Correlative analysis of 2-D solar atmosphere

Details Correlative analysis of 2-D solar atmosphere Correlative analysis of 2-D solar atmosphere

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnt...16..121g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 16, no. 2, p. 121-129

Computer Science

1

Scientific paper

Correlations between various parameters of 2-D inhomogeneous time-dependent solar atmospheres are analyzed to be directly related to height-dependent correlations found on the basis of spectral simulations. We detect four photospheric regions with thermal and overshooting convection, transition zone, and fully oscillating layears. The correlations found for the model data and those computed within simulated spectral scans are a good testing tool for systems of spectral line heights if these correlations are analyzed in comparison. In particular, we examine two methods providing the heights of line core formation in LTE and show that the approach which defines this quantity as a geometrical height at the optical depth of line center τλ0 = 1 is more suitable for diagnostic purpose than the method based on depression contribution function.

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