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Helioseismology Sun Oscillation 3D Explorer vs alternatives

Helioseismology Sun Oscillation 3D Explorer lets a reader see a simplified 3D model of the Sun's five-minute surface oscillation and toggle straight to the interior boundary it reveals - a SOHO/GONG/SDO-HMI data archive wins as the fixed, citable source for actual observational data; a textbook diagram wins for a quick static summary without needing WebGL.

OptionStrengthAccessTrade-off
Helioseismology Sun Oscillation 3D Explorer (this page)Interactive 3D visualization of the oscillation pattern and the interior boundary it reveals, with an amplitude slider and mode cyclingFree, in browserSimplified pattern, not real observational data
SOHO / GONG / SDO-HMI data archiveThe fixed, citable, official source for real helioseismic observations and inversionsFree, official science archivesRequires domain expertise to interpret; no interactive 3D model
Textbook diagramQuick static summary of the technique, no WebGL neededReference textsNo animation, no adjustable amplitude or mode cycling

Key published figures

FigureValue
Oscillation periodabout 5 minutes (about 3 mHz)
Resonant modes trackedmillions, via SOHO / GONG / SDO-HMI
Measured convection-zone base0.713 +/- 0.001 solar radii
Tachocline locationabout 0.69-0.72 solar radii

Start with the step-by-step guide or when to use. Open the Helioseismology Sun Oscillation 3D Explorer.


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