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Device for measuring observatory site astronomical seeing

A technology of seeing and observatories, which is applied in the field of devices for measuring seeing at observatory sites, and can solve problems such as inability to obtain seeing data, and the inability to describe turbulence changes by measuring atmospheric seeing at low temperatures

Pending Publication Date: 2019-07-30
YUNNAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI
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  • Summary
  • Abstract
  • Description
  • Claims
  • Application Information

AI Technical Summary

Problems solved by technology

However, in the existing technology, the atmospheric seeing at low temperature cannot describe the change of turbulence, making it impossible to obtain high-precision seeing data. Therefore, it is necessary to provide an improved device for measuring the seeing at the observatory site

Method used

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  • Device for measuring observatory site astronomical seeing
  • Device for measuring observatory site astronomical seeing
  • Device for measuring observatory site astronomical seeing

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Embodiment Construction

[0024] The implementation of the present application will be described in detail below with reference to the accompanying drawings and examples, so as to fully understand and implement the implementation process of how the present application uses technical means to solve technical problems and achieve technical effects.

[0025] A kind of device that this application provides for measuring the seeing degree of observatory site, refer to figure 1 and figure 2 A schematic block diagram of, in some embodiments, comprising:

[0026] Control module 1, pressure acquisition module 2, temperature acquisition module 3 and slight temperature difference acquisition module 4. The control module 1 can be an STM32 module: the chip used by this module is stm32f103c8t6; the pressure acquisition module can be an atmospheric pressure sensor BMP280, which can measure pressure and output corresponding signals; the temperature acquisition module can be a digital temperature sensor DS18B20, whic...

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Abstract

The application disclose a device for measuring observatory site astronomical seeing. The device comprises a control module, a pressure intensity collection module, a temperature collection module, and a micro-temperature difference collection module; an output end of the pressure intensity collection module is electrically connected with a first input end of the control module; an output end of the temperature collection module is electrically connected with the second input end of the control module; the output end of the micro-temperature difference collection module is electrically connected with a third input end of the control module; the pressure intensity collection module can be configured to measure the pressure intensity; the temperature collection module is configured to measure the average temperature between two points of the measured air; the micro-temperature difference collection module comprises an electric bridge unit, a differential amplification unit, an absolute value unit, a following unit and a filtering unit which are electrically connected in order; and the output end of the filtering unit is the output end of the micro-temperature difference collection module.

Description

technical field [0001] The application belongs to the field of electronic equipment, and in particular relates to a device for measuring the seeing degree of an observatory site. Background technique [0002] Among the various indicators of the observatory site, seeing is one of the most important indicators. For large telescopes that do not use adaptive optics, the angular diameter of the star image is determined by seeing. A 4m telescope placed on a site with a seeing degree of 2 arcseconds, compared with a 2m telescope placed on a site with a seeing degree of 1 arcsecond, has the same limiting magnitude, and the resolution of the latter is better high. Seeing is the brightness flickering, shape destruction, and position change of astrological images caused by the earth's atmosphere. Seeing is the total result of atmospheric influences at different altitudes. Generally, the atmosphere below 30m in height is called the ground layer, which can be sampled and observed wit...

Claims

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Application Information

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Patent Type & Authority Applications(China)
IPC IPC(8): G01M11/02G01D21/02
CPCG01M11/0228G01M11/0207G01D21/02
Inventor 丁旭王德清和寿圣常亮王传军伦宝利辛玉新范玉峰业凯
Owner YUNNAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI