International scientific conference |
30 August - 2 September, 2005 |
Chromospheric and Coronal Magnetic Fields |
Max Planck Institute for Solar System Research |
Katlenburg-Lindau, Germany |
|
|
Start Page
Coronal loops, plasma eruption and high energy particles from the Sun imply that the coronal dynamics are controlled by the magnetic field. Motion in the photosphere creates currents and sites of reconnection in the chromosphere and corona. Understanding the extent to which these currents and the surrounding magnetic fields can be measured directly and/or through comparison with modelling is a key goal of the workshop.
Poster Download
Scientific Organizing Committee
Sami Solanki (Chair), Bernhard Fleck, Sarah Gibson, Davina Innes, Franz Kneer, Tetsuya Magara, Valery Nakariakov, Eric Priest, Takashi Sakurai, Javier Trujillo Bueno, Stephen White
|
Coronal loops, plasma eruption and high energy particles from the Sun imply that the coronal dynamics are controlled by the magnetic field. Motion in the photosphere creates currents and sites of reconnection in the chromosphere and corona. Understanding the extent to which these currents and the surrounding magnetic fields can be measured directly and/or through comparison with modelling is a key goal of the workshop.
