European Solar Telescope: Progress status

被引：61

作者：

Collados, M. ^{[1
]}

Bettonvil, F. ^{[2
]}

Cavaller, L. ^{[3
]}

Ermolli, I. ^{[4
]}

Gelly, B. ^{[5
]}

Perez, A. ^{[1
]}

Socas-Navarro, H. ^{[1
]}

Soltau, D. ^{[6
]}

Volkmer, R. ^{[6
]}

机构：

[1] Inst Astrofis Canarias, Tenerife 38205, Spain

[2] Univ Utrecht, Astron Inst, NL-3584 CC Utrecht, Netherlands

[3] Grantecan SA, Tenerife 38205, Spain

[4] Osserv Astron Roma, I-00040 Rome, Italy

[5] CNRS UPS 853 THEMIS, Tenerife 38205, Spain

[6] Kiepenheuer Inst Sonnenphys, D-79100 Freiburg, Germany

来源：

ASTRONOMISCHE NACHRICHTEN | 2010年 / 331卷 / 06期

关键词：

instrumentation: adaptive optics; instrumentation: high angular resolution; instrumentation: interferometers; instrumentation: polarimeters; instrumentation: spectrographs; telescopes; POLARIZATION;

D O I：

10.1002/asna.201011386

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, the present status of the development of the design of the European Solar Telescope is described. The telescope is devised to have the best possible angular resolution and polar metric performance. maximizing the throughput of the whole system. To that aim, adaptive optics and multi-conjugate adaptive optics are integrated in the optical path. The system will have the possibility to correct for the diurnal variation of the distance to the turbulence layers, by using several deformable mirrors, conjugated at different heights. The present optical design of the telescope distributes the optical elements along the optical path in such a way that the instrumental polarization induced by the telescope is minimized and independent of the solar elevation and azimuth. This property represents a large advantage for polarimetric measurements. The ensemble of instruments that are planned is also presented. (C) 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

引用

页码：615 / 619

页数：5

共 50 条

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