Physics – Optics
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345.1088h&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 15, 1989, p. 1088-1103. Research supported by SRON.
Physics
Optics
3
Optical Resonance, Resonance Scattering, Solar Oscillations, Solar Spectrometers, Solar Velocity, Velocity Measurement, Instrument Errors, Integrated Optics, Power Spectra, Qualitative Analysis, White Noise
Scientific paper
The sensitivity of resonant scattering spectrometers for measuring solar velocity oscillations in integrated light is analyzed. It is shown that, with the help of simple analytical tools and qualitative arguments, most of the contributions to the instrumental sensitivity can be estimated. Although the frequency dependence of the individual sources of instrument noise cannot always be predicted reliably in this way, it is possible to derive useful estimates of instrumental parameters via comparison with a desired noise level.
No associations
LandOfFree
On the sensitivity of resonant scattering spectrometers for whole-disk solar velocity oscillation measurements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the sensitivity of resonant scattering spectrometers for whole-disk solar velocity oscillation measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the sensitivity of resonant scattering spectrometers for whole-disk solar velocity oscillation measurements will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1528289