THE EFFECTS OF CORONAL HOLE EVOLUTION ON SOLAR WIND DYNAMICS AND GEOMAGNETIC DISTURBANCE
Solar corona as the outermost part of the Sun is constantly emanating solar wind consisting of charged particles. Coronal holes are rigidly rotating phenomena in the solar corona that are magnetically open to interplanetary space, which allow the solar wind particles to escape from the Sun. The stud...
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Main Author: | SULISTIANI (NIM: 20315003), SANTI |
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Format: | Theses |
Language: | Indonesia |
Online Access: | https://digilib.itb.ac.id/gdl/view/24205 |
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Institution: | Institut Teknologi Bandung |
Language: | Indonesia |
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