Semiempirical modeling of bright magnetic structures observed with Rome PSPT

Details Semiempirical modeling of bright magnetic structures observed with Rome PSPT Semiempirical modeling of bright magnetic structures observed with Rome PSPT

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..295c&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

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Solar Atmosphere: Magnetic Structures

Scientific paper

Since the beginning of 1980s, semiempirical atmospheric models designed to represent the various features across the solar disk (quiet sun, network, plage and sunspot) have followed one other. We tested the capability of those proposed by Fontenla et al. (1999) to reproduce experimental data that are different from those in which the models were verified. In particular we studied the center to limb variation of the facular and network contrast and compared the results of the computed models with those obtained analyzing the observations carried out with the PSPT at the Rome Observatory. In this way, we single out the models better reproducing the two solar features operationally identified by the PSPT data analysis.

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