Forward analysis of the BBSO frequency-splitting coefficients for 1986

Details Forward analysis of the BBSO frequency-splitting coefficients for 1986 Forward analysis of the BBSO frequency-splitting coefficients for 1986

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...438..445w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 438, no. 1, p. 445-453

Astronomy and Astrophysics

Astrophysics

10

Coefficients, Frequencies, Recursive Functions, Solar Rotation, Splitting, Astronomical Observatories, Data Processing, Eigenvectors, Solar Oscillations

Scientific paper

Frequency-splitting data obtained at the Big Bear Solar Observatory (BBSO) for 1986 are collated by a method which permits qualitative inferences regarding the internal rotation profile of the Sun. The data are analyzed by a recursive forward approach which is first tested by a 'hare and hounds' experiment. The method is then applied to the Big Bear data yields a solution for the Sun's internal rotation profile for 1986.

Affiliated with

Also associated with

No associations

Rating

Forward analysis of the BBSO frequency-splitting coefficients for 1986 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 Forward analysis of the BBSO frequency-splitting coefficients for 1986, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Forward analysis of the BBSO frequency-splitting coefficients for 1986 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1818965