
The Latitudinal Distribution of Solar Sound Speed
The solar sound-speed distribution is not spherically symmetric. The figure shows the relative deviation from the spherically-symmetric sound-speed profile. The results are reliable between depths of 0.5 and 0.95 Rsun. In the deeper layers of the convection zone, sound-speed can be directly related to temperature, and thus the figure shows that the equatorial and lower-latitude regions of the Sun are cooler than the higher latitudes.
|
02.02.2009 The International Year of Astronomy at Yale The Astronomy Department is excited to participate in this global effort to help the citizens of the world rediscover their place in the Universe through the day- and night-time sky... MORE INFO |
|
10.21.2009 Popular Science just named Marla Geha one of its “Brilliant 10" Popular Science just named her one of its “Brilliant 10" — but for Marla Geha, the brilliance is all about the stars that don’t shine. MORE INFO |
![]() |
|
10.02.2009 Two Day Workshop Devoted to Yale/WIYN One Degree Image Survey The Yale Astronomy Department organized a two-day workshop on October 2-3, 2009 devoted to the Yale/WIYN One Degree Imager Survey. MORE INFO |
![]() |
Colloquia & Seminars | VIEW ALL
|
![]() |
|
|
![]() |
|




















