Low energetic events

Aims:Use these non-spectacular events to understand:
                    - the plausible link between coronal heating and flares.
                    - some basic physical mechanisms (e.g. magnetic reconnection)

Mandrini C.H., Démoulin P., Schmieder B., Deng Y.Y., Rudawy P.,
                 The role of bald patches in chromospheric events,
         2002, A&A, 391, 317    PDF
Fletcher L., López Fuentes M., Mandrini C.H., Schmieder B., Démoulin P.,
                   Mason H.E., Nitta N.,
                 A Relationship Between Transition Region Brightenings,
                         Abundances, and Magnetic Topology,
         2001, Solar Physics,  203, 255    PS gzip
Bentley R.D., Klein K.-L., van Driel-Gesztelyi L., Démoulin  P., Trottet G., Tassetto P., Marty G.,
                 Magnetic Activity associated with Radio Noise Storms,
         2000, Solar Physics 193, 227
Rovira M., Schmieder B., Démoulin P., Simnett G.M.,  Hagyard M.J., et al.
                 Bright Points and Subflares in Ultraviolet Lines and in X-rays,
         1999, ApJ 510, 474   PS gzip
Mandrini, C.H., Démoulin, P., van Driel-Gesztelyi, L., Schmieder, B., Cauzzi, G., Hofmann, A.,
                 3D Magnetic Reconnection at an X-ray Bright Point,
         1996, Solar Physics 168, 115   PDF