3D reconstruction methods of coronal structures by radio observations

Details 3D reconstruction methods of coronal structures by radio observations 3D reconstruction methods of coronal structures by radio observations

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..217a&link_type=abstract

In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 217-2

Physics

4

Coronal Loops, Imaging Techniques, Radio Emission, Solar Flares, Three Dimensional Models, Magnetic Fields, Radio Observation, Solar Activity, Solar Rotation, Tomography, Very Large Array (Vla)

Scientific paper

The ability to carry out the three dimensional (3D) reconstruction of structures in the solar corona would represent a major advance in the study of the physical properties in active regions and in flares. Methods which allow a geometric reconstruction of quasistationary coronal structures (for example active region loops) or dynamic structures (for example flaring loops) are described: stereoscopy of multi-day imaging observations by the VLA (Very Large Array); tomography of optically thin emission (in radio or soft x-rays); multifrequency band imaging by the VLA; and tracing of magnetic field lines by propagating electron beams.

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