| The solar X-EUV imaging telescope used to predict the space weather is under development in the Center for Space Science and Applied Research, Chinese Academy of Sciences. This instrument is a new solar storm surveillance and alert system, and the observed materials will be dedicated to the research of space weather prediction.This paper, aimed at imaging telescope's ground testing, designs a handily software with friendly interface in order to make data analysis on real time and multifunctional data display towards the solar X-EUV imaging telescope. With the help of the software, the telescope's system response analysis, image data process and image optimized process can be conveniently and rapidly realized.In the aspect of the system response, for different solar activity phenomenon, different thickness and material of the incidence window, filter, incidence modes, and etc. can be chosen on this software's interface. This paper calculates the acquired electron number in unit time in unit pixel of the CCD. The working waveband of the telescope can be rapidly calculated through the method of image display, the physics method and the realization for the inverse of the coronal plasma's temperature was discussed in this paper.In the aspect of image data process, the software has the function of directly read original data, can display the signal of the CCD on the screen, and conveniently realize the functions of multi-dimension display, analysis and statistics process of the data. For the space adaptability of the telescope, the image captured by CCD will be affected by the noise formed in structure modulation. This paper analyzes physical methods to eliminate noise, and makes noise filtering towards the image captured by the solar X-EUV imaging telescope. The software has the function of the pseudo color process for the need of the visualization of data analysis.This software plays a very important role in the process of developing and debugging the telescope. |
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