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Der Teufel ist in der russischen Literatur vielfach dargestellt worden, und seine Bilder und Funktionen ändern sich durch die Jahrhunderte – in Entsprechung zum Wandel der Epochen und literarischen Moden. In den Teufelsvorstellungen mischen sich volkstümlich animistische Elemente mit den biblischen Konzepten von Teufeln und Dämonen. Aus beiden Reservoirs schöpft die Literatur, die z. T. die naive Teufelsgläubigkeit verspottet, die sich aufgeklärt gebenden Skeptiker aber auch gerne mit Teufelserscheinungen schreckt. Der Teufel ist ein zentrales Motiv der russischen Literatur, dessen Geschichte nachzuerzählen, einen ganz zentralen Strang der russischen Literatur nachzuerzählen heißt – sub specie diaboli.
Auch wenn er schon lange vor den Romantikern – allen voran Nikolaj Gogol’ – einen prominenten Platz in der russischen Literatur inne hatte, mischen sich seitdem volkstümliche Vorstellungen mit dem biblischen Erbe. Im Volk sind Teufelsvorstellungen bis heute populär, die gebildeten Schichten zeigen sich eher skeptisch, weshalb die realistische Literatur – mit der großen Ausnahme Fedor Dostoevskij – den Teufel eher mied, die Modernisten gestalteten ihn dafür umso lieber. Einen Höhepunkt erreicht er bei Michail Bulgakov. Zeitgenossen fehlt häufig der religiöse Subtext.
The presence of a low-to mid-latitude interhemispheric hydrologic seesaw is apparent over orbital and glacial-interglacial timescales, but its existence over the most recent past remains unclear. Here we investigate, based on climate proxy reconstructions from both hemispheres, the inter-hemispherical phasing of the Intertropical Convergence Zone (ITCZ) and the low-to mid-latitude teleconnections in the Northern Hemisphere over the past 2000 years. A clear feature is a persistent southward shift of the ITCZ during the Little Ice Age until the beginning of the 19th Century. Strong covariation between our new composite ITCZ-stack and North Atlantic Oscillation (NAO) records reveals a tight coupling between these two synoptic weather and climate phenomena over decadal-to-centennial timescales. This relationship becomes most apparent when comparing two precisely dated, high-resolution paleorainfall records from Belize and Scotland, indicating that the low-to mid-latitude teleconnection was also active over annual-decadal timescales. It is likely a combination of external forcing, i.e., solar and volcanic, and internal feedbacks, that drives the synchronous ITCZ and NAO shifts via energy flux perturbations in the tropics.
Tolstoj, Lev Nikolaevic^
(1999)
Theater und Wandel
(2003)
We determine the metallicity distribution function (MDF) of the Galactic halo by means of a sample of 1638 metal-poor stars selected from the Hamburg/ESO objective-prism survey (HES). The sample was corrected for minor biases introduced by the strategy for spectroscopic follow-up observations of the metal-poor candidates, namely "best and brightest stars first". Comparison of the metallicities [Fe/H] of the stars determined from moderate-resolution (i.e., R similar to 2000) follow-up spectra with results derived from abundance analyses based on high-resolution spectra (i.e., R > 20 000) shows that the [Fe/H] estimates used for the determination of the halo MDF are accurate to within 0.3 dex, once highly C-rich stars are eliminated. We determined the selection function of the HES, which must be taken into account for a proper comparison between the HES MDF with MDFs of other stellar populations or those predicted by models of Galactic chemical evolution. The latter show a reasonable agreement with the overall shape of the HES MDF for [Fe/H] > -3.6, but only a model of Salvadori et al. (2007) with a critical metallicity for low-mass star formation of Z(cr) = 10(-3.4) Z(circle dot) reproduces the sharp drop at [Fe/H] similar to -3.6 present in the HES MDF. Although currently about ten stars at [Fe/H] < -3.6 are known, the evidence for the existence of a tail of the halo MDF extending to [Fe/H] similar to -5.5 is weak from the sample considered in this paper, because it only includes two stars [Fe/H] < -3.6. Therefore, a comparison with theoretical models has to await larger statistically complete and unbiased samples. A comparison of the MDF of Galactic globular clusters and of dSph satellites to the Galaxy shows qualitative agreement with the halo MDF, derived from the HES, once the selection function of the latter is included. However, statistical tests show that the differences between these are still highly significant.
To calibrate delta O-18 time-series from speleothems in the eastern Indian summer monsoon (ISM) region of India, and to understand the moisture regime over the northern Bay of Bengal (BoB) we analyze the delta O-18 and delta D of rainwater, collected in 2007 and 2008 near Cherrapunji, India. delta D values range from + 18.5 parts per thousand to 144.4 parts per thousand, while delta O-18 varies between +0.8 parts per thousand and 18.8 parts per thousand. The Local Meteoric Water Line (LMWL) is found to be indistinguishable from the Global Meteoric Water Line (GMWL). Late ISM (September-October) rainfall exhibits lowest delta O-18 and delta D values, with little relationship to the local precipitation amount. There is a trend to lighter isotope values over the course of the ISM, but it does not correlate with the patterns of temperature and rainfall amount delta O-18 and delta D time-series have to be interpreted with caution in terms of the 'amount effect' in this subtropical region. We find that the temporal trend in delta O-18 reflects increasing transport distance during the ISM, isotopic changes in the northern BoB surface waters during late ISM, and vapor re-equilibration with rain droplets. Using an isotope box model for surface ocean waters, we quantify the potential influence of river runoff on the isotopic composition of the seasonal freshwater plume in the northern BoB. Temporal variations in this source can contribute up to 25% of the observed changes in stable isotopes of precipitation in NE India. To delineate other moisture sources, we use backward trajectory computations and find a strong correlation between source region and isotopic composition. Palaeoclimatic stable isotope time-series from northeast Indian speleothems likely reflect changes in moisture source and transport pathway, as well as the isotopic composition of the BoB surface water, all of which in turn reflect ISM strength. Stalagmite records from the region can therefore be interpreted as integrated measures of the ISM strength.
Andrej Tarkovskij ist es gelungen, sich mit einem relativ kleinen Oeuvre in die Filmgeschichte einzuschreiben, obwohl fast alle seine Filme als schwer verständlich gelten. Legenden ranken sich um sie. Die Protokollierung des Films Stalker soll der intensiveren wissenschaftlichen Erforschung eine verlässliche Grundlage bieten. Das Nachwort untersucht das Verhältnis des Films zu der literarischen Vorlage und stellt ihn in russische Traditionen. Dabei werden einige nicht nur in Deutschland populäre Legenden berichtigt.
Eine Diskussion des Kitsch-Begriffs beschreibt diesen u.a. als das Bewusstsein, ein Werk mit einem Maßstab bewerten zu muessen, der nicht der eigene ist. Kitsch wird als (emotionale) Zumutung erlebt. In diesem Sinne erscheint der Film "Kljatva" ebenso als Kitsch wie der Band mit Erzaehlungen ueber Feliks Dzerzinski - zumindest heute, d.h. mit historischem Abstand.
Solzenicyn, Aleksandr
(2000)