El niño malo que se hizo director de cine : De mayor quiero ser soldado, de Christian Molina.

El artículo forma parte de un dossier titulado: Cine: emoción e identidad. Resumen basado en la publicación

Girona en una tesi doctoral francesa [Ressenya del llibre 'Girona al segle XIV', de Christian Guilleré]

Sobre la publicació del primer volum de la tesi de Christian Guilleré, La Girona del segle XIV

Christian Gottlob Heyne and the changing fortunes of the commentary in the age of Altertumswissenschaft

This chapter discusses the pedagogic and scholarly priorities that informed Heyne’s commentaries on Tibullus (1755), Virgil (1767-75) and Homer (1802), as well as their initial critical reception. Like those of his teachers, Gesner and Ernesti, Heyne’s works eschew detailed textual scholarship in favour of aesthetic and historicizing appreciation of literary works as wholes. Their formal innovations – most notably the relegation of advanced philological discussions to endnotes and the inclusion of excursuses on significant historical and cultural questions – are an attempt to tailor a traditional format to the demands of an Enlightened age and the cultural-historical interests of the new Altertumswissenschaft. The chapter discusses their contrasting critical receptions in order to raise questions about the viability of Heyne’s endeavours to make a traditional medium fit new concerns.

The Maunder minimum (1645-1715) was indeed a grand minimum: a reassessment of multiple datasets

Aims. Although the time of the Maunder minimum (1645–1715) is widely known as a period of extremely low solar activity, it is still being debated whether solar activity during that period might have been moderate or even higher than the current solar cycle (number 24). We have revisited all existing evidence and datasets, both direct and indirect, to assess the level of solar activity during the Maunder minimum. Methods. We discuss the East Asian naked-eye sunspot observations, the telescopic solar observations, the fraction of sunspot active days, the latitudinal extent of sunspot positions, auroral sightings at high latitudes, cosmogenic radionuclide data as well as solar eclipse observations for that period. We also consider peculiar features of the Sun (very strong hemispheric asymmetry of the sunspot location, unusual differential rotation and the lack of the K-corona) that imply a special mode of solar activity during the Maunder minimum. Results. The level of solar activity during the Maunder minimum is reassessed on the basis of all available datasets. Conclusions. We conclude that solar activity was indeed at an exceptionally low level during the Maunder minimum. Although the exact level is still unclear, it was definitely lower than during the Dalton minimum of around 1800 and significantly below that of the current solar cycle #24. Claims of a moderate-to-high level of solar activity during the Maunder minimum are rejected with a high confidence level.