scholarly journals A METHOD FOR THE ESTIMATION OF $p$-MODE PARAMETERS FROM AVERAGED SOLAR OSCILLATION POWER SPECTRA

2015 ◽  
Vol 803 (2) ◽  
pp. 92 ◽  
Author(s):  
J. Reiter ◽  
E. J. Rhodes Jr. ◽  
A. G. Kosovichev ◽  
J. Schou ◽  
P. H. Scherrer ◽  
...  
Keyword(s):  
Power Spectra ◽  
Solar Oscillation ◽  
Oscillation Power

Modeling of solar oscillation power spectra

1990 ◽  
Vol 364 ◽  
pp. 699 ◽  
Author(s):  
Edwin R. Anderson ◽  
Thomas L., Jr. Duvall ◽  
Stuart M. Jefferies
Keyword(s):  
Power Spectra ◽  
Solar Oscillation ◽  
Oscillation Power

A Method for the Estimation of f- and p-mode Parameters and Rotational Splitting Coefficients from Un-averaged Solar Oscillation Power Spectra

2020 ◽  
Vol 894 (1) ◽  
pp. 80
Author(s):  
J. Reiter ◽  
E. J. Rhodes ◽  
A. G. Kosovichev ◽  
P. H. Scherrer ◽  
T. P. Larson ◽  
...  
Keyword(s):  
Power Spectra ◽  
Solar Oscillation ◽  
Oscillation Power

scholarly journals Limits on radial differential rotation in Sun-like stars from parametric fits to oscillation power spectra

2017 ◽  
Vol 603 ◽  
pp. A6 ◽  
Author(s):  
M. B. Nielsen ◽  
H. Schunker ◽  
L. Gizon ◽  
J. Schou ◽  
W. H. Ball
Keyword(s):  
Differential Rotation ◽  
Power Spectra ◽  
Oscillation Power

scholarly journals High-Frequency Solar Oscillations

1998 ◽  
Vol 185 ◽  
pp. 415-422
Author(s):  
Stuart M. Jefferies
Keyword(s):  
Power Spectrum ◽  
High Frequency ◽  
The Sun ◽  
Solar Oscillation ◽  
Solar Oscillations ◽  
Oscillation Power ◽  
Peak Structure ◽  
Source Of Information

This paper reviews the properties of the solar oscillation power spectrum at frequencies near and above the acoustic cut-off frequency for the atmosphere. This region of the spectrum contains over 50% of the total peak structure observed and is a source of information not only on the outer layers of the sun and the origin of solar oscillations, but also on the physics of the solar core and chromosphere.

scholarly journals Observation of Low-Degree Modes from SOHO/MDI Using Optimal Masks

1998 ◽  
Vol 185 ◽  
pp. 179-180
Author(s):  
T. Toutain ◽  
A. Kosovichev ◽  
T. Appourchaux
Keyword(s):  
Power Spectra ◽  
Rotational Frequency ◽  
Mode Frequency ◽  
Michelson Doppler Imager ◽  
Oscillation Power ◽  
Frequency Measurements ◽  
Frequency Splitting ◽  
Doppler Imager ◽  
Low Degree

The overlap of peaks of split multiplets in oscillation power spectra and the leakage of other degree modes could significantly affect the measurements of the rotational frequency splitting. We have developed optimal masks which allow to isolate individual components of the multiplets. The method is applied to the Michelson Doppler Imager Low-l data. The results of the mode frequency measurements are reported.

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