After the loss of the meteroid shield required using the solar scientific airlock to erect the sun shade, methods were improvised to operate the S020 experiment on EVA's. Almost no data was obtained in the wavelength range 10 to 110 A. From 110 to 280 A the spectra were 10 to 100 time less intense than expected. A probable cause in loss of instrument sensitivity is the contamination of the filters by the spacecraft coolant. A list of observed lines in presented. Although less data was obtained than expected, several lines not previously observed were recorded; and the spectra serve to confirm many very faintly observed weak lines recorded from sounding rockets by other experiments
Predicting star magnitude visible through contaminated spacecraft window by naked eye or sextan
During the report period the BUGS-4 instrument was completed, and the maiden voyage took place on 29...
Photographs taken on Apollo 16 before, during, and after a water dump were analyzed for residual bac...
The problems encountered in the observing programs using the airlock coronagraph (T025) are reported...
Radiation tests were conducted on the various types of Skylab film to establish the total radiation ...
The solar radio spectra were recorded in real time, both on film and magnetic tape, during the perio...
The white light solar coronagraph was one of the scientific telescopes flown on Skylab to study the ...
Techniques originally developed for the Skylab T025 contamination experiment were applied to S052 wh...
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. Specific test sites in the White Sands,...
Results from research in solar physics related to the Skylab/ATM S-056 X-Ray Experiment are presente...
Spectral data obtained by the SO82B experiment aboard SKYLAB were used to critically evaluate existi...
The successful launch of Skylab on May 14, 1973, provided an unique space platform for study of the ...
This report covers the period from September 1, 1992 to August 31, 1993. During the reporting period...
The Skylab D024 Thermal Control Coatings and Polymeric Films Experiment was designed to determine th...
Predicting star magnitude visible through contaminated spacecraft window by naked eye or sextan
During the report period the BUGS-4 instrument was completed, and the maiden voyage took place on 29...
Photographs taken on Apollo 16 before, during, and after a water dump were analyzed for residual bac...
The problems encountered in the observing programs using the airlock coronagraph (T025) are reported...
Radiation tests were conducted on the various types of Skylab film to establish the total radiation ...
The solar radio spectra were recorded in real time, both on film and magnetic tape, during the perio...
The white light solar coronagraph was one of the scientific telescopes flown on Skylab to study the ...
Techniques originally developed for the Skylab T025 contamination experiment were applied to S052 wh...
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. Specific test sites in the White Sands,...
Results from research in solar physics related to the Skylab/ATM S-056 X-Ray Experiment are presente...
Spectral data obtained by the SO82B experiment aboard SKYLAB were used to critically evaluate existi...
The successful launch of Skylab on May 14, 1973, provided an unique space platform for study of the ...
This report covers the period from September 1, 1992 to August 31, 1993. During the reporting period...
The Skylab D024 Thermal Control Coatings and Polymeric Films Experiment was designed to determine th...
Predicting star magnitude visible through contaminated spacecraft window by naked eye or sextan
During the report period the BUGS-4 instrument was completed, and the maiden voyage took place on 29...
Photographs taken on Apollo 16 before, during, and after a water dump were analyzed for residual bac...