und Bildungssprache zu einer Reflexion über diese Herausforderungen anregen: Wie kann eine Förderung der (Bildungs-)Sprache und der emotional-sozialen Entwicklung (esE), die einander bedingen, gleichzeitig gelingen ? Um die Ergebnisse der Reflexionsprozesse in anwendbare Lehrkompetenz zu transferieren, entwickelten die Studierenden Materialien für sprachsensiblen Unterricht und esE-Förderung, die, ergänzt durch begründende Ausführungen, in Form eines Readers veröffentlicht werden. Im Folgenden wird das Lehrkonzept theoretisch hergeleitet, anschließend vorgestellt und sodann kritisch reflektiert.
Im Sinne einer „Meta-Reflexivität“ zielt dieser Beitrag darauf ab, den strukturtheoretischen und kompetenzorientierten Professionalisierungsansatz im Konstrukt der adaptiven Lehrkompetenz zusammenzuführen, was vor allem für inklusionsorientierte Ansätze vielversprechend erscheint: Anhand der Konstruktfacetten adaptiver diagnostischer, didaktischer sowie Sach- und Klassenführungskompetenz werden mögliche Herangehensweisen für eine inklusionsorientierte Lehrkräftebildung formuliert, die sowohl konkrete Kompetenzbereiche benennen als auch die Reflexion entsprechender Spannungsverhältnisse im strukturtheoretischen Sinne voraussetzen. So soll der Beitrag einen knappen theoretischen Aufriss zur Zusammenführung der unterschiedlichen Professionalisierungsansätze unter der Prämisse (mehr) Reflexion für (mehr) Inklusion leisten.
Der Auf- und Ausbau eines inklusiven Bildungssystems vor dem Hintergrund rascher und weitreichender gesellschaftlicher Veränderungen bringt für Lehrkräfte aller Schulformen vielfältige Aufgaben mit sich. Eine der entscheidenden Gelingensbedingungen für die Realisation inklusiver Bildung bildet dementsprechend die Professionalisierung von Lehrkräften. Reflexionskompetenz nimmt beim Auf- und Ausbau einer professionellen Handlungskompetenz von Lehrpersonen einen besonderen Stellenwert ein, allerdings reflektieren Lehramtsstudierende am Anfang ihres Studiums häufig noch auf eher niedrigem Niveau. Im Rahmen des fünfsemestrigen Zertifikatskurses „Handlungswissen Inklusion“ (HWI) an der Universität zu Köln erhalten BA-Studierende die Möglichkeit, ihr Lehramtsstudium inklusionsorientiert(er) auszurichten, um sich auf die anstehenden Herausforderungen in einer inklusiven Schule und Gesellschaft vorzubereiten und gleichzeitig die damit einhergehende domänenspezifische Reflexionskompetenz zu steigern.
Lehrkräfte fühlen sich nicht genug auf inklusiven Unterricht vorbereitet, wenngleich sie allen Schülerinnen und Schülern Zugänge zu Phänomenen, Konzepten, Arbeitsweisen usw. ermöglichen sollen. Im Projekt Nawi-In haben wir u. a. die Fragen adressiert, welche inklusiv naturwissenschaftlichen Charakteristika Lehramtsstudierende in ihren eigenen und fremden Unterrichtsvideos wahrnehmen und wie sich ihre Kompetenzen entwickeln. Die Reflexionen des Unterrichts fanden über drei Semester einschließlich der Praxisphase statt. In ausgewählten Videoszenen sollten die Studierenden inklusiv naturwissenschaftliche Charakteristika beschreiben und reflektieren. Ausgewertet wurden die autographierten und transkribierten Reflexionen mit dem KinU, welches systematisch die Charakteristika inklusiven naturwissenschaftlichen Unterrichts abbildet. Zu Beginn haben die Studierenden eher allgemeinpädagogische Aspekte und die Lehrkräftepersönlichkeit wahrgenommen. Später haben sie den Fokus auf den Naturwissenschaftsunterricht und die Diversität der Klasse gesetzt. Insgesamt haben die Studierenden zunehmend mehr Charakteristika inklusiven naturwissenschaftlichen Unterrichts identifiziert und Handlungsalternativen generiert.
The increasing number of known exoplanets raises questions about their demographics and the mechanisms that shape planets into how we observe them today. Young planets in close-in orbits are exposed to harsh environments due to the host star being magnetically highly active, which results in high X-ray and extreme UV fluxes impinging on the planet. Prolonged exposure to this intense photoionizing radiation can cause planetary atmospheres to heat up, expand and escape into space via a hydrodynamic escape process known as photoevaporation. For super-Earth and sub-Neptune-type planets, this can even lead to the complete erosion of their primordial gaseous atmospheres. A factor of interest for this particular mass-loss process is the activity evolution of the host star. Stellar rotation, which drives the dynamo and with it the magnetic activity of a star, changes significantly over the stellar lifetime. This strongly affects the amount of high-energy radiation received by a planet as stars age. At a young age, planets still host warm and extended envelopes, making them particularly susceptible to atmospheric evaporation. Especially in the first gigayear, when X-ray and UV levels can be 100 - 10,000 times higher than for the present-day sun, the characteristics of the host star and the detailed evolution of its high-energy emission are of importance.
In this thesis, I study the impact of stellar activity evolution on the high-energy-induced atmospheric mass loss of young exoplanets. The PLATYPOS code was developed as part of this thesis to calculate photoevaporative mass-loss rates over time. The code, which couples parameterized planetary mass-radius relations with an analytical hydrodynamic escape model, was used, together with Chandra and eROSITA X-ray observations, to investigate the future mass loss of the two young multiplanet systems V1298 Tau and K2-198. Further, in a numerical ensemble study, the effect of a realistic spread of activity tracks on the small-planet radius gap was investigated for the first time. The works in this thesis show that for individual systems, in particular if planetary masses are unconstrained, the difference between a young host star following a low-activity track vs. a high-activity one can have major implications: the exact shape of the activity evolution can determine whether a planet can hold on to some of its atmosphere, or completely loses its envelope, leaving only the bare rocky core behind. For an ensemble of simulated planets, an observationally-motivated distribution of activity tracks does not substantially change the final radius distribution at ages of several gigayears. My simulations indicate that the overall shape and slope of the resulting small-planet radius gap is not significantly affected by the spread in stellar activity tracks. However, it can account for a certain scattering or fuzziness observed in and around the radius gap of the observed exoplanet population.
The icosahedral non-hydrostatic large eddy model (ICON-LEM) was applied around the drift track of the Multidisciplinary Observatory Study of the Arctic (MOSAiC) in 2019 and 2020. The model was set up with horizontal grid-scales between 100m and 800m on areas with radii of 17.5km and 140 km. At its lateral boundaries, the model was driven by analysis data from the German Weather Service (DWD), downscaled by ICON in limited area mode (ICON-LAM) with horizontal grid-scale of 3 km.
The aim of this thesis was the investigation of the atmospheric boundary layer near the surface in the central Arctic during polar winter with a high-resolution mesoscale model. The default settings in ICON-LEM prevent the model from representing the exchange processes in the Arctic boundary layer in accordance to the MOSAiC observations. The implemented sea-ice scheme in ICON does not include a snow layer on sea-ice, which causes a too slow response of the sea-ice surface temperature to atmospheric changes. To allow the sea-ice surface to respond faster to changes in the atmosphere, the implemented sea-ice parameterization in ICON was extended with an adapted heat capacity term.
The adapted sea-ice parameterization resulted in better agreement with the MOSAiC observations. However, the sea-ice surface temperature in the model is generally lower than observed due to biases in the downwelling long-wave radiation and the lack of complex surface structures, like leads. The large eddy resolving turbulence closure yielded a better representation of the lower boundary layer under strongly stable stratification than the non-eddy-resolving turbulence closure. Furthermore, the integration of leads into the sea-ice surface reduced the overestimation of the sensible heat flux for different weather conditions.
The results of this work help to better understand boundary layer processes in the central Arctic during the polar night. High-resolving mesoscale simulations are able to represent temporally and spatially small interactions and help to further develop parameterizations also for the application in regional and global models.
With Arctic ground as a huge and temperature-sensitive carbon reservoir, maintaining low ground temperatures and frozen conditions to prevent further carbon emissions that contrib-ute to global climate warming is a key element in humankind’s fight to maintain habitable con-ditions on earth. Former studies showed that during the late Pleistocene, Arctic ground condi-tions were generally colder and more stable as the result of an ecosystem dominated by large herbivorous mammals and vast extents of graminoid vegetation – the mammoth steppe. Characterised by high plant productivity (grassland) and low ground insulation due to animal-caused compression and removal of snow, this ecosystem enabled deep permafrost aggrad-ation. Now, with tundra and shrub vegetation common in the terrestrial Arctic, these effects are not in place anymore. However, it appears to be possible to recreate this ecosystem local-ly by artificially increasing animal numbers, and hence keep Arctic ground cold to reduce or-ganic matter decomposition and carbon release into the atmosphere.
By measuring thaw depth, total organic carbon and total nitrogen content, stable carbon iso-tope ratio, radiocarbon age, n-alkane and alcohol characteristics and assessing dominant vegetation types along grazing intensity transects in two contrasting Arctic areas, it was found that recreating conditions locally, similar to the mammoth steppe, seems to be possible. For permafrost-affected soil, it was shown that intensive grazing in direct comparison to non-grazed areas reduces active layer depth and leads to higher TOC contents in the active layer soil. For soil only frozen on top in winter, an increase of TOC with grazing intensity could not be found, most likely because of confounding factors such as vertical water and carbon movement, which is not possible with an impermeable layer in permafrost. In both areas, high animal activity led to a vegetation transformation towards species-poor graminoid-dominated landscapes with less shrubs. Lipid biomarker analysis revealed that, even though the available organic material is different between the study areas, in both permafrost-affected and sea-sonally frozen soils the organic material in sites affected by high animal activity was less de-composed than under less intensive grazing pressure. In conclusion, high animal activity af-fects decomposition processes in Arctic soils and the ground thermal regime, visible from reduced active layer depth in permafrost areas. Therefore, grazing management might be utilised to locally stabilise permafrost and reduce Arctic carbon emissions in the future, but is likely not scalable to the entire permafrost region.
Large parts of the Earth’s interior are inaccessible to direct observation, yet global geodynamic processes are governed by the physical material properties under extreme pressure and temperature conditions. It is therefore essential to investigate the deep Earth’s physical properties through in-situ laboratory experiments. With this goal in mind, the optical properties of mantle minerals at high pressure offer a unique way to determine a variety of physical properties, in a straight-forward, reproducible, and time-effective manner, thus providing valuable insights into the physical processes of the deep Earth. This thesis focusses on the system Mg-Fe-O, specifically on the optical properties of periclase (MgO) and its iron-bearing variant ferropericlase ((Mg,Fe)O), forming a major planetary building block. The primary objective is to establish links between physical material properties and optical properties. In particular the spin transition in ferropericlase, the second-most abundant phase of the lower mantle, is known to change the physical material properties. Although the spin transition region likely extends down to the core-mantle boundary, the ef-fects of the mixed-spin state, where both high- and low-spin state are present, remains poorly constrained.
In the studies presented herein, we show how optical properties are linked to physical properties such as electrical conductivity, radiative thermal conductivity and viscosity. We also show how the optical properties reveal changes in the chemical bonding. Furthermore, we unveil how the chemical bonding, the optical and other physical properties are affected by the iron spin transition. We find opposing trends in the pres-sure dependence of the refractive index of MgO and (Mg,Fe)O. From 1 atm to ~140 GPa, the refractive index of MgO decreases by ~2.4% from 1.737 to 1.696 (±0.017). In contrast, the refractive index of (Mg0.87Fe0.13)O (Fp13) and (Mg0.76Fe0.24)O (Fp24) ferropericlase increases with pressure, likely because Fe Fe interactions between adjacent iron sites hinder a strong decrease of polarizability, as it is observed with increasing density in the case of pure MgO. An analysis of the index dispersion in MgO (decreasing by ~23% from 1 atm to ~103 GPa) reflects a widening of the band gap from ~7.4 eV at 1 atm to ~8.5 (±0.6) eV at ~103 GPa. The index dispersion (between 550 and 870 nm) of Fp13 reveals a decrease by a factor of ~3 over the spin transition range (~44–100 GPa). We show that the electrical band gap of ferropericlase significantly widens up to ~4.7 eV in the mixed spin region, equivalent to an increase by a factor of ~1.7. We propose that this is due to a lower electron mobility between adjacent Fe2+ sites of opposite spin, explaining the previously observed low electrical conductivity in the mixed spin region. From the study of absorbance spectra in Fp13, we show an increasing covalency of the Fe-O bond with pressure for high-spin ferropericlase, whereas in the low-spin state a trend to a more ionic nature of the Fe-O bond is observed, indicating a bond weakening effect of the spin transition. We found that the spin transition is ultimately caused by both an increase of the ligand field-splitting energy and a decreasing spin-pairing energy of high-spin Fe2+.