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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Bibliographic Details
Main Author: SULISTIANI (NIM: 20315003), SANTI
Format: Theses
Language:Indonesia
Online Access:https://digilib.itb.ac.id/gdl/view/24205
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Institution: Institut Teknologi Bandung
Language: Indonesia