Noam Chomsky on the Big Questions (Part 4) | Closer To Truth Chats

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“La crítica de arte ha perdido totalmente su función” Benjamin H. D. Buchloh -Germany (1941)

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La Critríca de arte ha perdido totalmente su función El historiador del arte reflexiona sobre la  p intura en la era digital y la dictadura del  mercado Otros 11 Guardar Enviar por correo Imprimir IKER SEISDEDOS 20 MAR 2016 - 00:23 CET BERNARDO PÉREZ El profesor de Harvard Benjamin H. D. Buchloh (Colonia, 1941)   es uno de los más influyentes historiadores del arte del siglo XX. León de Oro en la Bienal de Venecia de 2007, fue exégeta de los primeros conceptualismos europeos antes de mudarse en los setenta desde Alemania Occidental a Estados Unidos, donde ha intervenido en la esfera pública del arte junto a   Rosalind Krauss, Yve-Alain Bois   y   Hal Foster,   coautores del esencial tratado   Arte desde 1900  (Akal)   y compañeros de la revista   October,   boletín de pensamiento crítico que, libre de publicidad, edita el   Massachussets Institute of Technology (MIT). En el grupo de los últimos mohicanos de la crítica, Buchloh se sitúa en la e
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Chaos & An Unpredictable Tomorrow --Peter Saltzstein finds that Chaos Theory yields unexpected philosophical results.

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Solar active regions consist of strongly magnetic sunspots and surrounding regions of more diffuse magnetic field.

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Solar active region as seen by the Helioseismic and Magnetic Imager on board the NASA Solar Dynamics Observatory. The dark circular regions are sunspots; these regions of strong magnetic field are dark as they are cool. The image of Earth … more Solar active regions consist of strongly magnetic sunspots and surrounding regions of more diffuse magnetic field. These regions are the origin of solar activity which controls space weather and causes beautiful phenomena such as aurora but in some cases also damage to satellites or power grids. Solar active regions are thought to be the result of magnetic flux concentrations - bundles of magnetic field lines - rising from deep in the solar interior and penetrating the surface. A team consisting of researchers from the Max Planck Institute for Solar System Research (MPS), The University of Göttingen, NorthWest Research Associates, and the High Altitude Observatory of the National Center for Atmospheric Research has now shown that these magnet
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