Slide 1 Slide 2 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…
1.The Sun2. The Sun: Our Parent Star 3. The Sun 4. Physical Properties of the Sun Interior structureof the Sun: Outer layers are not to scale. Thecoreis where nuclear fusion…
Slide 1 ALFVEN WAVES IN A POLAR CORONAL HOLE FROM HINODE/EIS OFF LIMB OBSERVATIONS Bemporad A. & Abbo L. [email protected]@oato.inaf.it – [email protected]…
Slide 1 Magnetic Fields at Mt. Wilson and MDI Slide 2 The 150-foot Tower Spectrograph Measures 12 line pairs simultaneously The long-term program uses 5250. The full coverage…
Slide 1 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, Marc DeRosa,…
Slide 1 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, Ben Brown)…
Slide 1 1 Hinode Monthly Highlights – Slow Solar Wind Sources Derived from recent publication from the Hinode/EIS team through the Naval Research Laboratory EIS mosaics…
Slide 1 Mike Marsh; S. Dalla; T. Laitinen; M. Dierckxsens; N. B. Crosby [email protected] Jeremiah Horrocks Institute, University of Central Lancashire, Preston, UK See…