Extending the concept of separatrices to QSLs for magnetic reconnection
Magnetic reconfiguration before the X 17 Solar flare of October 28 2003
QUANTITATIVE LINK BETWEEN SOLAR EJECTA AND INTERPLANETARY MAGNETIC CLOUDS: MAGNETIC HELICITY
Reorganization of the Solar Corona Following a C4.7 Flare
Brightening Event in Halpha and Soft X-Ray on May 18, 1994
The smallest source region of an interplanetary magnetic cloud: A mini-sigmoid
Active Region Helicity Evolution and Related Coronal Mass Ejection Activity
3-D Magnetic Configurations for Filaments and Flares: The Role of "Magnetic Dips" and "Bald Patches"