Discovery of the Neutrino Mass P1X* Frontiers of Physics Lectures psoler/P1X_neutrino.ppt 21-22 October 2003 Dr Paul Soler.
Micro solar
Hubble Science Briefing Hubble Does Double-Duty Science: Finding Planets and Characterizing Stellar Flares in an Old Stellar Population Rachel Osten Space.
Advantage: Neutrinos 2. Neutrino scattering Super Kamiokande located 1000m underground in Kamioka mine in Japan is a water Cherenkov detector made up of.
Towards real-time Space Weather forecasts using CMIT: Geomagnetic variations and regional K indexes George Millward …with help from: Michael Gehmeyr (LASP),
Nonlinear Tides in Exoplanet Host Stars (Extreme Solar Systems II) Phil ArrasUniversity of Virginia Josh BurkartU. C. Berkeley Eliot QuataertU. C. Berkeley.
Prospects for 7 Be Solar Neutrino Detection with KamLAND Stanford University Department of Physics Kazumi Ishii.
Physics 681: Solar Physics and Instrumentation – Lecture 23 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
October 3, 2003IFIC, UVEG-CSIC A road map to solar fluxes, osc. param., and test for new physics Carlos Pena Garay IAS ~
Chapter 16 – Chemical Analysis
Neutrino Reactions on the Deuteron in Core-Collapse Supernovae Satoshi Nakamura Osaka University Collaborators: S. Nasu, T. Sato (Osaka U.), K. Sumiyoshi.
Chapter 16 – Chemical Analysis Review of curves of growth –The linear part: The width is set by the thermal width Eqw is proportional to abundance –The.
