Numerical MHD modelling of waves in solar coronal loops Petr Jelínek 1,2 and Marian Karlický 2 1 University of South Bohemia, Department of Physics České.
Outline How do we define space weather? How do we observe it? What drives it (solar activity and solar phenomena)? Which are the impacts on: the atmosphere.
Astronomy Lecture The Sun: Our Extraordinary Ordinary Star.
Working Group I: Solar Filaments (Mon. afternoon + Tues morning) Activation through eruption Sub-surface (Wed. morning) Understanding the magnetic.
FAST-ION-BEAM ATOMIC SPECTROSCOPY Toledo Heavy Ion Accelerator (THIA) Laboratory.
Announcements Pick up graded homework Seminar on gravitational waves today, 1:00, SL 240 No class this Friday! Test next week on material through today’s.
THE NEW SOLAR CORONA Ashwanden, Markus J., Arthur I. Poland, and Douglas M. Rabin Annual Review of Astronomy and Astrophysics 2001. 39:175-210 Presented.
Coronal hard X-rays prior to RHESSI H. S. Hudson Space Sciences Lab, UC Berkeley.
Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind.
