1,065 research outputs found

    Sempronius Marcellinus Sírköve Savariában

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    Magna Mater in wandelndem Wirkungskreis

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    In the poetry of the late Republic and the age of Augustus, a gradual expansion and Romanisation of the role of Magna Mater can be observed. In Catullus, she appears only as a goddess from Asia Minor linked to Attis’ repulsive act. In Lucretius, Cybele is identical with Rhea, which remarkably changes her position as she becomes the mother of all Olympian gods. In Vergil, in addition to being the mother of all gods, she is also the Chief Goddess of the Trojans, who plays an active role in shaping Aeneas’ fate. The most thorough picture of the Goddess is provided by Ovid, who covers every detail of the cult, placing emphasis on embracing the cult. He goes to great lengths to attribute Roman origin to its apparently foreign features, i.e., he tries to Romanise the already embraced cult as much as possible. All this must have taken place under the aegis of and in accordance with Augustus’ religious policy

    Grave relief of Sempronius Marcellinus in Savaria

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    The grave relief of Sempronius Marcellinus in Savaria does not show the scene of abreptio Helenae — as thinks Z. Kádár — but rather the painful moment of Eriphyle’s fateful decision followed by Amphiaraus’s leave (profectio). The closest conceptual analogy of the scene can be found on the Phaedra-sarcophagus with the difference that the fateful decision is made by the man there, not by the woman. Instead of the multi-figure scene of the sarcophagi here the three-figure composition, together with the figures in the background, can compress the entire story, enabling a complex semantic interpretation. This meaning is fateful separation and praise of the deceased person. Sempronius Marcellinus, who had ordered the tombstone, placed himself in the role of Amphiaraus while his wife in that of Eriphyle. But the representation of their relationship is obviously not the expression of betrayal but of pain felt over eternal separation

    Long duration thermal hard X-ray sources observed in two eruptive flares

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    We present observations of two eruptive flares on 17 of December 2006 (C1.9) and 19 of May 2007 (B9.7) which had good coverage with both Hinode and RHESSI. In these flares we see a long lived, gradual thermal hard X-ray source of low emission measure and, relative to the loops observed with GOES and XRT, high temperature. The lack of a non-thermal hard X-ray component and impulsive behaviour is inconsistent with electron beam driven chromospheric evaporation
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