Add to ORKGSpectral data obtained by the SO82B experiment aboard SKYLAB were used to critically evaluate existing models of the solar upper photosphere and lower chromosphere. These spectral diagnostics were used to develop new solar models
The author has identified the following significant results. Comparison of several existing infrared...
The author has identified the following significant results. During all three Skylab missions, prism...
A dynamical model was proposed which is in agreement with the observations that suggest the solar ch...
The use of the solar H I Lyman spectral line as a diagnostic of the lower to middle chromosphere is ...
Since the early 1970s we have been developing the extensive computer programs needed to construct mo...
Solar chromospheric models are described. The models included are based on the observed spectrum, an...
A computer program was developed which, given a line list and a model atmosphere, computes a solar u...
Theoretical solar chromospheric and photospheric models are computed for use in analyzing OSO 8 spec...
Oscillations, physical properties of the solar atmosphere, motions in the quiet solar atmosphere, co...
The Solar Maximum Mission support program is mentioned along with investigations of the solar corona...
The complete set of C 4 time sequences generated by the University of Colorado high resolution ultra...
We study off-limb emission of the lower solar atmosphere using high-resolution imaging spectroscopy ...
A detailed reexamination of the temperature-density structure of the photosphere and low chromospher...
The author has identified the following significant results. Specific test sites in the White Sands,...
Over 700 far UV photos were obtained with the S201 electrographic camera on Skylab 4 (27 Nov. 1973 -...
The author has identified the following significant results. Comparison of several existing infrared...
The author has identified the following significant results. During all three Skylab missions, prism...
A dynamical model was proposed which is in agreement with the observations that suggest the solar ch...
The use of the solar H I Lyman spectral line as a diagnostic of the lower to middle chromosphere is ...
Since the early 1970s we have been developing the extensive computer programs needed to construct mo...
Solar chromospheric models are described. The models included are based on the observed spectrum, an...
A computer program was developed which, given a line list and a model atmosphere, computes a solar u...
Theoretical solar chromospheric and photospheric models are computed for use in analyzing OSO 8 spec...
Oscillations, physical properties of the solar atmosphere, motions in the quiet solar atmosphere, co...
The Solar Maximum Mission support program is mentioned along with investigations of the solar corona...
The complete set of C 4 time sequences generated by the University of Colorado high resolution ultra...
We study off-limb emission of the lower solar atmosphere using high-resolution imaging spectroscopy ...
A detailed reexamination of the temperature-density structure of the photosphere and low chromospher...
The author has identified the following significant results. Specific test sites in the White Sands,...
Over 700 far UV photos were obtained with the S201 electrographic camera on Skylab 4 (27 Nov. 1973 -...
The author has identified the following significant results. Comparison of several existing infrared...
The author has identified the following significant results. During all three Skylab missions, prism...
A dynamical model was proposed which is in agreement with the observations that suggest the solar ch...