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A non-contact measuring device for measuring the surface temperature of the primary mirror of a large-aperture solar telescope

A solar telescope, non-contact technology, applied in the field of temperature control of solar telescopes, can solve problems such as affecting the coating of the surrounding light-transmitting area, inability to fully reflect the temperature, and damage to the coating in the pasting area, achieving strong practicability and innovation. Small size, the effect of avoiding damage

Active Publication Date: 2017-10-20
INST OF OPTICS & ELECTRONICS - CHINESE ACAD OF SCI
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  • Abstract
  • Description
  • Claims
  • Application Information

AI Technical Summary

Problems solved by technology

However, this method not only cannot fully reflect the temperature of each area of ​​the mirror, but also may cause damage to the coating in the pasted area and even further affect the coating in the surrounding light-transmitting area.

Method used

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  • A non-contact measuring device for measuring the surface temperature of the primary mirror of a large-aperture solar telescope
  • A non-contact measuring device for measuring the surface temperature of the primary mirror of a large-aperture solar telescope
  • A non-contact measuring device for measuring the surface temperature of the primary mirror of a large-aperture solar telescope

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Embodiment Construction

[0044] The present invention will be further described below in conjunction with the accompanying drawings and specific embodiments.

[0045] like Figures 1 to 3 As shown, the basic idea of ​​the present invention is to provide a kind of non-contact measuring device for large aperture solar telescope primary mirror mirror surface temperature measurement, by primary mirror panel, air nozzle, ambient temperature sensor, air jet temperature sensor, total radiation It consists of 7 modules including sensor, anemometer and data processing module.

[0046] A possible implementation of a non-contact measuring device for the temperature measurement of the primary mirror of a large-aperture solar telescope, specifically, as Figure 4 Shown:

[0047] Among them, b-1 is a refrigerator, b-2 is a heat exchanger, b-3 is an electric heater, b-4 is a controller, b-5 is a fan, and b-6 is an air distribution box. The above six parts together constitute the temperature control system of the ...

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Abstract

The invention provides a non-contact measurement device for measuring the temperature of the main mirror surface of a large-diameter solar telescope, comprising a main mirror panel (1), an air nozzle (2), an ambient temperature sensor (3), and an air jet temperature sensor (4), a total radiation sensor (5), an anemometer (6) and a data processing module (7). During the working process of the solar telescope, the temperature rise of the primary mirror surface will cause the mirror seeing effect and the thermal deformation of the mirror surface, which greatly limits the performance of the telescope. The device can monitor the temperature of the primary mirror surface in real time, providing an important basis for the temperature control of the primary mirror surface of the solar telescope; at the same time, it also provides data for the analysis of mirror seeing effect and thermal deformation. Compared with the traditional contact temperature measurement device, the device can effectively avoid the damage to the mirror coating caused by the traditional device and the measurement error caused by the temperature sensor being exposed to solar radiation. In addition, the device has the advantages of simple structure, convenient operation, low cost, and strong practicability and innovation.

Description

technical field [0001] The invention relates to the field of solar telescope temperature control, in particular to a non-contact measuring device for measuring the temperature of the primary mirror of a large-aperture solar telescope. Background technique [0002] With the development of modern heliophysics research, the requirements for spatial, temporal and spectral resolutions required for the observation of solar surface activities have been continuously improved, and the aperture of solar telescopes has been continuously increased. At present, the study of solar physics has penetrated into the high-resolution observation of the fine structure of the solar surface, requiring the spatial resolution of the solar surface to reach 50-70km, which requires that the aperture of the corresponding solar telescope must reach 1m or larger. [0003] Due to the difficulty in manufacturing large-aperture sealed windows and the pressure birefringence effect, the traditional vacuum-type...

Claims

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Application Information

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Patent Type & Authority Patents(China)
IPC IPC(8): G01K13/00
Inventor 饶长辉刘洋毅顾乃庭
Owner INST OF OPTICS & ELECTRONICS - CHINESE ACAD OF SCI