Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations

Details Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations

2009-03-30

arxiv.org/abs/0903.5219v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Accepted for publication in MNRAS; 5 pages, 3 tables

Scientific paper

We present a list of "best possible" estimates of low-degree p-mode frequencies, from 8640 days of observations made by the Birmingham Solar-Oscillations Network (BiSON). This is the longest stretch of helioseismic data ever used for this purpose, giving exquisite precision in the estimated frequencies. Every effort has been made in the analysis to ensure that the frequency estimates are also accurate. In addition to presenting the raw best-fitting frequencies from our "peak bagging" analysis, we also provide tables of corrected frequencies pertinent to the quiet-Sun and an intermediate level of solar activity.

Affiliated with

Also associated with

No associations

Rating

Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations 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 Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-425161