1. Simulating Cyclic Evolution of Coronal Magnetic Fields using a Potential Field Source Surface Model Coupled with a Dynamo Model Akshaya Suresh (Yale University, REU-LASP/HAO),…

Slide 1Outline How do we define space weather? How do we observe it? What drives it (solar activity and solar phenomena)? Which are the impacts on: the atmosphere and technological…

Slide 1 Observations and Magnetic Field Modeling of CMEs’ Source Regions Yingna Su Harvard-Smithsonian Center for Astrophysics Collaborators: Adriaan van Ballegooijen,…

Slide 1 Determining the Location of Open Magnetic Field Areas in Active Regions and their Potential as Sources of the Slow Solar Wind J. L. Culhane1, S.J. Edwards2,3, C.E.…

Structure of a Transition Region Explosive Event Imaging-Spectroscopy with MOSES Lewis Fox1, C. C. Kankelborg1, R. J. Thomas2, D. W. Longcope1 1 Montana State University,…

Slide 1 Active Region Upflow Plasma and its Possible Contribution to the Slow Solar Wind J. L. Culhane1, D.H. Brooks2, L. van Driel-Gesztelyi1,3,4, P. Démoulin3, D. Baker1,…

Scientific Interests in OVSA Expanded Array Haimin Wang Physics of Elementary Bursts Multi-wavelength Observations: Microwave imaging spectroscopy RHESSI demodulated light…

Publish and be Damned: An overview of the cycle variations in the solar corona Louise Harra [email protected] UCL Department of Space and Climate Physics Mullard Space Science…

Flare Energy Build-Up in a Decaying Active Region Near a Coronal Hole Yingna Su1,2, Adriaan van Ballegooijen1, Brigitte Schmieder3, Arkadiusz Berlicki3, Yang Guo3,Leon Golub1,…