Big Bear Solar Observatory New Solar Telescope in Big Bear Philip R. Goode Big Bear Solar Observatory Center for Solar-Terrestrial Research New Jersey.
Coronal Ejecta in October - November of 2003 and predictions of the associated geomagnetic events 1 Big Bear Solar Observatory, New Jersey Institute of.
Signatures of Intermittent Turbulence in Hinode Quiet Sun Photosphere
The Astrophysical Journal, 619:1160–1166, 2005
Probing the Solar Interior on Multiple Timescales Using Global Helioseismololgy
Helioseismic Holography with GONG
1 1 AST Committee of Visitors February 2011 National Solar Observatory Overview Craig Foltz Program Officer NSO.
STR Program: Past, Present, and Future ILIA I. Roussev [email protected] Program Director, STR Program Division of Atmospheric and Geospace Sciences SHINE.
Stokes Inversion 180 Azimuth Ambiguity Resolution Non-linear Force-free field (NLFFF) Extrapolation of Magnetic Field Progress in Setting up Data Processing.
Stokes Inversion 180 Azimuth Ambiguity Resolution
This work utilizes data obtained by the Global Oscillation Network Group (GONG) Program and the SOI/MDI instrument on SoHO. GONG is managed by the National.
AST Committee of Visitors February 2011
