4 resultados para Temps de conduction

em CentAUR: Central Archive University of Reading - UK


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The Arthurian world of Culhwch and Olwen initially appears as a resolutely masculine, warrior-based society with little or no place for women. As a rule, the names of the mothers of the many characters remain unmentioned, and even the young hero clearly had no idea of his family ties on his mother’s side. It comes as news to him that Arthur is his cousin. The Arthurian world is equally afflicted with a form of wilful amnesia of the existence of relatives on the distaff side, allowing the giant Ysbaddaden to victimise Custennin and his family with impunity. The hair-cutting ritual represents an intrusion of female memory and a reminder of the biological imperative of reproduction, which means that in order to survive, Arthur’s clan has to be prepared to face destruction.

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The problem of heat conduction in one-dimensional piecewise homogeneous composite materials is examined by providing an explicit solution of the one-dimensional heat equation in each domain. The location of the interfaces is known, but neither temperature nor heat flux are prescribed there. Instead, the physical assumptions of their continuity at the interfaces are the only conditions imposed. The problem of two semi-infinite domains and that of two finite-sized domains are examined in detail. We indicate also how to extend the solution method to the setting of one finite-sized domain surrounded on both sides by semi-infinite domains, and on that of three finite-sized domains.

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The fair weather atmospheric electrical current (Jz) couples the ionosphere to the lower atmosphere and thus provides a route by which changes in solar activity can modify processes in the lower troposphere. This paper examines the temporal variations and spectral characteristics of continuous measurements of Jz conducted at the Wise Observatory in Mitzpe-Ramon, Israel (30°35′ N, 34°45′ E), during two large CMEs, and during periods of increased solar wind density. Evidence is presented for the effects of geomagnetic storms and sub-storms on low latitude Jz during two coronal mass ejections (CMEs), on 24–25th October 2011 and 7–8th March 2012, when the variability in Jz increased by an order of magnitude compared to normal fair weather conditions. The dynamic spectrum of the increased Jz fluctuations exhibit peaks in the Pc5 frequency range. Similar low frequency characteristics occur during periods of enhanced solar wind proton density. During the October 2011 event, the periods of increased fluctuations in Jz lasted for 7 h and coincided with fluctuations of the inter-planetary magnetic field (IMF) detected by the ACE satellite. We suggest downward mapping of ionospheric electric fields as a possible mechanism for the increased fluctuations.