Chinese Academy of Sciences, National Development and Reform Commission and the Xinjiang Uygur Autonomous Region will unite together to construct a large all-movable radio telescope which has an aperture of 110m diameter in the county of Qitai. It will be the largest all-movable radio telescope on the ground to achieve the most advanced level in the world after it is put into use. Yet if such large radio telescope is built, the most prominent problems from the structure techniques are listed as follows. There are several improper points in the conventional structure style. Only the gravity load seriously reduces the reflector surface precision (which is called as RMS for short, Root Mean Square) and restricts its performance. Meanwhile, many kinds of upwind profiles cause complicated wind pressure distribution to reflector surface. Moreover, non-uniform temperature deformation caused by solar effect inevitably affects the RMS surface, especially solar cooker problem in the secondary reflector because of the electromagnetic wave focusing also should be paid attention to.
Les informations fournies dans la section « Synopsis » peuvent faire référence à une autre édition de ce titre.
Associate professor, School of Civil Engineering at Chang’an University. Mainly engaged in the following researches: first - research on Structural Technology of Large Aperture All-Movable Telescope Structures; second - Extreme Temperature Field Analysis and Precision Control of Inflatable Antenna Structure.
Les informations fournies dans la section « A propos du livre » peuvent faire référence à une autre édition de ce titre.
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Chinese Academy of Sciences, National Development and Reform Commission and the Xinjiang Uygur Autonomous Region will unite together to construct a large all-movable radio telescope which has an aperture of 110m diameter in the county of Qitai. It will be the largest all-movable radio telescope on the ground to achieve the most advanced level in the world after it is put into use. Yet if such large radio telescope is built, the most prominent problems from the structure techniques are listed as follows. There are several improper points in the conventional structure style. Only the gravity load seriously reduces the reflector surface precision (which is called as RMS for short, Root Mean Square) and restricts its performance. Meanwhile, many kinds of upwind profiles cause complicated wind pressure distribution to reflector surface. Moreover, non-uniform temperature deformation caused by solar effect inevitably affects the RMS surface, especially solar cooker problem in the secondary reflector because of the electromagnetic wave focusing also should be paid attention to. 56 pp. Englisch. N° de réf. du vendeur 9783659129056
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -Chinese Academy of Sciences, National Development and Reform Commission and the Xinjiang Uygur Autonomous Region will unite together to construct a large all-movable radio telescope which has an aperture of 110m diameter in the county of Qitai. It will be the largest all-movable radio telescope on the ground to achieve the most advanced level in the world after it is put into use. Yet if such large radio telescope is built, the most prominent problems from the structure techniques are listed as follows. There are several improper points in the conventional structure style. Only the gravity load seriously reduces the reflector surface precision (which is called as RMS for short, Root Mean Square) and restricts its performance. Meanwhile, many kinds of upwind profiles cause complicated wind pressure distribution to reflector surface. Moreover, non-uniform temperature deformation caused by solar effect inevitably affects the RMS surface, especially solar cooker problem in the secondary reflector because of the electromagnetic wave focusing also should be paid attention to.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 56 pp. Englisch. N° de réf. du vendeur 9783659129056
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Taschenbuch. Etat : Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Chinese Academy of Sciences, National Development and Reform Commission and the Xinjiang Uygur Autonomous Region will unite together to construct a large all-movable radio telescope which has an aperture of 110m diameter in the county of Qitai. It will be the largest all-movable radio telescope on the ground to achieve the most advanced level in the world after it is put into use. Yet if such large radio telescope is built, the most prominent problems from the structure techniques are listed as follows. There are several improper points in the conventional structure style. Only the gravity load seriously reduces the reflector surface precision (which is called as RMS for short, Root Mean Square) and restricts its performance. Meanwhile, many kinds of upwind profiles cause complicated wind pressure distribution to reflector surface. Moreover, non-uniform temperature deformation caused by solar effect inevitably affects the RMS surface, especially solar cooker problem in the secondary reflector because of the electromagnetic wave focusing also should be paid attention to. N° de réf. du vendeur 9783659129056
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Taschenbuch. Etat : Neu. Key technologies of Large Aperture Fully-Steerable Antenna Structure | Yan Liu (u. a.) | Taschenbuch | 56 S. | Englisch | 2017 | LAP LAMBERT Academic Publishing | EAN 9783659129056 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu. N° de réf. du vendeur 109417557
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