995 resultados para Seyferth Fritz


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von Fritz Mänzer [d. i. Isaac Breuer]

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von Fritz Haubrich

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von Georg Fritz

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Die Doktorarbeit “Dein Gott ist ein Esel. Griechische und römische Tierkarikaturen als Spiegel antiker Wertvorstellungen” hat sowohl die lange und intensive Beziehung zwischen Mensch und Tier als auch das antike Humorverständnis zum Thema. Trotz seiner verschiedenen Rollen als Helfer und Freund blieb (und bleibt) das Tier der Stereotyp des ‚Anderen’, das Gegenbild, das alle Menschen teilen. Das Lachen und damit die Karikatur wiederum helfen uns, zu reflektieren und Distanz zu den Dingen und vielleicht zu uns selbst zu gewinnen. Tierkarikaturen sind deshalb besonders geeignet, ein Spiegel menschlicher Fehler und Schwächen zu sein. In der Regel handelt es sich bei den antiken Tierkarikaturen um Bilder von Menschen, die tiergestaltig ‚verzerrt’ sind, zum Beispiel ein Lehrer mit dem Äusseren eines Esels. Solche Darstellungen sind ab dem 6. Jh. v. Chr. zu finden und werden in hellenistischer und römischer Zeit häufiger, wo der Fokus der Arbeit liegt. Meist sind es Terrakotta- oder Bronzefiguren, die verschiedenen gesellschaftlichen Bereichen zugeordnet werden können wie Religion, Politik, Freizeit usw. Unter Berücksichtigung des spezifischen kulturellen und funktionalen Kontextes jedes Stückes sowie zeitgenössischen schriftlichen Quellen wird die Bedeutung dieser Karikaturen erarbeitet.

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BACKGROUND Psoriatic arthritis (PsA) substantially impacts the management of psoriatic disease. OBJECTIVE This study aimed to generate an interdisciplinary national consensus on recommendations of how PsA should be managed. METHODS Based on a systematic literature search, an interdisciplinary expert group identified important domains and went through 3 rounds of a Delphi exercise, followed by a nominal group discussion to generate specific recommendations. RESULTS A strong consensus was reached on numerous central messages regarding the impact of PsA, screening procedures, organization of the interaction between dermatologists and rheumatologists, and treatment goals. CONCLUSION These recommendations can serve as a template for similar initiatives in other countries. At the same time, they highlight the need to take into account the impact of the respective national health care system. © 2015 S. Karger AG, Basel.

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von Fritz Baer

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Hellas basin is a large impact basin situated in the southern highlands of Mars. The north-western part of the basin has the lowest elevation (-7.5 km) on the planet and contains a possibly unique terrain type, which we informally call “banded terrain”. The banded terrain is made up of smooth-looking banded deposits that display signs of viscous behavior and a paucity of superimposed impact craters. In this study, we use newly acquired high spatial resolution images from the High Resolution Imaging Science Experiment (HiRISE) in addition to existing datasets to characterize the geomorphology, the morphometry and the architecture of the banded terrain. The banded terrain is generally confined to the NW edge of the Alpheus Colles plateau. The individual bands are ~3–15 km-long, ~0.3 km-wide and are separated by narrow inter-band depressions, which are ~65 m-wide and ~10 m-deep. The bands display several morphologies that vary from linear to concentric forms. Morphometric analysis reveals that the slopes along a given linear or lobate band ranges from 0.5° to 15° (average~6°), whereas the concentric bands are located on flatter terrain (average slope~2–3°). Crater-size frequency analysis yields an Amazonian-Hesperian boundary crater retention age for the terrain (~3 Gyr), which together, with the presence of very few degraded craters, either implies a recent emplacement, resurfacing, or intense erosion. The apparent sensitivity to local topography and preference for concentrating in localized depressions is compatible with deformation as a viscous fluid. In addition, the bands display clear signs of degradation and slumping at their margins along with a suite of other features that include fractured mounds, polygonal cracks at variable size-scales, and knobby/hummocky textures. Together, these features suggest an ice-rich composition for at least the upper layers of the terrain, which is currently being heavily modified through loss of ice and intense weathering, possibly by wind.