Disturbance of Pre-existing Magnetic Polarities Prior to Subsequent Emergence of Magnetic Flux in Close Proximity


Georgios Chintzoglou, University Corporation for Atmospheric Research, Boulder, CO, United States, Matthias Rempel, National Center for Atmospheric Research, High Altitude Observatory, Boulder, United States and Chun Ming Mark Cheung, CSIRO Astronomy and Space Science Geraldton, Perth, Australia
Back to: Evolution and Instability of Coronal Magnetic Structures Leading to the Onset of Solar Eruptions I