Solar g-mode oscillations: Comparison of SMM-ACRIM and ground-based observations

Details Solar g-mode oscillations: Comparison of SMM-ACRIM and ground-based observations Solar g-mode oscillations: Comparison of SMM-ACRIM and ground-based observations

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989stan.reptq....s&link_type=abstract

Final Report, 1 Jul. 1987 - 30 Jun. 1988 Stanford Univ., CA. Center for Space Science and Astrophysics.

Astronomy and Astrophysics

Astrophysics

Data Acquisition, Mathematical Models, Solar Oscillations, Transparence, Brightness, Gradients, Spectrum Analysis

Scientific paper

Progress was made in access to data and in developing programs for its analysis. The difficulties in completing the work in the planned time can be traced to several factors. The correction of the Stanford oscillation using gridded intensity data was not successful. It was concluded that due to poor continuity of the 1985 and 1986 data due to clouds, that a joint analysis with the ACRIM data (best solar oscillation data to date) on the summer 1987 observations should be performed. The 1988 Stanford oscillation data are being examined and the cross comparison of the ACRIM spectrum with the Standford spectrum for 1987 in the g-mode regime will shortly begin.

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