Interplanetary Consequences of a Large CME
M. Lahkar, P. K. Manoharan, K. Mahalakshmi, K. Prabhu, G. Agalya, S., Shaheda Begum, P. Revathi
TL;DR
This paper investigates how a large coronal mass ejection from 2003 affected interplanetary space, emphasizing the role of internal magnetic energy in determining its consequences.
Contribution
It combines multiple observational methods to analyze CME propagation and highlights the importance of magnetic energy in its interplanetary impact.
Findings
CME propagation speed varies with magnetic energy
Interplanetary scintillation images reveal CME structure
Magnetic energy influences CME's space weather effects
Abstract
We analyze a coronal mass ejection (CME) which resulted from an intense flare in active region AR486 on November 4, 2003. The CME propagation and speed are studied with interplanetary scintillation images, near-Earth space mission data, and Ulysses measurements. Together, these diverse diagnostics suggest that the internal magnetic energy of the CME determines its interplanetary consequences.
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