Slide 1Solar Wind Acceleration and Waves in the Corona Perspectives for a spectrometer on Solar C/Plan A L. Teriaca Max-Planck-Institut für Sonnensystemforschung 09 –…

Slide 1Numerical 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 Budějovice,…

Slide 1 P.K. Manoharan Radio Astronomy Centre National Centre for Radio Astrophysics Tata Institute of Fundamental Research Ooty 643001, India [email protected] P.K.…

Slide 1 The Solar Corona and Solar Wind Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics Slide 2 The Solar Corona Plasma at T > 1 million K emits most of…

Slide 1 1 The search for signatures of ion cyclotron resonance in the low corona Laurent Dolla Jacques Solomon Philippe Lemaire Institut d'Astrophysique Spatiale [email protected]…

Slide 1 Connections Between the Magnetic Carpet and the Unbalanced Corona: New Monte Carlo Models Steven R. Cranmer & Adriaan van Ballegooijen Harvard-Smithsonian CfA,…

Slide 1 Solar/Stellar Winds: An Overview Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics (Untapped gold mines for space physicists?) Slide 2 Solar/Stellar Winds:…

Slide 1 The Dynamic Evolution of Quiet Sun Magnetic Fields in the Solar Atmosphere W.P. Abbett, Space Sciences Laboratory, Univ. of California, Berkeley [email protected]…

Slide 1 What coronal parameters determine solar wind speed? M. Kojima, M. Tokumaru, K. Fujiki, H. Itoh and T. Murakami Solar-Terrestrial Environment Laboratory, Nagoya University…

ESS 200C Lectures 6 and 7 The Solar Wind The Earth’s atmosphere is stationary. The Sun’s atmosphere is not stable but is blown out into space as the solar wind filling…