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Measuring the sun's eigenfrequencies from velocity and intensity helioseismic spectra: Asymmetrical line profile-fitting formula
R. Nigam,
A. G. Kosovichev
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peer-review
133
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Dive into the research topics of 'Measuring the sun's eigenfrequencies from velocity and intensity helioseismic spectra: Asymmetrical line profile-fitting formula'. Together they form a unique fingerprint.
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Keyphrases
Line Profiles
100%
Eigenfrequency
100%
Profile Fitting
100%
Fitting Formula
100%
Spectral Lines
50%
Michelson
50%
Power Spectrum
50%
Oscillation
25%
Intrinsic Properties
25%
Observatory
25%
Background Noise
25%
Physical Model
25%
Solar Oscillations
25%
Systematic Error
25%
Excitation Source
25%
Line Asymmetry
25%
Lorentzian
25%
Engineering
Eigenfrequencies
100%
Line Profile
100%
Power Spectra
50%
Spectral Line
50%
Intrinsic Property
25%
Physical Model
25%
Excitation Source
25%
Systematic Error
25%
Earth and Planetary Sciences
Line Spectra
100%
Power Spectra
100%
Solar Oscillation
50%
Systematic Error
50%
Background Noise
50%
Physics
Line Spectra
100%
Power Spectra
100%
Solar Oscillation
50%