Monte Carlo simulation of solar p-mode profiles revisited: Bias and uncertainty estimation from one, not many, fits

Details Monte Carlo simulation of solar p-mode profiles revisited: Bias and uncertainty estimation from one, not many, fits Monte Carlo simulation of solar p-mode profiles revisited: Bias and uncertainty estimation from one, not many, fits

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...433..713t&link_type=abstract

Astronomy and Astrophysics, Volume 433, Issue 2, April II 2005, pp.713-715

Astronomy and Astrophysics

Astrophysics

5

Methods: Data Analysis, Methods: Statistical, Sun: Helioseismology

Scientific paper

It is quite common in helioseismology to use extensive Monte Carlo simulations to investigate the bias and associated uncertainties in fitted p-mode parameters. This can, however, be very time-intensive if the fitting problem is complicated or large datasets (in time or resolution) are involved. Here, we show that it is often possible to reduce significantly the task by taking advantage of the statistical properties of the p-mode profiles.

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