Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992osuc.rept.....m&link_type=abstract
Final Report Ohio State Univ., Columbus. Dept. of Astronomy.
Astronomy and Astrophysics
Astronomy
High Resolution, Irradiance, Solar Radiation, Solar Spectra, Spectrum Analysis, Stellar Luminosity, Astronomical Spectroscopy, Data Reduction, Doppler Effect, Sunlight
Scientific paper
In this research, we aim to determine to what extent the solar irradiance changes measured through the 1980's from orbiting vehicles are accompanied by spectroscopic irradiance changes observable from the ground. We describe fractional changes in line absorption as 'blanketing'. In section 2, we briefly review results obtained in an earlier project and which have been published. Section 3 describes the data of this investigation; section 4 describes the data reduction; section 5 describes the observational results in terms of blanketing; and section 6 describes the interpretation of the measured changes. Section 7 contains an outline of possible uses for Doppler-shift data that emerges with the measurements of the blanketing variations. Section 8 is an outline for future research suggested by our results in this project.
No associations
LandOfFree
Comparison of high-resolution solar irradiance spectra and the solar luminosity in the period 1980-1989 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 Comparison of high-resolution solar irradiance spectra and the solar luminosity in the period 1980-1989, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison of high-resolution solar irradiance spectra and the solar luminosity in the period 1980-1989 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1739150