|High-accuracy determination of the temperatures in the upper atmosphere of the sun, with the ESA-Dresden Radio Telescope
|Chen Xi, Author
|ISU Individual Project
|Illkirch-Graffenstaden (France) : International Space University, 2018
|1 electronic resource (33 p.) / col. ill.
|Includes bibliographical references
|The ESA-Dresden Radio Telescope, operates within a range of 10-12 GHz, located at the International Space University(ISU), aim to measure the height of the sun's temperature above the chromosphere and the photosphere. This report describes all observation and analyzing process, which must be followed to obtain accurate results, the temperature of the sun. Most of the efforts are dedicated in optimizing the application of overall accuracy and stability of the improvement of the hardware and software radio telescope. After one month of observational studies, the calculated average temperature of the sun is XX K. The report also analyzed other factors, and climate conditions did not affect the sun's observations significantly. The report finally gives some Suggestions on the problems encountered in the process of the project.
|ISU program :
|Master of Space Studies
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