International scientific conference
30 August - 2 September, 2005

Chromospheric and Coronal Magnetic Fields

Max Planck Institute for Solar System Research
Katlenburg-Lindau, Germany
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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.

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PDF Program and Abstract Book
PDF List of Talks
> Oral Presentation Download
> Social Program

Poster Download

PDF CCMag Poster A4 (856 KB)
PDF CCMag Poster A3 (1.49 MB)

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