paper_1_12889_997
1 GONG Magnetogram pipeline. 2 The GONG Data Processing Pipeline
Unveiling the visible face of VLTI O. Chesneau 1,, N. Nardetto 1, K. Perraut 2, Ph. Stee 1, I. Tallon-Bosc 3 1 Nice/Fizeau, 2 Grenoble/IPAG, 3 Lyon/CRAL.
IMD 203 - Ch08
Cassini UVIS Update: He 584 Dayglow at Saturn Christopher Parkinson Ian Stewart and Yuk Yung January 05, 2006.
D. Mourard, N. Nardetto, R. Ligi and K. Perraut OCA/FIZEAU (Nice) – UJF/IPAG (Grenoble) Near Mt Wilson.
Estimating the magnetic energy in solar magnetic configurations Stéphane Régnier Reconnection seminar on Thursday 15 December 2005.
DEVELOPING A SOLAR RADIOMETRIC CALIBRATION SYSTEM USING SPECTRAL SYNTHESIS. Peter Fox (HAO/NCAR) We present quantitative information on how we estimate.
1 Lites FPP-SP Initial Reduct SOT #17 Meeting, NAOJ, April. 2006 Solar-B FPP Initial Data Reduction for the FPP Spectro- Polarimeter October, 2004 Bruce.
Using HMI to Understand Flux Cancellation by Brian Welsch 1, George Fisher 1, Yan Li 1, and Xudong Sun 2 1 Space Sciences Lab, UC-Berkeley, 2 Stanford.
Photospheric Flows and Solar Flares Brian T. Welsch 1, Yan Li 1, Peter W. Schuck 2, & George H. Fisher 1 1 Space Sciences Lab, UC-Berkeley 2 Naval Research.
ISSI, October 11-15, 2004 Synthesis of the Solar Spectrum including future plans Peter Fox ([email protected]) HAO/NCAR Work partly funded by NSF/RISE and.
