Space weather: solar drivers, impacts and forecasts Henrik Lundstedt Swedish Institute of Space Physics Lund We live inside the continuously expanding.
1 The Future of Particle Physics S F King Southampton, March 22, 2004 S F King Southampton, March 22, 2004 universe.exe.
Solar Image Processing: A Multiscale View C. Alex Young NASA/GSFC C. Alex Young NASA/GSFC UCLA - IPAM (January 28, 2004)
The on-going programme. 3-family oscillation matrix (Pontecorvo, Maki, Nakagawa, Sakata) S = sine c = cosine CP violation phase. drives SOLAR.
and the US Neutrino Programme Leslie Camilleri CERN, PH GDR Neutrino IPNO Orsay, 4 octobre 2006.
1.B – Solar Dynamo 1.C – Global Circulation 1.D – Irradiance Sources 1.H – Far-side Imaging 1.F – Solar Subsurface Weather 1.E – Coronal Magnetic Field.
Page 1HMI Team Meeting – January 26-27, 2005 HMI Investigation Overview Philip Scherrer [email protected] 650-723-1504.
Investigation Overview, Scherrer, Page 1SDO Science Writers Workshop – 16 Dec 2009 HMI Investigation Overview Philip Scherrer HMI Principal Investigator.
Kinetic and Magnetic Helicities of Solar Active Regions Ram Ajor Maurya, Ashok Ambastha And Vema Reddy Udaipur Solar Observatory Physical Research Laboratory,
Pioneering Works on Ring Diagram Analysis with Irene González Hernández
NOnA and the US Neutrino Programme
Looking for New Physics in Neutrino Experiments Morgan Wascko Imperial College London.
