Emerging flux, magnetic reconnection, plasma turbulence and waves in the transition zone of the solar atmosphere

Details Emerging flux, magnetic reconnection, plasma turbulence and waves in the transition zone of the solar atmosphere Emerging flux, magnetic reconnection, plasma turbulence and waves in the transition zone of the solar atmosphere

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.275...95b&link_type=abstract

In ESA, Proceedings of the 21st ESLAB Symposium on Small Scale Plasma Processes in the Solar Chromosphere/Corona, Interplanetary

Physics

2

Magnetic Field Reconnection, Magnetic Flux, Plasma Turbulence, Plasma Waves, Solar Corona, Solar Magnetic Field, Solar Prominences, Solar Energy Conversion, Solar Wind, Spacelab Payloads, Ultraviolet Spectroscopy

Scientific paper

Ultraviolet spectroscopy of the solar transition zone, especially Spacelab 2 results, is reviewed. Emerging magnetic flux is considered as the energy source of the solar corona and the solar wind. The conversion of magnetic into kinetic energy is facilitated in the transition zone because of unique conditions. Radiation losses are sufficient to create fast instabilities. Observed nonthermal velocities in spectra of the transition zone indicate the existence of strong plasma oscillations and turbulence. The small filling factor of the transition zone indicates a highly filamentary structure of density, magnetic field strength, and currents, which results in rapid reconnection time scales. Particle acceleration and the heating of the corona are placed in the areas of strong plasma oscillations of the transition zone.

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