Solar XUV limb brightening observations. I - The lithium-like ions
Solar equatorial limb brightening of far UV resonance lines of lithium-like N V, O VI, Ne VIII, Mg X and Si XIII ions, interpreting oso-4 data with coronal model
Withbroe, G. L.↗
Engineering topics
Withbroe, G. L.
Publications and source records attributed to Withbroe, G. L..
Solar XUV limb brightening observations. II - Lines formed in the chromospheric- coronal transition region
Solar far UV limb brightening of C III, N III, N IV, O III, O IV and Si IV lines in chromospheric-corona transition region, correcting coronal model for spicule effects
Withbroe, G. L.↗
Extreme ultraviolet observations of active regions in the chromosphere and the corona
Oso-4 far UV observations of solar chromosphere and corona active regions
Kirshner, R. P.↗
The results and interpretation of some of the Harvard OSO-IV observations.
OSO-4 solar UV spectrum measurements, correlating chromospheric line intensity and photospheric magnetic field strengths
Goldberg, L.↗
The center-limb behavior of solar molecular lines.
Solar photosphere molecular lines behavior analyzed by various models, discussing local thermal equilibrium hypothesis validity
Withbroe, G. L.↗
A solar iron abundance determination using lines in the near UV
Solar iron abundance determination using lines in near ultraviolet
SPECTRAL LINE WIDTH↗
An analysis of CH in the solar atmosphere.
CH molecule solar spectral observations interpreted using several upper photosphere models and assuming local thermodynamic equilibrium approximation
THERMODYNAMIC EQUILIBRIUM↗
Theoretical profiles for the solar auto- ionization lines of A1 I.
Solar autoionization line profiles for Al I in rocket UV spectrum
SOLAR FLUX↗