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Results of Gabor-wavelet fitting for the central frequency (ω 0 ) for... | Download Scientific Diagram
arXiv:1607.04987v1 [astro-ph.SR] 18 Jul 2016
PDF) Helioseismic Travel-Time Definitions and Sensitivity to Horizontal Flows Obtained From Simulations of Solar Convection
Time-Distance Sunspot Seismology
Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and
Subsurface structure of sunspots
Subsurface structure of sunspots
Statistics of the two-point cross-covariance function of solar oscillations | Astronomy & Astrophysics (A&A)
PDF) The Seismology of Sunspots: A Comparison of Time-Distance and Frequency-Wavenumber Methods
arXiv:1607.04987v1 [astro-ph.SR] 18 Jul 2016
Local Helioseismology of Sunspots: Current Status and Perspectives | SpringerLink
Reconstruction of Solar Subsurfaces by Local Helioseismology | SpringerLink
Time-Distance Sunspot Seismology
Implementation of Travel- Time Measurements in the HMI pipeline
ÈContour plot of the square of the vertical component of the Ñuid... | Download Scientific Diagram
Results of Gabor-wavelet fitting for the central frequency (ω 0 ) for... | Download Scientific Diagram
Results of Gabor-wavelet fitting for the central frequency (ω 0 ) for... | Download Scientific Diagram
Results of Gabor-wavelet fitting for the central frequency (ω 0 ) for... | Download Scientific Diagram
PDF) Validation of Time-Distance Helioseismology by Use of Realistic Simulations of Solar Convection
arXiv:1607.04987v1 [astro-ph.SR] 18 Jul 2016
PDF) Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager Time – Distance Helioseismology Pipeline
Results of Gabor-wavelet fitting for the central frequency (ω 0 ) for... | Download Scientific Diagram
Time-Distance Sunspot Seismology
Time--Distance Helioseismology Data Analysis Pipeline for Helioseismic and Magnetic Imager onboard Solar Dynamics Observatory (SDO/HMI) and Its Initial Results
Sub-Wavelength Resolution Imaging of the Solar Deep Interior