Comparing the Hinode and SOHO/MDI Data to the Simulated Large Scale Solar Convection

Details Comparing the Hinode and SOHO/MDI Data to the Simulated Large Scale Solar Convection Comparing the Hinode and SOHO/MDI Data to the Simulated Large Scale Solar Convection

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..415..421g&link_type=abstract

The Second Hinode Science Meeting: Beyond Discovery-Toward Understanding ASP Conference Series, Vol. 415, proceedings of a meeti

Astronomy and Astrophysics

Astronomy

Scientific paper

Large-scale simulations of solar turbulent convection produce realistic data and provide a unique opportunity to study solar oscillations and test various techniques commonly used for the analysis of solar observations. We applied helioseismic methods to the sets of simulated as well as observed data and find remarkable similarities. Power spectra, k-ν diagrams, time-distance diagrams exhibit similar details, although sometimes subtle differences are present.

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