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March 1, 2005Open Access

simulation on Solar Type II Radio Bursts associated with Coronal Mass Ejections

J.I SAKAI T. Mori S. Saito

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Key Points

The aim is to understand the generation and transformation of waves associated with solar type II radio bursts.
Conducted simulations of solar radio bursts related to coronal mass ejections.
Analyzed wave transformations near shock fronts.
Examined the conversion of electrostatic Langmuir waves to electromagnetic waves.
Identified the generation of electrostatic Langmuir waves near the shock front.
Observed the conversion of Langmuir waves into extraordinary electromagnetic waves.
Highlighted the role of direct linear mode conversion in wave dynamics.

Implication

Simulation reveals electromagnetic wave conversions in radio bursts from coronal mass ejections, suggesting complex wave dynamics.

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Cite This Study

SAKAI et al. (2005) studied this question.

synapsesocial.com/papers/69cd7a4e5652765b073a749b https://doi.org/10.15099/00005761

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