Mathematics – Optimization and Control
Scientist
Mathematics
Optimization and Control
Scientist
NASA Goddard Space Flight Center, Solar Physics Laboratory, Greenbelt, MD / GSFC
Goddard Space Flight Ctr., USA
NASA Goddard Space Flight Ctr., USA
NASA, Goddard Space Flight Center, Greenbelt, MD
Laboratory for Solar Physics, NASA / Goddard Space Flight Center
NASA's GSFC
Raytheon ITSS
NASA Goddard Space Flight Center, Solar Physics Laboratory, Code 671, Greenbelt, MD 20771 - Goddard Space Flight Center
Code 682, NASA Goddard Space Flight Center, Greenbelt, MD 20771; Remote Sensing Division, Naval Research Laboratory, Code 7210, Washington, DC 20375 Goddard Space Flight Center, Greenbelt, MD, US
NASA / Goddard Space Flight Ctr.
NASA's GSFC.
NASA Goddard Space Flight Ctr.
Solar Physics Laboratory, Code 671, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Code 682, NASA / Goddard Space Flight Center
Department of Astronomy and the McMath-Hulbert Observatory, The University of Michigan
Department of Astronomy and the McMath-Hulbert Observatory, The University of Michigan;, Laboratory for Solar Physics, NASA / Goddard Space Flight Center
Goddard Space Flight Center NASA / GSFC Code 671, Greenbelt, MD 20771, USA
Colorado, University, Boulder, CO
NASA, Goddard Space Flight Center, Greenbelt, Md.
NASA, Goddard Space Flight Center, Laboratory for Solar Physics and Astrophysics, Greenbelt, Md.
NASA Goddard Space Flight Center, Laboratory for Solar and Space Physics, Mail Code 612.1, Greenbelt, MD 20771, USA
Laboratory for Astronomy and Solar Physics, Code 682, NASA's Goddard Space Flight Center, Greenbelt, MD 20771, USA
Laboratory for Astronomy and Solar Physics, Code 680, NASA / Goddard Space Flight Center, Greenbelt, MD 20771, USA
National Aeronautics and S
<formula>O+, O, and <formula>O2 densities derived from measurements made by the High Resolution Airglow/Aurora Spectrograph (HIRAAS) sounding rocket experiment
A Comparison of Electron Density Profiles Derived from the Low Resolution Airglow and Aurora Spectrograph (LORAAS) Ultraviolet Measurements
A comparison of theoretical CIV emission line strengths with active region observations obtained with the solar EUV rocket telescope and spectrograph (SERTS)
A Comparison of Theoretical mg vi Emission Line Strengths with Active-Region Observations From Serts
A Comparison of Theoretical Si <Emphasis Type="SmallCaps">VIII</Emphasis> Emission Line Ratios with Observations from Serts
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