Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978clus.nasa..118v&link_type=abstract
In JPL A Close-up of the Sun p 118-131 (SEE N78-32964 23-92)
Astronomy and Astrophysics
Astronomy
Coronagraphs, High Resolution, Mathematical Models, Solar Corona, Ultraviolet Astronomy, X Ray Imagery, Data Reduction, Emission Spectra, Mission Planning, Solar Probes, Solar Radiation
Scientific paper
Very high resolution stereoscopic images of high temperature loop structures observed at UV and X-ray wavelengths in the solar corona can be used to understand physical processes in the corona. An existing computational model is described and sample results are given to demonstrate that computational modeling of coronal structures can indeed take advantage of very high resolution images. The sample results include the run of temperature and number density along a typical loop and the variation of the differential emission measure with temperature. The integration of the differential emission measure with temperature along a column commensurate with an instrument's spatial resolution is the relevant parameter obtained from UV and X-ray observations. The effects of loop geometry and energy input are examined.
Antiochos Spiro K.
Underwood James H.
Vesecky John F.
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