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Exploring the Connection between Helioseismic Travel Time Anomalies and the Emergence of Large Active Regions during Solar Cycle 24
Published 2023-01-01Subjects: Get full text
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Asphericity of the Base of the Solar Convection Zone
Published 2024-01-01Subjects: Get full text
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23
Connection between Subsurface Layers and Surface Magnetic Activity over Multiple Solar Cycles Using GONG Observations
Published 2024-01-01Subjects: Get full text
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24
Deciphering Solar Magnetic Activity: On Grand Minima in Solar Activity
Published 2015-07-01Subjects: Get full text
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Radial gradient of the solar rotation rate in the near-surface shear layer of the Sun
Published 2022-12-01Subjects: Get full text
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Identifying Acoustic Wave Sources on the Sun. II. Improved Filter Techniques for Source Wavefield Seismology
Published 2023-01-01Subjects: Get full text
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28
Minuscule Corrections to Near-surface Solar Internal Rotation Using Mode Coupling
Published 2023-01-01Subjects: “…Helioseismology…”
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29
Helioseismic Investigation of Quasi-biennial Oscillation Source Regions
Published 2023-01-01Subjects: Get full text
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30
Waves from the Sun: to the 100th anniversary of V.A. Troitskaya’s birth
Published 2017-09-01Subjects: Get full text
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31
Removal of Active Region Inflows Reveals a Weak Solar Cycle Scale Trend in the Near-surface Meridional Flow
Published 2023-01-01Subjects: Get full text
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32
Highly Energetic Electrons Accelerated in Strong Solar Flares as a Preferred Driver of Sunquakes
Published 2023-01-01Subjects: Get full text
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33
Generation of the toroidal magnetic field in the radiant zone of the Sun and alternation of the amplitude of the neighboring magnetic cycles
Published 2019-12-01Subjects: Get full text
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34
Differential rotation, radiative equilibrium, and local hydrodynamic stability in stellar interiors
Published 2016“…In particular:</p> <ol type="a"><li>The data from helioseismology show that the upper radiative zone of the Sun is in near-uniform rotation, but they have a significant uncertainty. …”
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Observational Evidence of Shallow Origins for the Magnetic Fields of Solar Cycles
Published 2018-05-01“…Observational evidence for the origin of active region magnetic fields has been sought from published information on extended solar cycles, statistical distributions of active regions and ephemeral regions, helioseismology results, positional relationships to supergranules, and fine-scale magnetic structure of active regions and their sunspots during their growth. …”
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Solar Surface Convection
Published 2009-04-01“…One of the most noteworthy results has been a significant reduction in recent years in the derived solar C, N, and O abundances with far-reaching consequences, not the least for helioseismology.Convection in the solar surface layers is also of great importance for helioseismology in other ways; excitation of the wave spectrum occurs primarily in these layers, and convection influences the size of global wave cavity and, hence, the mode frequencies. …”
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Large-Scale Dynamics of the Convection Zone and Tachocline
Published 2005-04-01“…The past few decades have seen dramatic progress in our understanding of solar interior dynamics, prompted by the relatively new science of helioseismology and increasingly sophisticated numerical models. …”
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Radiation burnthrough measurements to infer opacity at conditions close to the solar radiative zone–convective zone boundary
Published 2023“…An increased radiative opacity of the solar mixture, in particular iron, is a possible explanation for the disagreement in the position of the solar convection zone-radiative zone boundary as measured by helioseismology and predicted by modeling using the most recent photosphere analysis of the elemental composition. …”
Journal article