Evolution of subsurface flows in active regions
1. INTRODUCTION
PDF) Time-Distance Helioseismology Data-Analysis Pipeline for Helioseismic and Magnetic Imager Onboard Solar Dynamics Observatory (SDO/HMI) and Its Initial Results
Response to Comment on “Detection of Emerging Sunspot Regions in the Solar Interior” | Science
Comparison of Travel-Time Definitions
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arXiv:0911.4295v1 [astro-ph.SR] 22 Nov 2009
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Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and
Chapter 3 Near-surface oscillations 3.1 IntroductionW For almost two decades, methods of local helioseismology (e.g, Hill, 1988;
Comparison of acoustic travel-time measurements of solar meridional circulation from SDO/HMI and SOHO/MDI
Time-Distance Helioseismology of Sunspots
Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager Time – Distance Helioseismology Pipeline | SpringerLink
Subsurface Supergranular Vertical Flows as Measured Using Large Distance Separations in Time–Distance Helioseismology
Probing sunspots with two-skip time–distance helioseismology
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Comparison of acoustic travel-time measurements of solar meridional circulation from SDO/HMI and SOHO/MDI
Towards Waveform Heliotomography: Observing Interactions of Helioseismic Waves with a Sunspot
