New Generation Solar Telescope of Operative Predictions

被引：4

作者：

Peshcherov, V. S. ^{[1
]}

Grigor'ev, V. M. ^{[1
]}

Svidskii, P. M. ^{[2
]}

Bevzov, A. N. ^{[3
]}

Budnikov, K. I. ^{[3
]}

Vlasov, S. V. ^{[3
]}

Zotov, A. A. ^{[3
]}

Kotov, V. N. ^{[3
]}

Kitov, A. K. ^{[1
]}

Lubkov, A. A. ^{[3
]}

Lylov, S. A. ^{[3
]}

Perebeinos, S. V. ^{[1
]}

机构：

[1] Russian Acad Sci, Inst Solar Terr Phys, Siberian Branch, Ul Lermontova 126,POB 291, Irkutsk 664033, Russia

[2] Fedorov Inst Appl Geophys, Moscow 129128, Russia

[3] Russian Acad Sci, Inst Automat & Electrometry, Siberian Branch, Novosibirsk 630090, Russia

来源：

OPTOELECTRONICS INSTRUMENTATION AND DATA PROCESSING | 2013年 / 49卷 / 06期

关键词：

telescope; automated control system; measurements of LMF; the Sun; magnetogram;

D O I：

10.3103/S8756699013060071

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The functional and metrological characteristics of a new solar telescope designed to obtain quantitative data on large-scale magnetic fields (LMF) of the Sun are considered. The full automation of measurements, the application of CCD matrices in image scanning and spectra recording systems, and the optical diagram corresponding to the main purpose of the telescope significantly increased the efficiency, quality, and accuracy of measurements of the LMF and expanded the range of tasks in comparison with existing telescopes. The developed automated system of telescope control, measuring system, and software for real-time processing of measurement results make it possible to obtain LMF magnetograms with the required accuracy for about 15 min.

引用

页码：578 / 584

页数：7

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