Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
NASA / Goddard
NASA, Goddard Space Flight Center, Greenbelt, MD
Institut für Theoretetische Physik, Peilinstitut 1, Pfaffen Walbrind, 57-4, Stuttgart, D-70550 Germany
NASA, Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, MD
NASA, Goddard Space Flight Center, Greenbelt, Md.
NASA, Goddard Space Flight Center, Theoretical Studies Group, Greenbelt, Md.
NASA / GSFC
NASA, Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, Md.
NASA. Goddard Space Flight Center, Greenbelt, MD, US
Laboratory for Astronomy and Solar Physics-Code 681, Goddard Space Flight Center, Greenbelt, MD 20771, USA
Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771
NASA Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, MD 20771
Laboratory for Astronomy and Solar Physics, Goddard Space Flight Center, Greenbelt, MD 20771, USA
NASA, Goddard Space Flight Center, Laboratory for Astrophysics and Solar Physics, Greenbelt, Md.
NASA / Goddard Space Flight Center Greenbelt, Maryland 20771 USA
NASA / Goddard Space Flight Center, Greenbelt, MD 20771, USA
Laboratory for Astronomy and Solar Physics, Goddard Space Flight Center, Greenbelt MD 20771, USA
NASA, Goddard Space Flight Center, Laboratory for Solar Physics and Astrophysics, Greenbelt, Md.
Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771.
NASA Goddard Space Flight Center
Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center Greenbelt, MD 20771, USA
Mathematical Science Consultants, Inc., Greenbelt, MD, US
Laboratory for Astronomy and Solar Physics, Godda
A comparison of the C III, O V, F VI, and NE VII Delta N = 0 (2-2) line emissions from a laboratory plasma with theoretical predictions and astrophysical observations
A comparison of theoretical and solar-flare intensity ratios for the Fe XIX X-ray lines
A correction factor for Gaussian deconvolution of optically thick linewidths in homogeneous sources
A distorted-wave methodology for electron-ion impact excitation - Calculation for two-electron ions
A Multi-Level Analysis of Opacity in the Coronal Fe XVII Spectrum
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