The flare-CME relationship – determining factors (if any!) Sarah Matthews, Lucie Green, Hilary Magee, Louise Harra & Len Culhane MSSL, University College.
Planets Bkup Live
Observations. The SPIRIT sometimes observes in a high-temperature Mg XII 8.42 Å line large-scale features existing many hours high in the corona (Zhitnik.
Star Properties studied so far… Period Mass Eccentricity Red shift Velocity Temperature (Wiens Law) Composition – which elements and how much of each Color.
SHINE SEP Campaign Events: Long-term development of solar corona in build-up to the SEP events of 21 April 2002 and 24 August 2002 A. J. Coyner, D. Alexander,
Conclusions. 1. Plasma parameters in the arcade: Ne ~10 10 cm -3 , Te ~6 MK.
Report on ‘Extreme Space Weather Events’ workshop that I co-organized in Boulder in June 2014
KSRBL Science Colloquium 2009 Aug 24 1 Science with the Korean Solar Radio Burst Locator (KSRBL) Dale E. Gary & Gelu M. Nita Center for Solar-Terrestrial.
THE ORIGIN OF THE SLOW SOLAR WIND
SHINE 2004 THE ORIGIN OF THE SLOW SOLAR WIND Leon Ofman Department of Physics The Catholic University of America and NASA Goddard Space Flight Center.
14 C increase 775 and 993 AD: Aurora observations in ancient times. M. A. Shea.
Astronomy Chapter 4 Review Game. Light wiz Em Waves student The Atom pro Spectrum genius 10 point 10 point 10 point 10 point 10 point 10 point 10 point.