Measures of solar oblateness using active- region masking H.J. Zahid, M.D. Fivian, H.S. Hudson Space Sciences Lab, UC Berkeley.
Co-spatial White Light and Hard X-ray Flare Footpoints seen above the Solar Limb: RHESSI and HMI observations Säm Krucker Space Sciences Laboratory, UC.
1 Interpreting SECCHI White Light Images: FOV Sensitivity & Stereo Viewing Paulett Liewer, JPL; Russ Howard & Dennis Socker, NRL SECCHI Consortium Meeting.
Day-3. Announcements Next week: Dark Night Observing on Tues. 9/8 & Thur. 9/10 Plan to re-start the “Astro-group” meetings. When is good for everyone?
Structure of the solar corona Ramón Oliver Universitat de les Illes Balears PPARC Advanced Summer School in Solar Physics.
Yohkoh statistical studies
Basic principle of medical dermatology: “ If it’s dry, wet it. If it’s wet, dry it. ”
Transition Region and Coronal Explorer (TRACE) Spacecraft Results The study of the Transit of Venus in 2004 is an alternative test for observing methods,
Venus Transit 2004 in Slovak Republic
M. Gai - GAMELa Thuile, Rencontres de Moriond XLVI, 20111 Gravitation Astrometric Measurement Experiment M. Gai - INAF-Osservatorio Astronomico di Torino.
Ionization patterns in the circumstellar medium of active galaxies Joss Bland-Hawthorn (AAO) Collaborator: P.R. Maloney (U Colorado)
The Space Weather Week