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Progression i progymnasmata

Temat “Retorik och lärande” fångar den pedagogiska dimensionen av retoriken som ett undervisningsämne. Historiskt har utgångspunkten varit de retoriska övningarna, progymnasmata. Min översättning av Afthonios progymnasmata publicerades 2002 under titeln Retoriska övningar. I mina kurser har vi återupptagit dessa övningar så att studenterna gradvis lär sig retorikens grunder. Övningsserien bygger p

Public Reading and Aural Intensity : An Analysis of the Soundscape in John 1–4

This study investigates the public reading of New Testament writings in early Christian communities during the first two centuries C.E. from the perspective of the lectors who prepared and performed the readings. A survey of literary and pictorial sources from the Greek and Roman world indicates that only oratory and drama were delivered from memory, whereas most literary writings were read aloud

What sets could not be

Sets are often taken to be collections, or at least akin to them. In contrast, this paper argues that. although we cannot be sure what sets are (and the question, perhaps, does not even make sense), what we can be entirely sure of is that they are not collections of any kind. The central argument will be that being an element of a set and being a member in a collection are governed by quite differ

Data commentary in science writing: Using a small, specialized corpus for formative self-assessment practices

Data commentary, the verbal comment on visual material, is a complex area in science writing; yet, few studies in academic writing focus on it, and teaching material is often too generic to be of use for students. This chapter presents an approach to addressing the teaching and learning of data commentary in ESP writing courses within the science disciplines involving direct application of a small

Long-term evolution of three-planet systems to the post-main sequence and beyond

We study the stability of systems of three giant planets orbiting 3-8 M☉ stars at orbital distances of >10 au as the host star ages through the main sequence (MS) and well into the white dwarf (WD) stage. Systems are stable on the MS if the planets are separated by more than ~9 Hill radii. Most systems surviving the MS will remain stable until the WD phase, although planets scattered on to small p