Observations of Solar Eruptions On-Disk through the Low Corona out to 4 solar radii: Current Observations from SDO and Proposed Instruments to Fill the Gap
Phillip C Chamberlin1, Joan Burkepile2, Dr. Francis Gerard Eparvier, Ph.D.3, Yuhong Fan4, Sarah E Gibson2, Andrew R Jones5, Dr. James Paul Mason, PhD6, Scott William McIntosh7, Jeffrey S Newmark8, William Dean Pesnell9, Daniel B Seaton10, Barbara J Thompson11, Steven Tomczyk12 and Thomas N Woods13, (1)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (2)National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, (3)Univ Colorado, Boulder, CO, United States, (4)NCAR, Boulder, United States, (5)Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, United States, (6)University of Colorado Boulder, LASP, Boulder, United States, (7)High Altitude Observatory, Boulder, United States, (8)NASA Headquarters, Washington, United States, (9)NASA / GSFC, Greenbelt, United States, (10)Southwest Research Institute, Boulder, CO, United States, (11)NASA GSFC, Greenbelt, United States, (12)National Center for Atmospheric Research, High Altitude Observatory, Boulder, United States, (13)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States
