IL of reaction for determinate structure (08.01.03.106)
Introduction to Cosmos and Organic.Edunet
Galaxies (From Seeds Ch. 12-14). The Milky Way Almost everything we see in the night sky belongs to the Milky Way. We see most of the Milky Way as a faint.
Dynamos in Accretion Disks: A general review and some moderately biased comments Chicago - October 2003.
The Disk Dynamo: How to drive a dynamo in an accretion disk through shear and a local instability Collaborators: Jungyeon Cho --- Chungnam U. Dmitry Shapovalov.
[email protected] The solar dynamo(s) Fausto Cattaneo Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas Chicago 2003.
Chicago, October 2003 David Hughes Department of Applied Mathematics University of Leeds Nonlinear Effects in Mean Field Dynamo Theory.
CHAPTER 10: CHAPTER 10: The Sun – Our Favorite (and Ordinary) Star.
Infall and Rotation around Young Stars Formation and Evolution of Protoplanetary Disks Michiel R. Hogerheijde Steward Observatory The University of Arizona.
Accretion Processes in Star Formation Lee Hartmann Cambridge Astrophysics Series, 32 Cambridge University Press (also from Nuria Calvet talks (2004) (continued)
The Sun – Our Star. General Properties Average star Absolute visual magnitude = 4.83 (magnitude if it were at a distance of 32.6 light years) Central.
Our Sun – Physical Properties. 109 Earths would fit across the diameter of the sun!! Diameter: 1,400,000 km, 864,000 miles 4.5 light-seconds 1,300,000.
