Our star, the Sun is a big ball of gas And it's 99 percent of our solar system's mass It's an average star in our Milky Way Warming the Earth every day.
Drift models and polar field for cosmic rays propagation Stefano Della Torre 11th ICATPP, Como 5-9 october 2009.
Space Weather: Forecasting, Tracking, and the Effects of Earth Directed Solar Phenomena
The sun
Simulations of the Dynamics Generated in the Solar Atmosphere by Solar Global Oscillating Eigenmodes
SH13A-2240 Automatic Detection of EUV Coronal Loops from SDO-AIA Data Alissa N. Oppenheimer¹ ( [email protected] ), A. Winebarger², S. Farid³,
ALFVEN WAVES IN A POLAR CORONAL HOLE FROM HINODE/EIS OFF LIMB OBSERVATIONS Bemporad A. & Abbo L. [email protected]@oato.inaf.it – [email protected].
Magnetic Fields at Mt. Wilson and MDI. The 150-foot Tower Spectrograph Measures 12 line pairs simultaneously The long-term program uses 5250. The full.
Global Convection Modeling (where are we heading and how does this impact HMI?) Mark Miesch HAO/NCAR, JILA/CU (Sacha Brun, Juri Toomre, Matt Browning,
Dynamo Modeling: What HMI/AIA can do for us (and perhaps vice versa) Mark Miesch HAO/NCAR, JILA/CU (Sacha Brun, Juri Toomre, Matt Browning, Marc DeRosa,
What coronal parameters determine solar wind speed? M. Kojima, M. Tokumaru, K. Fujiki, H. Itoh and T. Murakami Solar-Terrestrial Environment Laboratory,
What coronal parameters determine solar wind speed?
