Minientradas

VICHAMA, de la Cultura Caral

VICHAMA, UN ENCUENTRO CON LA CIVILIZACIÓN AGROPESQUERA DE CARAL

Vichama (Végueta, Huaura) estuvo a punto de ser devorada por el avance urbano, pero la acción decidida de los responsables de la Zona Arqueológica Caral (ZAC), permitió preservar uno de los once sitios relacionados a la civilización más antigua de América.

El crecimiento urbano era el verdugo que cumpliría con la sentencia ordenada por la falta de memoria histórica: desaparecer de la faz de la tierra un espacio cultural de más de 136 hectáreas. Ese era el destino que le esperaba a Vichama (Végueta, Lima), cuando empezaron a erigirse las primeras construcciones modernas en la zona arqueológica.

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Ante la amenaza urbanística, los responsables de la Zona Arqueológica Caral (ZAC), Unidad Ejecutora 003 del Ministerio de Cultura, instaron a las autoridades locales a reubicar a los pobladores para que no dañen el espacio histórico. El acuerdo se concretó y, a partir de entonces, se abrió el camino para revelar los secretos milenarios del Perú antiguo.

Los estudios arqueológicos de la ZAC, dirigidos por la doctora Ruth Shady, demostrarían que los primeros pobladores de Végueta se asentaron durante el periodo Arcaico Tardío (3000 a 1800 a.C.), en la cadena de cerros Halconcillo. Ese sería el punto de partida de las construcciones piramidales de Vichama, la ciudad agropesquera que se erigió a finales de la civilización Caral, la más antigua de América.

“La sociedad de Vichama, por su ubicación, interactuó con otros asentamientos, tales como Supe (Barranca) y Santa (Áncash). Los intercambios comerciales y sociales fueron óptimos. Los productos marinos y agrícolas destacaron entre ellos”, explica el arqueólogo Aldemar Crispín, jefe de la ZAC sede Vichama.

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El investigador afirma que el apogeo agrícola se debió a uno de los hijos del dios Sol: Vichama. Los ecos de su historia mitológica se escuchan hasta hoy en los fértiles campos y en las orillas del Pacífico.

“Pachacámac celoso lo asesinó. De sus restos nacieron frutos y alimentos. La madre campesina lloró mucho y el Inti tuvo que hacer renacer a su hijo. En venganza, Pachacámac la mató. Vichama lo buscó, pero él huyó al valle de Lurín donde se sumergió al mar para siempre. La sed de venganza del semidiós fue tan grande que le pidió a su padre que convirtiera a los hombres en piedras y creara una nueva era”, detalla el agricultor Juan Cabrera, mientras vigila sus sembríos de maíz.

Los nuevos yungas que habitaron los arenales y llanos se organizaron bajo un sistema administrativo, político y social dirigido por una élite que hizo de sus construcciones un legado arqueológico.

Entre las 16 pirámides y edificaciones menores de la zona, resaltan el edificio Mayor, con una plaza circular y una secuencia de terrazas donde se encuentra el relieve de la mano con cuchillo y un salón ceremonial; Las Shicras, donde hay estatuillas humanas pintadas en barro no cocido y una huaca con representaciones pintadas del sol y de la luna; y Los Depósitos que alberga el relieve de un rostro humano pintado de rojo.

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También están los edificios de Las Ofrendas, Las Chakanas y Público Menor. Pero el monumento que atrae más miradas es Las Cornisas. Aquí existen dos plazas circulares y murales donde 24 personajes antropomorfos en alto relieve que realizan un baile ritual. Además de la imagen de un sapo con manos humanas y un rayo, símbolos que representan la conexión entre las divinidades y los pobladores de la ciudad milenaria.

Fuente: La República /Rumbos

Fecha de publicación: 29/05/2016

SKA Selecciona el diseño final del plato

SKA Selects The Final Design Of The SKA Dish

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An artist impression of the full SKA at night, with the selected Panel Space-frame supported Metal (PSM) SKA dish design in the foreground.
SKA Global Headquarters, UK – The Square Kilometre Array (SKA) Project has selected the design for its dish, opening up the way for the eventual production of hundreds of dishes that will make up the world’s largest radio telescope.

“This decision is a major milestone towards delivering the SKA,” said Alistair McPherson, Head of Project at SKA Organisation “Being able to “see” what the SKA dishes will look like for the first time is a big satisfaction for all involved.”

Three antenna concepts were built to be considered for the design of the SKA dish: DVA-1 in Canada, DVA-C in China, and MeerKAT-1 in South Africa. All three were constructed using different technology from the different partners, representing the very best in radio telescope dish technology currently available.

The consortium then presented the following designs for study:

An innovative Single Skin, Rim supported Composite (SRC) concept led by the National Research Council of Canada (NRC), along with SED Systems of Canada and RPC Composites of Australia.
An optimised Panel, Space-frame supported Metal (PSM) concept, led by a Shijiazhuang, China based team composed of JLRAT/CETC-54 along with their European partner, MT Mechatronics (MTM) of Mainz, Germany
A five-strong selection panel of engineering experts in the fields of composites, radio telescope antennas and systems engineering assessed both designs on a series of indicators including surface accuracy, feasibility of on-site manufacturing and ability to maintain structural integrity over long time-frames and made a unanimous recommendation that the Chinese PSM concept should be selected for the SKA dishes, a recommendation that was then approved by the SKA Dish Consortium Board.

DVA-1 prototype antenna built at NRC’s Dominion Radio Astrophysical Observatory (DRAO) just outside of Penticton, BC, Canada

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DVA-1 prototype antenna built at NRC’s Dominion Radio Astrophysical Observatory (DRAO) just outside of Penticton, BC, Canada
The SKA Dish Consortium, made up of institutes from Australia (who leads the consortium), Canada, China, Germany, Italy and South Africa is responsible for the design and verification of the dish that will make up SKA-mid, one of two SKA instruments. In its first phase of deployment (SKA1), SKA-mid will be initially composed of 133 15-metre diameter dishes providing a continuous coverage from 350 MHz to 14 GHz.

One of the greatest challenges faced by the consortium is the mass production of hundreds of these dishes, all with identical performance characteristics, and built to last and tolerate the harsh conditions of the remote arid areas in which they will operate for 50 years. Combined with achieving a large high precision collecting area at a competitive price, it’s a formidable technical and engineering challenge.

“We’re confident the selected design will perform well in the harsh conditions of the Karoo in South Africa and will deliver the precision that the scientific community needs to answer the questions they’re trying to solve” said Roger Franzen, SKA Dish Consortium Lead.

“The next step for us is to build and test a prototype at the South African site” he continued.

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Mr. Wang Feng, Vice Chairman of CETC54, inspects the first mould out of 66 that will be needed for SKA-P
The detailed design and manufacturing of such prototype, called SKA-P, is led by JLRAT/CETC54 in collaboration with the European companies MTM and Società Aerospaziale Mediterranea (SAM), and the Assembly, Integration and Verification of SKA-P will be done on site together with SKA SA team.

“We expect the installation of SKA-P on the ground to happen by spring 2017”, said Roger Franzen. “Once satisfied with its performance, the project will be in a good position to go to tender and issue the contract for the mass production of 133 dishes to make up SKA1-mid.”

Beyond the design of the dish structure, the consortium is also tasked with designing and testing optics, receivers and other elements of the dish. As part of that process, NRC continues its valuable contributions to single pixel feed (SPF) receivers/digitizers and cryogenic low noise amplifiers (LNAs).

About the SKA

The Square Kilometre Array (SKA) project is an international effort to build the world’s largest radio telescope, led by SKA Organisation. The SKA will conduct transformational science to improve our understanding of the Universe and the laws of fundamental physics, monitoring the sky in unprecedented detail and mapping it hundreds of times faster than any current facility.

The SKA is not a single telescope, but a collection of telescopes or instruments, called an array, to be spread over long distances. The SKA is to be constructed in two phases: Phase 1 (called SKA1) in South Africa and Australia; Phase 2 (called SKA2) expanding into other African countries, with the component in Australia also being expanded.

Already supported by 10 member countries – Australia, Canada, China, India, Italy, New Zealand, South Africa, Sweden, The Netherlands and the United Kingdom – SKA Organisation has brought together some of the world’s finest scientists, engineers and policy makers and more than 100 companies and research institutions across 20 countries in the design and development of the telescope. Construction of the SKA is set to start in 2018, with early science observations in 2020.

Mr. Wang Feng, Vice Chairman of CETC54, inspects the first mould out of 66 that will be needed for SKA-P

About the Design process

In 2013, the SKA Organisation sent out requests to research organisations and commercial partners around the world to help design the SKA. Eleven international teams – called consortia – were established and each tasked with designing a critical element of the project, with each consortium composed of partners who are leaders in their fields.