46 research outputs found
Spectral features of Earth-like planets and their detectability at different orbital distances around F, G, and K-type stars
We investigate the spectral appearance of Earth-like exoplanets in the HZ of
different main sequence stars at different orbital distances. We furthermore
discuss for which of these scenarios biomarker absorption bands may be detected
during primary or secondary transit with near-future telescopes and
instruments.We analyze the spectra taking into account different filter
bandpasses of two photometric instruments planned to be mounted to the JWST. We
analyze in which filters and for which scenarios molecular absorption bands are
detectable when using the space-borne JWST or the ground-based telescope E-ELT.
Absorption bands of CO2, H2O, CH4 and O3 are clearly visible in high-resolution
spectra as well as in the filters of photometric instruments. However, only
during primary eclipse bands of CO2, H2O and O3 are detectable for all
scenarios when using photometric instruments and an E-ELT telescope setup. CH4
is only detectable at the outer HZ of the K star since here the atmospheric
modeling results in very high abundances. Since the detectable CO2 and H2O
bands overlap, separate bands need to be observed to prove their existence in
the atmosphere. In order to detect H2O in a separate band, a S/N>7 needs to be
achieved for E-ELT observations, e.g. by co-adding at least 10 transit
observations. Using a spaceborne telescope like the JWST enables the detection
of CO2 at 4.3mu, which is not possible for ground-based observations due to the
Earth's atmospheric absorption. Hence combining observations of spaceborne and
groundbased telescopes might allow to detect the presence of the biomarker
molecule O3 and the related compounds H2O and CO2 in a planetary atmosphere.
Other absorption bands using the JWST can only be detected for much higher
S/Ns, which is not achievable by just co-adding transit observations since this
would be far beyond the planned mission time of JWST.(abridged)Comment: 15 pages, 8 figure
Rezension: Ulrike Fickler-Stang (2019): Dissoziale Kinder und Jugendliche - unverstanden und unverstehbar?
Transmission Spectroscopy with the ACE-FTS Infrared Spectral Atlas of Earth: A Model Validation and Feasibility Study
Infrared solar occultation measurements are well established for remote
sensing of Earth's atmosphere, and the corresponding primary transit
spectroscopy has turned out to be valuable for characterization of extrasolar
planets. Our objective is an assessment of the detectability of molecular
signatures in Earth's transit spectra.
To this end, we take a limb sequence of representative cloud-free
transmission spectra recorded by the space-borne ACE-FTS Earth observation
mission (Hughes et al., ACE infrared spectral atlases of the Earth's
atmosphere, JQSRT 2014) and combine these spectra to the effective height of
the atmosphere. These data are compared to spectra modeled with an atmospheric
radiative transfer line-by-line infrared code to study the impact of individual
molecules, spectral resolution, the choice of auxiliary data, and numerical
approximations. Moreover, the study serves as a validation of our infrared
radiative transfer code.
The largest impact is due to water, carbon dioxide, ozone, methane, nitrous
oxide, nitrogen, nitric acid, oxygen, and some chlorofluorocarbons (CFC11 and
CFC12). The effect of further molecules considered in the modeling is either
marginal or absent. The best matching model has a mean residuum of 0.4 km and a
maximum difference of 2 km to the measured effective height. For a quantitative
estimate of visibility and detectability we consider the maximum change of the
residual spectrum, the relative change of the residual norm, the additional
transit depth, and signal-to-noise ratios for a JWST setup. In conclusion, our
study provides a list of molecules that are relevant for modeling transmission
spectra of Earth-like exoplanets and discusses the feasibility of retrieval.Comment: 25 pages, 15 figures, 3 table
Zur Relevanz sprachsensiblen Unterrichts im Förderschwerpunkt emotionale und soziale Entwicklung
SprachsensibilitĂ€t gilt als etabliertes QualitĂ€tsmerkmal von Unterricht. Die Bedeutung von Sprachsozialisation und Bildungssprache wird in der PĂ€dagogik bei Verhaltensstörungen bisher jedoch kaum rezipiert. Der Beitrag soll aufzeigen, warum diese Leerstelle geschlossen werden sollte. Er skizziert theoretische Ăberschneidungen von SonderpĂ€dagogik und Sprachwissenschaft, indem er zunĂ€chst fachspezifische sowie linguistische HintergrĂŒnde darstellt und anschlieĂend Konsequenzen dieses interdisziplinĂ€ren Blicks auf den Unterricht im Förderschwerpunkt emotionale und soziale Entwicklung (FS esE) ableitet. (DIPF/Orig.
Sprach- und MilieusensibilitÀt im Kontext von Teilhabe als Gegenstand der (ersten Phase der) Lehrer*innenbildung: Relevanz und Ideen zur Umsetzung
SprachsensibilitĂ€t gilt seit lĂ€ngerer Zeit als ein QualitĂ€tsmerkmal fĂŒr Unterricht. Mit Blick auf die Bedingungen des Aufwachsens der Kinder und Jugendlichen ist sie jedoch unterbestimmt, wenn sie ausschlieĂlich SchĂŒler*innen mit Migrationshintergrund fokussiert. Im Beitrag wird deshalb MilieusensibilitĂ€t als Erweiterung von SprachsensibilitĂ€t vorgeschlagen. Diese greift die Bedingungen des Aufwachsens auf und nutzt sie reflektiert im Unterricht. Durch eine umfassendere BerĂŒcksichtigung der realen Situation aller SchĂŒler*innen sollen die Chancen auf nachschulische Teilhabe erhöht werden.
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This article discusses the importance of sensitivity to language in teaching and proposes an extension to this concept through the introduction of âmilieu sensitivityâ. The article suggests that while sensitivity to language has been recognized as a quality criterion for teaching, it has often only focused on students with a migration background, without fully understanding the conditions of growing up and socialization of all children and young people. By taking into account these conditions and reflecting on them, the concept of milieu sensitivity can promote a more comprehensive understanding of the real-life situation. We argue that by promoting inclusivity and equitable learning outcomes for all students through this approach, post-school participation can be increased
Warming the early Earth - CO2 reconsidered
Despite a fainter Sun, the surface of the early Earth was mostly ice-free.
Proposed solutions to this so-called "faint young Sun problem" have usually
involved higher amounts of greenhouse gases than present in the modern-day
atmosphere. However, geological evidence seemed to indicate that the
atmospheric CO2 concentrations during the Archaean and Proterozoic were far too
low to keep the surface from freezing. With a radiative-convective model
including new, updated thermal absorption coefficients, we found that the
amount of CO2 necessary to obtain 273 K at the surface is reduced up to an
order of magnitude compared to previous studies. For the late Archaean and
early Proterozoic period of the Earth, we calculate that CO2 partial pressures
of only about 2.9 mb are required to keep its surface from freezing which is
compatible with the amount inferred from sediment studies. This conclusion was
not significantly changed when we varied model parameters such as relative
humidity or surface albedo, obtaining CO2 partial pressures for the late
Archaean between 1.5 and 5.5 mb. Thus, the contradiction between sediment data
and model results disappears for the late Archaean and early Proterozoic.Comment: 53 pages, 4 tables, 11 figures, published in Planetary and Space
Scienc
Counseling-related tasks in the context of social and emotional disorders
Beratung gilt als Standardaufgabe sonderpĂ€dagogischer LehrkrĂ€fte, wobei die KomplexitĂ€t der Aufgabe und die einhergehende Notwendigkeit der Professionalisierung hĂ€ufig unterschĂ€tzt werden. Der Beitrag stellt die vielfĂ€ltigen Aufgaben der BeratungstĂ€tigkeit im Förderschwerpunkt esE in ihrer Gesamtheit dar und gibt einen ersten Einblick in ein aktuelles Forschungsprojekt der SonderpĂ€dagogischen Forschungsstelle zu Beratung in der Erziehungshilfe (SFBE) der UniversitĂ€t WĂŒrzburg, das auf der Basis dieser VorĂŒberlegungen die genaue Erfassung, Typisierung und Beschreibung dieser Aufgaben zum Ziel hat. (DIPF/Orig.)On the one hand, Counseling is a key task of special education teachers (Melzer & Hillenbrand, 2015). On the other hand, its complexity combined with the need of professionalization in this field is mostly underestimated (Grewe, 2008). First, this article provides the variety of counseling-related tasks in the context of social and emotional disorders. Second, the paper provides a first insight into a current research project by the Special Educational Research Centre for Consultation Relating to Educational Assistance (SFBE) at Wuerzburg university, which aims on the documentation, typing and description of said tasks. (DIPF/Orig.
Beratung im Kontext der PÀdagogik bei Verhaltensstörungen. Kernelemente eines VerstÀndnisses
Beratung stellt neben Erziehung und Unterricht nicht nur im Bereich der schulischen Erziehungshilfe â aber hier besonders â eine zentrale Aufgabe von LehrkrĂ€ften dar. Was genau diese Aufgabe jedoch beinhaltet und welche Kompetenzen hier von den beratenden SonderpĂ€dagog:innen gefordert werden, bedarf der Diskussion. Ziel dieses Beitrags ist es, durch die Skizzierung des Profils von Beratung fĂŒr den Kontext Verhaltensstörungen eine Grundlage fĂŒr diese Diskussion herauszuarbeiten. Zu diesem Zweck werden Basislinien eines fachspezifischen BeratungsverstĂ€ndnisses umrissen und Merkmale beratender TĂ€tigkeiten im Bereich der schulischen Erziehungshilfe nĂ€her bestimmt. (DIPF/Orig.
GARLIC â A Generic Atmospheric Radiation Line-by-line Infrared Code for Earth and Planetary Science
GARLIC has been developed with emphasis on efficient and reliable numerical algorithms and a modular approach appropriate for simulation and/or retrieval in a variety of applications. It is suitable for arbitrary observation geometry, instrumental field-of-view, and line shape. The core of GARLIC's subroutines constitutes the basis of forward models used to implement inversion codes to retrieve atmospheric state parameters from limb and nadir sounding instruments. In view of the computational burden of lbl modeling considerable effort has been devoted to optimized algorithms. Collision induced absorption has been implemented as a complement of the H2O, CO2, etc continua. Furthermore, the DISORT multiple-scattering solver has been added to GARLIC for an assessment of the impact of clouds on exoplanet spectra. As a recent upgrade Jacobians with respect to temperature have been implemented utilizing algorithmic differentiation.
In this contribution we summarize GARLIC's main features and give some examples from Earth and planetary science