Characteristics of different groups of flare-CME in the minimum to rising phase of solar cycle 24
Coronal Mass Ejections are significant solar events that involve intense explosions of magnetic fields and mass particles out from the corona. As the hot plasma are brought by the solar wind into the Earth’s magnetosphere, geomagnetic storm is generated and causing malfunctions in telecommunication...
Main Authors: | N. Mohamad Ansor, Z.S. Hamidi, N.N.M. Shariff |
---|---|
Format: | Article |
Language: | English |
Published: |
Universiti Kebangsaan Malaysia
2023
|
Online Access: | http://journalarticle.ukm.my/21932/1/ST%2021.pdf |
Similar Items
-
High Time Resolution Observation of Solar Radio of A Group
Type III And U Burst Associated of Solar Flares Event
by: Hamidi, Z.S., et al.
Published: (2012) -
Solar Radio Burst Type II characteristics and Coronal Mass Ejections (CMEs) structure based on the presence of a moreton wave
by: Z.S. Hamidi,, et al.
Published: (2022) -
The Beginning Impulsive of Solar Burst Type IV Radio Emission Detection Associated with M Type Solar Flare
by: Hamidi, Z.S., et al.
Published: (2012) -
Modeling Solar Energetic Neutral Atoms from Solar Flares and CME-driven Shocks
by: Gang Li, et al.
Published: (2023-01-01) -
Can the Parker Solar Probe Detect a CME-flare Current Sheet?
by: Yuhao Chen, et al.
Published: (2023-01-01)