Abstract
Mode conversion occurs when a wave passes through a region where the sound and Alfvén speeds are equal. At this point there is a resonance, which allows some of the incident wave to be converted into a different mode. We study this phenomenon in the vicinity of a twodimensional, coronal null point. As a wave approaches the null it passes from low- to high-β plasma, allowing conversion to take place. We simulate this numerically by sending in a slow magnetoacoustic wave from the upper boundary; as this passes through the conversion layer a fast wave can clearly be seen propagating ahead. Numerical simulations combined with an analytical WKB investigation allow us to determine and track both the incident and converted waves throughout the domain.
Original language | English |
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Pages | 752-755 |
Number of pages | 4 |
DOIs | |
Publication status | Published - 23 Apr 2009 |
Event | 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St Andrews, St Andrews, United Kingdom Duration: 21 Jul 2008 → 25 Jul 2008 |
Conference
Conference | 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun |
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Country/Territory | United Kingdom |
City | St Andrews |
Period | 21/07/08 → 25/07/08 |
Keywords
- Magnetohydrodynamics
- Sun: corona
- Sun: oscillations