Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...662l.135w&link_type=abstract
The Astrophysical Journal, Volume 662, Issue 2, pp. L135-L138.
Astronomy and Astrophysics
Astronomy
2
Convection, Sun: Helioseismology, Sun: Photosphere, Sun: Rotation, Turbulence, Waves
Scientific paper
We explore the nature of ``hills'' observed on the solar surface that had previously been attributed to Rossby waves. We investigate the solar hills phenomenon by analyzing the output from a synthetic model based solely on the observed solar photospheric convection spectrum. We show that the characteristics of these hills can be explained by the corrugation of the surface produced by the radial flows of the convection. The hills in our simulations are dominated by supergranules, a well-known component of solar convection. Rossby waves have been predicted to exist within the Sun and may play an important role in the dynamics of the solar interior, including the Sun's differential rotation and magnetic dynamo. Our study suggests, however, that the hills observed at the solar limb do not confirm the existence of solar Rossby waves.
Cuntz Manfred
Hathaway David H.
Williams Peter E.
No associations
LandOfFree
Solar Rossby Wave ``Hills'' Identified as Supergranules 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 Rossby Wave ``Hills'' Identified as Supergranules, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Rossby Wave ``Hills'' Identified as Supergranules will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1419306