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Atmospheric Refraction Sunset 3D Explorer vs Twilight Types 3D Explorer


Both pages render real atmospheric optics in one page load - 0 MB installed, USD 0, no account. The Atmospheric Refraction Sunset 3D Explorer covers the SUB-DEGREE bending and color-splitting of the Sun's own disk right at the horizon; the Twilight Types 3D Explorer covers the WIDER 0-18 degree sky-brightness bands after the Sun is already below the horizon.


The numbers side by side

AspectAtmospheric Refraction Sunset ExplorerTwilight Types Explorer
Install size0 MB - runs in the browser0 MB - runs in the browser
PriceUSD 0USD 0
Angular range shownabout -1.5 to +4 degrees around the horizon0 to 18 degrees of solar depression
What it showsthe Sun's disk lifting, flattening, and color-splittingcivil, nautical, and astronomical sky-brightness bands
Real feature highlightedthe green flash, and why "sunset" is defined 50 arcminutes below the horizonwhite nights at high latitude in summer
Interactionscrub true altitude, toggle air quality and the light-bend pathscrub depression angle, latitude, and season

Where the Twilight Types Explorer wins

The Twilight Types Explorer wins when the question is how dark the whole sky gets, and for how long, once the Sun is several degrees below the horizon - including why some latitudes get white nights in summer.


Where the Atmospheric Refraction Sunset Explorer wins

The Atmospheric Refraction Sunset Explorer wins when the question is why the Sun's own disk looks flattened, sits higher than its true position, and can briefly flash green right at the horizon crossing - a sub-degree optical story the Twilight Types Explorer does not cover.


A reasonable rule

As a reasonable rule, use the Atmospheric Refraction Sunset Explorer first to see what happens to the Sun's disk itself in the last few minutes before it sets, then use the Twilight Types Explorer to see how the whole sky dims afterward.

See how to use the Atmospheric Refraction Sunset 3D Explorer for a step-by-step walkthrough.

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