Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol

Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol

The Moreton wave (also known as flare wave) has been extensively studied in the hope of explaining the relation between solar flare, Coronal Mass Ejections (CMEs) and Solar Radio Burst Type II (SRBT II) phenomena. It is interpreted as an intersection of coronal Magneto-hydrodynamic (MHD) fast mode s...

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Main Author: Zainol, Nur Hidayah
Format: Thesis
Language:English
Published: 2019
Online Access:https://ir.uitm.edu.my/id/eprint/86115/1/86115.pdf
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spelling my-uitm-ir.861152024-10-02T02:11:29Z Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol 2019 Zainol, Nur Hidayah The Moreton wave (also known as flare wave) has been extensively studied in the hope of explaining the relation between solar flare, Coronal Mass Ejections (CMEs) and Solar Radio Burst Type II (SRBT II) phenomena. It is interpreted as an intersection of coronal Magneto-hydrodynamic (MHD) fast mode shock wave and solar chromosphere. It is well known that the occurrence of CME is always associated with both solar flare and SRBT II. Furthermore, SRBT II is also originated from the MHD fast mode shock wave theory. Previous research showed that Moreton wave constantly associated with solar flare event. 2019 Thesis https://ir.uitm.edu.my/id/eprint/86115/ https://ir.uitm.edu.my/id/eprint/86115/1/86115.pdf text en public masters Universiti Teknologi MARA (UiTM) Faculty of Applied Sciences
institution Universiti Teknologi MARA
collection UiTM Institutional Repository
language English
description The Moreton wave (also known as flare wave) has been extensively studied in the hope of explaining the relation between solar flare, Coronal Mass Ejections (CMEs) and Solar Radio Burst Type II (SRBT II) phenomena. It is interpreted as an intersection of coronal Magneto-hydrodynamic (MHD) fast mode shock wave and solar chromosphere. It is well known that the occurrence of CME is always associated with both solar flare and SRBT II. Furthermore, SRBT II is also originated from the MHD fast mode shock wave theory. Previous research showed that Moreton wave constantly associated with solar flare event.
format Thesis
qualification_level Master's degree
author Zainol, Nur Hidayah
spellingShingle Zainol, Nur Hidayah
Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol
author_facet Zainol, Nur Hidayah
author_sort Zainol, Nur Hidayah
title Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol
title_short Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol
title_full Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol
title_fullStr Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol
title_full_unstemmed Effects of the Moreton waves on the structure of Coronal Mass Ejections Events (CMEs) based on solar radio burst type II (SRBT II) characteristics / Nur Hidayah Zainol
title_sort effects of the moreton waves on the structure of coronal mass ejections events (cmes) based on solar radio burst type ii (srbt ii) characteristics / nur hidayah zainol
granting_institution Universiti Teknologi MARA (UiTM)
granting_department Faculty of Applied Sciences
publishDate 2019
url https://ir.uitm.edu.my/id/eprint/86115/1/86115.pdf
_version_ 1818587942666371072

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