NO WEBCAST OR RECORDING WILL BE AVAILABLEEnergy transport by kink waves in the solar atmosphere
NO WEBCAST OR RECORDING WILL BE AVAILABLEA simulation of solar convective dynamo: self-consistent maintenance of the solar differential rotation and emerging flux
NO WEBCAST OR RECORDING WILL BE AVAILABLEOpposite polarity and convective flows in simulated sunspot penumbra: comparison with observations
NO HAO COLLOQUIUM JUNE 11
Stellar evolution beyond the standard picture
NO WEBCAST OR RECORDING WILL BE AVAILABLE FOR THIS PRESENTATION
Do we understand sunquakes?
Reconnection of an emerging flux region with a magnetic dome topology
The Role of H2 in the Solar Atmosphere
How Meridional Flow Variations May Save Us from the Next Maunder Minimum
MAVEN: A mission to investigate the upper atmosphere of Mars
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