Physics – Fluid Dynamics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..416..557h&link_type=abstract
Solar-Stellar Dynamos as Revealed by Helio- and Asteroseismology: GONG 2008/SOHO 21 ASP Conference Series, Vol. 416, proceedings
Physics
Fluid Dynamics
Scientific paper
The future of observational helioseismology lies in four areas: extremely high-degree observations, ground-based multi-wavelength observations, space-based observations from multiple viewpoints, and space weather predictive tools. On the theoretical front, advances in numerical simulations, further understanding of the effect of surface magnetic fields on the observations, and the development of methods to detect sub-surface magnetic fields are at the forefront. Finally, new developments in astrophysical fluid dynamics and dynamo models will provide new insights into the generation of magnetic fields, and will motivate new efforts to determine the nature of the internal solar velocity and magnetic fields.
No associations
LandOfFree
The Future of Helioseismology 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 The Future of Helioseismology, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Future of Helioseismology will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1111179