Construction and Research of the Observation and Data Processing System for the Solar Hα High-Resolution Image
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Abstract
A receiving and processing terminal system for the solar Hα image is constructed and attached to the Solar Fine- Structure Telescope at the Yunnan Observatory for researching the physical processes and high-energy phenomena of solar flares. The high-resolution observed data and digitized results of the process of a solar flare can be acquired with the system, which is of great significance to monitoring and research of solar Hα active regions.
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