The LPSP instrument on OSO 8. II - In-flight performance and preliminary results

Physics

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Oso-8, Satellite-Borne Instruments, Solar Instruments, Solar Physics, Angular Resolution, Calibrating, Chromosphere, Gratings (Spectra), Light Scattering, Lyman Alpha Radiation, Operational Problems, Photometry, Pointing Control Systems, Real Time Operation, Solar Activity, Solar Prominences, Spectral Resolution, Sunspots, Target Acquisition, Ultraviolet Spectrometers

Scientific paper

The paper describes the in-flight performance for the first 18 months of operation of the LPSP (Laboratoire de Physique Stellaire et Planetaire) instrument incorporated in the OSO 8 launched June 1975. By means of the instrument, an absolute pointing accuracy of nearly one second was achieved in orbit during real-time operations. The instrument uses a Cassegrain telescope and a spectrometer simultaneously observing six wavelengths. In-flight performance is discussed with attention to angular resolution, spectral resolution, dispersion and grating mechanism (spectral scanner) stability, scattered light background and dark current, photometric standardization, and absolute calibration. Real-time operation and problems are considered with reference to pointing system problems, target acquisition, and L-alpha modulation. Preliminary results involving the observational program, quiet sun and chromospheric studies, quiet chromospheric oscillation and transients, sunspots and active regions, prominences, and aeronomy investigations are reported.

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