Solar Wind Acceleration and Waves in the Corona Perspectives for a spectrometer on Solar C/Plan A L. Teriaca Max-Planck-Institut für Sonnensystemforschung.
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.
P.K. Manoharan Radio Astronomy Centre National Centre for Radio Astrophysics Tata Institute of Fundamental Research Ooty 643001, India [email protected].
The Solar Corona and Solar Wind Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
1 The search for signatures of ion cyclotron resonance in the low corona Laurent Dolla Jacques Solomon Philippe Lemaire Institut d'Astrophysique Spatiale.
Connections Between the Magnetic Carpet and the Unbalanced Corona: New Monte Carlo Models Steven R. Cranmer & Adriaan van Ballegooijen Harvard-Smithsonian.
Solar/Stellar Winds: An Overview Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics (Untapped gold mines for space physicists?)
The Dynamic Evolution of Quiet Sun Magnetic Fields in the Solar Atmosphere W.P. Abbett, Space Sciences Laboratory, Univ. of California, Berkeley [email protected].
What coronal parameters determine solar wind speed? M. Kojima, M. Tokumaru, K. Fujiki, H. Itoh and T. Murakami Solar-Terrestrial Environment Laboratory,
The Earth’s atmosphere is stationary. The Sun’s atmosphere is not stable but is blown out into space as the solar wind filling the solar system and then.
What coronal parameters determine solar wind speed?
Design and Fabrication of a Particle-Transparent Ultraviolet Filter for Solar Wind Measurements Pran Mukherjee, Thomas H. Zurbuchen, and L. Jay Guo The.
