Solar noise simulations in irradiance

Details Solar noise simulations in irradiance Solar noise simulations in irradiance

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..152..247a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 152, no. 1, p. 247-252

Physics

16

Brightness Distribution, Decay Rates, Gravity Waves, Low Frequencies, Noise Spectra, Solar Atmosphere, Solar Granulation, Astronomical Photometry, Nonoscillatory Action, Observability (Systems), Stellar Models

Scientific paper

The global signature of granulation, meso- and supergranulation is calculated using values for intensities and lifetimes from spatially resolved observations. These simulations are compared with observations from Active Cavity Radiometer Irradiance Monitor (ACRIM), IPHIR and the Solar Variability, Experiment 1 (SOVA-1) photometers. The results indicate that the overall shape of the background signal in the simulations reproduce the observations at low frequency. However when the granulation lifetimes are about 500 seconds the simulated data do not correspond to the observations between 1 and 2 mHz.

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