Magnetism ~ The Energy Sea We Live In
Subsurface Flows from ring-diagram analysis Irene González Hernández National Solar Observatory Tucson, Arizona.
Stellar Formation 1)Solar Wind/Sunspots 2)Interstellar Medium 3)Protostars 4)A Star is Born October 23, 2002.
Solar cycle variation in the peak asymmetry: solar or artefact? S. J. Jiménez-Reyes IAC 13-sept-2004.
Nonlinear Force-Free Field Modeling AIA/HMI Science Team Meeting Session C2 14 February 2006 Marc DeRosa on behalf of the “NLFFF Consortium” (Karel Schrijver,
Solar Dynamics Observatory and Seeing the Sun. Solar Dynamics Observatory (SDO) SDO during assembly The Launch Orbit Mission Instruments Capabilities.
Astronomy 1020 Stellar Astronomy Spring_2015 Day-30.
Solar Dynamics Observatory and Seeing the Sun
Observing the Sun. Corona: EUV; X-rays Chromosphere: H , UV, EUV Photosphere: near UV, Visible light, infra-red.
Solar-B Global DataGrid 21 st September 2006 UK e-Science All Hands Meeting 2006 RALMSSL Tim Folkes Elizabeth Auden Jens Jensen Paul Lamb Matthew WildMatthew.
Manolis K. Georgoulis 1 & Thomas Wiegelmann 2
Meridional Circulation from ring-diagram analysis Irene González Hernández and the GONG++ team National Solar Observatory Tucson, Arizona.
