Slide 1 The Sun – Our Star Chapter 8 Slide 2 The preceding chapter described how we can get information from a spectrum. In this chapter, we apply these techniques to the…

Slide 1 European and French solar physics from space Jean ARNAUD Laboratoire FIZEAU Observatoire de la côte d’Azur Université de Nice Sophia Antipolis Slide 2 Introduction…

Slide 1 Connections Between the Magnetic Carpet and the Unbalanced Corona: New Monte Carlo Models Steven R. Cranmer & Adriaan van Ballegooijen Harvard-Smithsonian CfA,…

Slide 1 Page 1LWS Teams Day JSOC Overview HMI Data Products: Plan and Status Slide 2 Page 2LWS Teams Day JSOC Overview Primary goal: origin of solar variability The primary…

Stellar Activity in the Kepler Era Tom Ayres (CASA) Talk deals with lower rungs of Drakeâs Ladder, where, sadly, sexiness is low, but on positive side, knowledge content…

Stellar Activity in the Kepler Era Tom Ayres (CASA) Talk deals with lower rungs of Drakeâs Ladder, where, sadly, sexiness is low, but on positive side, knowledge content…

Coronal Dynamics - Can we detect MHD shocks and waves by Solar B ? K. Shibata Kwasan Observatory Kyoto University 2003 Feb. 3-5 Solar B Meeting @ ISAS Introduction Recent…

The structure of the lower solar atmosphere Robert Erdélyi [email protected] SPARC, Department of Applied Mathematics, The University of Sheffield (UK) http://robertus.staff.shef.ac.uk…

N+N+N International Meeting for Young Scientists (a British Council initiative) From our star to far stars: variation and variability Budapest (Hungary) 15-18 January, 2007…

Coronal Dynamics - Can we detect MHD shocks and waves by Solar B ? K. Shibata Kwasan Observatory Kyoto University 2003 Feb. 3-5 Solar B Meeting @ ISAS Introduction Recent…