Solar cycle variation in solar f-mode frequencies and radius

Details Solar cycle variation in solar f-mode frequencies and radius Solar cycle variation in solar f-mode frequencies and radius

2000-01-17

arxiv.org/abs/astro-ph/0001293v1

Solar Phys. 192 (2000) 459

Astronomy and Astrophysics

Astrophysics

To appear in Solar Physics

Scientific paper

Using data from the Global Oscillation Network Group (GONG) covering the period from 1995 to 1998, we study the change with solar activity in solar f-mode frequencies. The results are compared with similar changes detected from the Michelson Doppler Imager (MDI) data. We find variations in f-mode frequencies which are correlated with solar activity indices. If these changes are due to variation in solar radius then the implications are that the solar radius decreases by about 5 km from minimum to maximum activity.

Affiliated with

Also associated with

No associations

Rating

Solar cycle variation in solar f-mode frequencies and radius 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 cycle variation in solar f-mode frequencies and radius, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar cycle variation in solar f-mode frequencies and radius will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-266408