DELAY TIMES BETWEEN GEOEFFECTIVE SOLAR DISTURBANCES AND GEOMAGNETIC INDICES Y. D. PARK 1, Y. -J. MOON 1, I. S. KIM 2, H. S. YUN 3 1.Korea Astronomy Observatory,
Low-Coronal and Coronagraphic Images: Their Complementary Roles in Understanding Geo-Effective Eruptions N. V. Nitta, Lockheed Martin Solar and Astrophysics.
Energy partition during initial stages of the CME
SEP Data Analysis and Data Products for EMMREM Mihir I. Desai & Arik Posner Southwest Research Institute San Antonio, Texas Mihir I. Desai & Arik Posner.
Relationships between flares and CMEs
Photospheric Sources of Very Fast (>1100km/s) Coronal Mass Ejections Recent studies show that only very fast CMEs (> 1100 km/s) are capable of producing.
