NO WEBCAST OR RECORDING WILL BE AVAILABLE

Opposite 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

The CESM Last Millennium Project: A Solar-Climate Connection?

Kinetic Simulations of Current Sheets for Different Stellar Magnetospheres