Elevation

Solar elevation instrument

Model · clear sky, sea level

Live

01 Now

Where the sun is

The sun's angle above the horizon at this moment, and what that angle puts in the light reaching you.

Elevation

—

degrees above the horizon — 0° is sunrise or sunset, 90° is directly overhead

Loading the selected sky.

  • Visible light—
  • UVA—
  • UVB—
Fig. 01 — the check you can make yourself
A stick and its shadow at the selected solar elevation —

Cloud and aerosol reduce UVB more than visible light, so on an overcast day the real UVB is lower than shown while the daylight looks much the same.

02 Today Drag to scrub · release for live

Sun through the day

How the angle moves from sunrise to sunset, and which hours actually carry vitamin D and sunburn.

The black line is the sun's height through the day; the two bars beneath it show what that height delivers. The sunburn bar starts earlier and finishes later than the vitamin D bar — the shaded columns are those hours, when you can still burn and synthesis has already stopped.

The background colour is the sun's own colour at that height.

Colour strength in the two bars is logarithmic, and each bar is measured against its own best moment today. A full-strength bar in winter at a high latitude can still be very little light in absolute terms; the year map below is where that comparison is made honestly.

03 Why Drag to orbit · slide the latitude

Why the sun's arc tilts

The sun's daily path across the sky dome at the two solstices, and the cone it has to enter before vitamin D synthesis has light to work with.

The two solid arcs are the sun's path on the June and December solstices; the dashed one is the date you have selected. The cone sits at 45°, and the circle on the ground has the figure's own height for its radius: the sun is inside the cone exactly when your shadow is shorter than you are. Slide the latitude below — past roughly 20°N the December arc stops entering that cone for months on end, and past roughly 67°N it stops clearing the horizon entirely.

19°N

Hours above 45°

04 Year Hover a cell · drag the latitude

Every day of the year

The same reading repeated for all 365 days, at any latitude — where the vitamin D window opens, and where it closes.

Each cell is coloured by how high the sun is at that moment, and the dashed line rings the region where enough UVB reaches the ground for vitamin D synthesis to run. Drag the latitude slider upward and watch that region close: past roughly 37° a hole opens through the middle of the year — months during which the sun never climbs high enough, on any day, at any hour.

19°N

The dashed line marks where the vitamin D index reaches roughly 2% of the clear-sky planetary maximum. It is a soft boundary, not a switch: nothing changes abruptly when you cross it.

05 You

Your day in words

A plain-text summary of the selected day, written for the skin type you pick below.

Skin type

Darker skin needs proportionally longer exposure for the same effect, so the burn estimate changes with this setting; pick the closest match on the Fitzpatrick scale, I (always burns) to VI (never burns). Adjacent types overlap substantially in the literature, and the exposure multiplier between them is a wide range, not a settled number.