The Sun – Our Star Chapter 8. The preceding chapter described how we can get information from a spectrum. In this chapter, we apply these techniques to.
European and French solar physics from space Jean ARNAUD Laboratoire FIZEAU Observatoire de la côte d’Azur Université de Nice Sophia Antipolis.
Connections Between the Magnetic Carpet and the Unbalanced Corona: New Monte Carlo Models Steven R. Cranmer & Adriaan van Ballegooijen Harvard-Smithsonian.
Page 1LWS Teams Day JSOC Overview HMI Data Products: Plan and Status.
Stellar Activity in the Kepler Era Tom Ayres (CASA)
Solar Physics & upper-Atmosphere Research Group Robert Erdélyi University of SheffieldPPARC ASSSP 2006 31 Aug – 4 Sep.
N+N+N International Meeting for Young Scientists (a British Council initiative)
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.
Coronal Dynamics - Can we detect MHD shocks and waves by Solar B ?
