Dynamics of the Overshooting Photospheric Region from THEMIS-IPM Observations

Details Dynamics of the Overshooting Photospheric Region from THEMIS-IPM Observations Dynamics of the Overshooting Photospheric Region from THEMIS-IPM Observations

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp41b01b&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP41B-01

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7529 Photosphere, 7594 Instruments And Techniques, 7859 Transport Processes

Scientific paper

Here, we present the results of our investigation on quiet photospheric fields. We study the features of intensity and velocity solar fields as derived from observations of photospheric lines, obtained at the French-Italian THEMIS telescope (Observatorio del Teide, Tenerife) using the Italian Panoramic Monochromator (IPM). In detail, the vertical dynamics is investigated using monochromatic observations at three spectral lines (C I 538.0, Fe I 537.9, and Fe I 557.6), as representative of three atmospheric heights in the overshooting photosphere. Moreover, granulation properties and horizontal flows are also studied using broad band images.

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