Aims:
Study the global properties of the magnetic flux tubes forming active regions.
This provides important informations on:
the origin of these flux tubes (formation,and transport in the convective
zone)
the "boundary conditions" for flares and coronal mass ejections.
Lòpez Fuentes, M.C., Démoulin,
P., Mandrini, C.H., Pevtsov, A.A.,
van Driel-Gesztelyi, L.,
Magnetic Twist and Writhe of Actives Regions
2003, A&A, 397, 305 PS
gzip
van Driel-Gesztelyi L., Malherbe
J.M., Démoulin P.,
Emergence of a U-loop-sub-photospheric link
between solar active regions
2000, A&A, 364, 845 PS
gzip
López Fuentes M., Démoulin
P., Mandrini C.H., van Driel-Gesztelyi L.,
The Counter-kink Rotation of a Non-Hale Active
Region
2000, ApJ, 544, 540 PS gzip
Deng Y.Y., Schmieder B., Mandrini
C.H., Khan J.I., Démoulin P., Rudawy P.,
The evolution from birth to decay of a
short-lived active region
1999, A&A, 349, 927 PS gzip