Determining the Location of Open Magnetic Field Areas in Active Regions and their Potential as Sources of the Slow Solar Wind J. L. Culhane 1, S.J. Edwards.
Solar Wind Transients and SEPs
HMI Magnetogram 2012.06.08_21:30
GONG Magnetograms and Coronal Field Modeling G.J.D. Petrie, J. Bolding, R. Clark, K. Donaldson-Hanna, J.W. Harvey, F. Hill, C. Toner & T.M. Wentzel National.
195 Å image – behind 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – ahead SECCHI Extreme.
J. Todd Hoeksema Stanford University
Case Studies of Interplanetary Coronal Mass Ejections Interplanetary Coronal Mass Ejections – Different Phases of the Cycle Of particular interest to the.
Solar Cycle Trends and Case Studies of Interplanetary Coronal Mass Ejections Interplanetary Coronal Mass Ejections During Different Phases of the Cycle.
195 Å image – behind
Solar Cycle Trends and Case Studies of Interplanetary Coronal Mass Ejections
Thomas Zurbuchen University of Michigan [email protected] The Structure and Sources of the Solar Wind during the Solar Cycle.
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