The solar O I 7773 triplet. I - Spatially resolved profiles

Details The solar O I 7773 triplet. I - Spatially resolved profiles The solar O I 7773 triplet. I - Spatially resolved profiles

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...92...47k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 92, May 1984, p. 47-51. Research supported by the Australian Research Grants Committee.

Physics

7

Oxygen Spectra, Photosphere, Solar Spectra, Spatial Resolution, Line Spectra, Magnetohydrodynamic Flow, Solar Granulation, Tables (Data), Vertical Motion

Scientific paper

The reduction of observations of the O I λ7773 triplet obtained at high spatial resolution (≡0.5arcsec) at two disk positions is described. Two sets of triplet profile data are presented at each disk position. One set represents data taken from ≡0.5arcsec regions centered on the brightest granules, while the other set represents data taken from ≡0.5arcsec regions centered on the cooler infalling intergranular material.

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