Dynamics and Diagnostics of Explosive Events and Blinkers

Details Dynamics and Diagnostics of Explosive Events and Blinkers Dynamics and Diagnostics of Explosive Events and Blinkers

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mwoc.conf...69m&link_type=abstract

Multi-Wavelength Observations of Coronal Structure and Dynamics -- Yohkoh 10th Anniversary Meeting. Proceedings of the conferenc

Physics

Scientific paper

The knowledge of the main physical parameters of UV explosive events and blinkers, such as density and temperature, is of great importance for the better understanding of the true nature of these transient events. In this context, density and temperature diagnostics based on lines belonging to O iv 1400Å and O iii multiplets is presented for both kind of events. The dynamics of the solar transient phenomena is revealed through their temporal and spatial evolution as observed in spectral lines covering a wide temperature range. The results are obtained using SUMER, CDS, MDI and EIT aboard SoHO, TRACE and Big Bear Solar Observatory observations and are aimed to give more information about the main properties of these phenomena. The events are also studied in connection with the evolution of the underlying magnetic field, searching for observational evidences of their further propagation higher in the solar corona.

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