Diagnostics of solar coronal loops at interferometric angular resolution

Details Diagnostics of solar coronal loops at interferometric angular resolution Diagnostics of solar coronal loops at interferometric angular resolution

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987esasp.273..217f&link_type=abstract

In ESA, ESA Workshop on Optical Interferometry in Space p 217-219 (SEE N88-10613 01-74)

Astronomy and Astrophysics

Astronomy

Angular Resolution, Coronal Loops, Interferometry, Ultraviolet Astronomy, Density Distribution, Extreme Ultraviolet Radiation, Fine Structure, Temperature Gradients

Scientific paper

The advent of very high angular resolution (equivalent to 20 km on the sun) for extreme ultraviolet observations would allow to diagnose the fine structure in density and temperature of solar coronal loops. In the framework of the variety and uncertainties of the existing theoretical models of loops, the high angular resolution is of particular importance to estimate the filling factor of loops by hot and cool material, to measure radial gradients of temperature and density, to observe flows, spatiotemporal evolution due to heating mechanisms and interaction between loops.

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