24 Oct 2001 A Cool, Dense Flare T. S. Bastian 1, G. Fleishman 1,2, D. E. Gary 3 1 National Radio Astronomy Observatory 2 Ioffe Institute for Physics and.
Coronal expansion and solar wind The large solar corona Coronal and interplanetary temperatures Coronal expansion and solar wind The heliosphere Origin.
11 February 2000Genova (I)1 ESA Space Environment & Effects Analysis Section Space Radiation Environment P. Nieminen, ESA/ESTEC, The Netherlands Overview.
AGU Dec 2000 The Structure and Evolution of a Sigmoid Observed During Whole Sun Month 3 Lyndsay Fletcher Sarah Gibson, and the WSM3 sigmoid structure working.
A Presentation to the SHINE ’02 Workshop by J.G. Luhmann (August 19, 2002) CME initiation: A zoo not an animal (Images from the on-line CDAW CME catalogue.
A Presentation to the SHINE ’02 Workshop by J.G. Luhmann (August 19, 2002) CME initiation:
Coronal waves. EIT has observed wave-like disturbances propagating across the solar disk in association with eruptive events. Yohkoh SXT may have detected.
