Observational maps of the moments of strong line profiles on the solar disk

Details Observational maps of the moments of strong line profiles on the solar disk Observational maps of the moments of strong line profiles on the solar disk

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..112..383c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 112, no. 2, 1987, p. 383-386.

Physics

2

Astronomical Maps, Astronomical Spectroscopy, Line Shape, Solar Atmosphere, Chromosphere, Spatial Distribution, Spectral Energy Distribution

Scientific paper

Using the method of solar bidimensional spectroscopy based on the Universal Birefringent Filter (UBF), the authors have determined the bidimensional maps of moments of some chromospheric lines. The observational material, referring to a quiet region on the disk center, have been acquired with the UBF of the NSO at Sacramento Peak on Aug. 27, 1985. The authors present the work in progress and the new observational aspects arising from the diagnostic method.

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