Abstract
The study of the structure of the active region in triggering various classes of solar flare events is necessary to understand the relationship between the magnetic field and solar activity. This association has been the most interesting topic among researchers for nearly a century due to the reason that the Sun is not a stationary object and can cause changes in the magnetic complexity in the active region. These changes will lead to a variety form of solar flares phenomenon and also the amount of magnetic energy that will be released per day. Generally, most previous studies indicated that solar flares event is closely related to the large active region. Therefore, the structure of the magnetic class in the active region that triggered the evolution of powerful solar flares was determined as the first aim of this study
Metadata
Item Type: | Thesis (Masters) |
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Creators: | Creators Email / ID Num. Tengku Affendi, Tengku Nur Ain UNSPECIFIED |
Contributors: | Contribution Name Email / ID Num. Thesis advisor Hamidi, Zety Sharizat UNSPECIFIED |
Subjects: | Q Science > QC Physics > Atomic physics. Constitution and properties of matter |
Divisions: | Universiti Teknologi MARA, Shah Alam > Faculty of Applied Sciences |
Programme: | Master of Science |
Keywords: | Active region, magnetic class, solar flare, climate change |
Date: | 2024 |
URI: | https://ir.uitm.edu.my/id/eprint/106834 |
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