What have we learnt with the Luminosity Oscillations Imager over the past 6 years?

Details What have we learnt with the Luminosity Oscillations Imager over the past 6 years? What have we learnt with the Luminosity Oscillations Imager over the past 6 years?

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508...47a&link_type=abstract

In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze

Physics

8

Intensity, P-Modes, Soho, Sun

Scientific paper

We summarize what we achieved with 6 years of LOI data. We present old as well as new results regarding the p-mode parameters dependence upon solar activity. We have also derived the dependence of the solar background noise upon solar activity and solar disk position. Inversions done using LOI frequencies and higher-degree mode frequencies from GONG confirm previous velocity inversions.

Affiliated with

Also associated with

No associations

Rating

What have we learnt with the Luminosity Oscillations Imager over the past 6 years? 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 What have we learnt with the Luminosity Oscillations Imager over the past 6 years?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and What have we learnt with the Luminosity Oscillations Imager over the past 6 years? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1893835