Momentum Conservation in Flares H. S. Hudson Space Sciences Laboratory, University of California, Berkeley, USA Astronomy & Astrophysics Group, Glasgow.
1 Chromospheric UV oscillations depend on altitude and local magnetic field Noah S. Heller and E.J. Zita, The Evergreen State College, Olympia, WA 98505.
Feb. 2006HMI/AIA Science Team Mtg.1 Heating the Corona and Driving the Solar Wind A. A. van Ballegooijen Smithsonian Astrophysical Observatory Cambridge,
Pinpointing a stellar X-ray flare using XMM-Newton and VLT/UVES
Quelques développements récents sur la physique du chauffage coronal. T. Passot UNS, CNRS, OCA Hinode/XRT Thanks to: E. Buchlin, S. Galtier. Some viewgraphs.
Heating the Corona and Driving the Solar Wind
Pinpointing a stellar X-ray flare using XMM-Newton and VLT/UVES Uwe Wolter Hamburger Sternwarte May 2008 J.U. Ness J. Robrade J.H.M.M. Schmitt.
