Solar radio burst type II and III with half wave dipole antenna / Farah Aqilah Mohd Pauzi
An investigation into the physics of solar radio burst type II was done to understand the frequency gap between its fundamental and harmonic emissions that happen as aftershocks of Coronal Mass Ejection (CME). Up until now, the evolution of type II and its associated coronal wave still remain a myst...
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| Format: | Thesis |
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2020
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| Online Access: | http://studentsrepo.um.edu.my/14059/1/Farah_Aqilah.pdf http://studentsrepo.um.edu.my/14059/2/Farah_Aqilah.pdf http://studentsrepo.um.edu.my/14059/ |
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