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Svenarodni opadanje motor kosovichev and duvall 1997 gabor Perioperativno razdoblje dozivati Provodljivost

Time Distance Study of Isolated Sunspots
Time Distance Study of Isolated Sunspots

Time Distance Study of Isolated Sunspots – arXiv Vanity
Time Distance Study of Isolated Sunspots – arXiv Vanity

Time-Distance Helioseismology of Sunspots
Time-Distance Helioseismology of Sunspots

ÈRay paths for modes with a horizontal phase speed of 65 km s~1 in the... |  Download Scientific Diagram
ÈRay paths for modes with a horizontal phase speed of 65 km s~1 in the... | Download Scientific Diagram

PDF) Implementation and Comparison of Acoustic Travel-Time Measurement  Procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic  Imager Time – Distance Helioseismology Pipeline
PDF) Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager Time – Distance Helioseismology Pipeline

arXiv:1209.4877v1 [astro-ph.SR] 21 Sep 2012
arXiv:1209.4877v1 [astro-ph.SR] 21 Sep 2012

SYSTEMATIC CENTER-TO-LIMB VARIATION IN MEASURED HELIOSEISMIC TRAVEL TIMES  AND ITS EFFECT ON INFERENCES OF SOLAR INTERIOR MERIDIO
SYSTEMATIC CENTER-TO-LIMB VARIATION IN MEASURED HELIOSEISMIC TRAVEL TIMES AND ITS EFFECT ON INFERENCES OF SOLAR INTERIOR MERIDIO

Towards Waveform Heliotomography: Observing Interactions of Helioseismic  Waves with a Sunspot
Towards Waveform Heliotomography: Observing Interactions of Helioseismic Waves with a Sunspot

Comparison of Travel-Time Definitions
Comparison of Travel-Time Definitions

Subsurface Supergranular Vertical Flows as Measured Using Large Distance  Separations in Time–Distance Helioseismology
Subsurface Supergranular Vertical Flows as Measured Using Large Distance Separations in Time–Distance Helioseismology

Chapter 3 Near-surface oscillations 3.1 IntroductionW For almost two  decades, methods of local helioseismology (e.g, Hill, 1988;
Chapter 3 Near-surface oscillations 3.1 IntroductionW For almost two decades, methods of local helioseismology (e.g, Hill, 1988;

PDF) Time-Distance Helioseismology Data-Analysis Pipeline for Helioseismic  and Magnetic Imager Onboard Solar Dynamics Observatory (SDO/HMI) and Its  Initial Results
PDF) Time-Distance Helioseismology Data-Analysis Pipeline for Helioseismic and Magnetic Imager Onboard Solar Dynamics Observatory (SDO/HMI) and Its Initial Results

Comparison of Travel-Time Definitions
Comparison of Travel-Time Definitions

Probing sunspots with two-skip time–distance helioseismology
Probing sunspots with two-skip time–distance helioseismology

PDF) Validation of Helioseismology through Forward Modeling: Realization  Noise Subtraction and Kernels
PDF) Validation of Helioseismology through Forward Modeling: Realization Noise Subtraction and Kernels

Comparison of acoustic travel-time measurements of solar meridional  circulation from SDO/HMI and SOHO/MDI
Comparison of acoustic travel-time measurements of solar meridional circulation from SDO/HMI and SOHO/MDI

Time Distance Study of Isolated Sunspots – arXiv Vanity
Time Distance Study of Isolated Sunspots – arXiv Vanity

Comparison of acoustic travel-time measurements of solar meridional  circulation from SDO/HMI and SOHO/MDI
Comparison of acoustic travel-time measurements of solar meridional circulation from SDO/HMI and SOHO/MDI

Comparison of Travel-Time Definitions
Comparison of Travel-Time Definitions

ÈContour plot of the energy density E of the wave packet of at time t \...  | Download Scientific Diagram
ÈContour plot of the energy density E of the wave packet of at time t \... | Download Scientific Diagram

Inversions for Deep Solar Meridional Flow Using Spherical Born Kernels –  arXiv Vanity
Inversions for Deep Solar Meridional Flow Using Spherical Born Kernels – arXiv Vanity

arXiv:1607.05681v1 [astro-ph.SR] 19 Jul 2016
arXiv:1607.05681v1 [astro-ph.SR] 19 Jul 2016

An l−ν diagram, showing the power spectrum of p-modes sampled 20 km... |  Download Scientific Diagram
An l−ν diagram, showing the power spectrum of p-modes sampled 20 km... | Download Scientific Diagram

arXiv:astro-ph/0702499v1 19 Feb 2007
arXiv:astro-ph/0702499v1 19 Feb 2007

Evolution of subsurface flows in active regions
Evolution of subsurface flows in active regions