Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Marshall Space Flight Center, XD12, Space Science Branch, Huntsville, Al 35812, USA
University of Maryland, NASA / GSFC
University of Alabama in Huntsville, Hunstville, AL, USA; / University of Alabama - Huntsville
University of Alabama - Huntsville / NSSTC
Marshall Space Flight Center, SD50, Space Science Department, Huntsville, AL 35812; Physics Department, University of Alabama at Huntsville, Huntsville, AL 35899. of Alabama - Huntsville
University of Alabama - Huntsville / MSFC
NRC / MSFC
University of Alabama - Huntsville / MSFC / NSSTC
UAHuntsville
University of Alabama, Huntsville, AL
NASA / MSFC / NSSTC Space Science Department, SD50 Marshall Space Flight Center, Huntsville, AL 35812, USA
University of Alabama in Huntsville, SD50 NASA / Marshall Space Flight Center, Huntsville, AL 35812, USA of Alabama - Huntsville / MSFC / NSSTC, Space Science Department, SD50 Marshall Space Flight Center, Huntsviile, Al 35812, USA Space Flight Center / NASA Space Flight Center / NASA of Alabama, Huntsville
NASA / Marshall Space Flight Center, Marsahall Space Flight Center, Huntsville, AL 35812, USA of Physics, The University of Alabama in Huntsville, Huntsville, AL 35899, USA; SD 50, NASA / Marshall Space Flight Center, NSSTC, 301 Sparkman Drive, Huntsville, AL 35899, USA of Alabama - Huntsville, Huntsville, AL, USA Space Flight Center, SD50 / Space Science Department, Huntsville, AL 35812; Physics Department, University of Alabama at Huntsville, Huntsville, AL 35899. Marshall Space Flight Center, SD 50, Space Science Department, Huntsville, AL 35812; Physics Department, Univers
24-Hour Forecasting of CME/Flare Eruptions from Active-Region Magnetograms (Invited)
3D Magnetic Fields and Coronal Heating in Active Regions
A Correlation between Length of Strong-Shear Neutral Lines and Total X-ray Brightness in Active Regions
A Correlation between Length of Strong-Shear Neutral Lines and Total X-ray Brightness in Active Regions
A measure from line-of-sight magnetograms for prediction of coronal mass ejections
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