Solar oscillations as they are seen from minimum to maximum of solar activity

Details Solar oscillations as they are seen from minimum to maximum of solar activity Solar oscillations as they are seen from minimum to maximum of solar activity

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464...57g&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Computer Science

3

Solar Oscillations, Helioseismology, Excitation, Low Degree

Scientific paper

The GONG time series, 1692 days long, is used for the evaluation of the
low-l (l = 0 - 8) p-mode parameters. The set of the mode frequencies,
the most comprehensive up to date in radial orders n, is presented. The
variations of mode profiles with time are discussed.

Affiliated with

Also associated with

No associations

Rating

Solar oscillations as they are seen from minimum to maximum of solar activity 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 Solar oscillations as they are seen from minimum to maximum of solar activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar oscillations as they are seen from minimum to maximum of solar activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-923442