Three-dimensional coronal structures using Clark Lake observations

Details Three-dimensional coronal structures using Clark Lake observations Three-dimensional coronal structures using Clark Lake observations

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..150..325s&link_type=abstract

Solar Physics, vol. 150, no. 1-2, p. 325-337

Astronomy and Astrophysics

Astronomy

4

Coronal Holes, Mathematical Models, Plasmas (Physics), Radio Astronomy, Solar Corona, Solar Electrons, Solar Limb, Solar Radio Emission, Solar Temperature, Absorptivity, Angular Resolution, Brightness Temperature, Coronagraphs, Diurnal Variations, Hamiltonian Functions, Image Analysis, Image Enhancement, Mapping, Radio Telescopes, Ray Tracing, Soho Mission, Spectroheliographs

Scientific paper

We have undertaken a study of coronal features observed at meter-decameter wavelengths using the Clark Lake radioheliograph. Among the coronal structures we have studied are the radio manifestations of coronal streamers on the solar disk and above the solar limb. We have analyzed the radio data quantitatively, using ray-tracing models for comparison with the maps. Our study provides information about the streamers' three-dimensional shapes, scales, and density profiles, for comparison with related observations using white-light coronagraphs.

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