Analysis of time-dependent phenomena observed with the LPSP OSO-8 instrument. Final report
Technical Report
·
OSTI ID:5472120
The dynamics of the solar photosphere and chromosphere are studied. Observations obtained by the Laboratorie de Physique Stellaire et Planetaire's (LPSP) ultraviolet spectrometer onboard the OSO-8 spacecraft are analyzed, and dynamic models of the chromosphere and the emitted resonance line spectrum are calculated. Some of the unpublished data analysis and theoretical modeling which are being prepared for publication are discussed. A discussion of the state of the theory of velocity fields in the solar atmosphere is also presented. An invited review presented at the OSO-8 Workshop on the topic of oscillatory motions in the quiet sun is included. The results of the OSO-8 data analysis prepared in close collaboration with LPSP scientists are presented. Material for two articles is also presented.
- Research Organization:
- Lockheed Missiles and Space Co., Palo Alto, CA (USA)
- OSTI ID:
- 5472120
- Report Number(s):
- N-79-24932
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640104* -- Astrophysics & Cosmology-- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATMOSPHERES
CHROMOSPHERE
DATA
DATA FORMS
DYNAMICS
EXPERIMENTAL DATA
GRAPHS
INFORMATION
MECHANICS
MOTION
NUMERICAL DATA
ORBITING SOLAR OBSERVATORIES
OSCILLATION MODES
PHOTOSPHERE
SATELLITES
SOLAR ATMOSPHERE
SPECTRA
THEORETICAL DATA
TIME DEPENDENCE
ULTRAVIOLET SPECTRA
VELOCITY
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATMOSPHERES
CHROMOSPHERE
DATA
DATA FORMS
DYNAMICS
EXPERIMENTAL DATA
GRAPHS
INFORMATION
MECHANICS
MOTION
NUMERICAL DATA
ORBITING SOLAR OBSERVATORIES
OSCILLATION MODES
PHOTOSPHERE
SATELLITES
SOLAR ATMOSPHERE
SPECTRA
THEORETICAL DATA
TIME DEPENDENCE
ULTRAVIOLET SPECTRA
VELOCITY