Titlebook: Solar and Heliospheric Plasma Physics; Proceedings of the 8 George M. Simnett,Constantine E. Alissandrakis,Lou Conference proceedings 1997

熄灭

FRAX-tool

Observations of energetic ions during the ulysses mission,has now started on its second solar orbit. We review here energetic ion observations from the many regions encountered during the out-of-ecliptic phase of the mission: the low latitude traversal of the streamer belt, the passage through the south polar region, the fast latitude scan, and the passage

特征

Solar wind and interstellar medium coupling,nal frontiers of the solar wind, as it pushes itself into the ISM, have been an object of speculation and analysis for many years. Observational evidence from the solar wind and heliospheric energetic particles, and measurements of the very local interstellar medium (VLISM), have led to a consensus

萤火虫

Flows through the magnetically structured solar atmosphere,in the low corona but is already less than unity in the middle chromosphere. The dynamics of the chromosphere and the transition region are driven by magnetic effects, even in the “quiet” Sun. We will review some promising research programs concerning steady flows and oscillatory phenomena in the sm

同位素

高歌

Topologically forced reconnection,ing done upon it, no matter how small the electrical resistivity may be. Recent numerical experiments have clarified the mechanisms through which balance between the boundary work and the dissipation in the interior is achieved. The results largely confirm Parker’s (1972) idea of “topological dissip

死亡

合法

无王时期,

indecipherable

Future space instrumentation for solar physics,has support from Yohkoh, Coronas I and a variety of “particles and fields” spacecraft such as Polar, Wind, Geotail and Interball. The principal new facility will be the TRACE mission, which is scheduled for launch in 1997/1998. For the medium term future, missions such as the Solar Probe, Coronas-F