Sunrise, sunset and twilight calculations using the Air Almanac. Polar day, polar night, and high-latitude phenomena.
Local noon occurs at the same Local Mean Time on all meridians — it is always 1200 LMT. By extension, sunrise and sunset occur at the same LMT at all places on the same parallel of latitude, on any given day.
📌 Sunrise LMT and Sunset LMT are the same at a given latitude on a given date, regardless of longitude.
📌 To find UTC of sunrise/sunset: look up LMT from Air Almanac → convert using arc-to-time for your longitude.
📌 As the Sun rises due East and sets due West only at the equinoxes — at other times of year, the Sun rises/sets north or south of East/West.
The combination of Earth's axial tilt and high latitudes produces remarkable seasonal effects:
| Phenomenon | Condition | Where? | When (NH)? |
|---|---|---|---|
| Midnight Sun (☀️ all day) | Sun above horizon 24 hrs | 66°N and higher | Around 21 June |
| Polar Night (❄️ all night) | Sun below horizon 24 hrs | 66°N and higher | Around 21 December |
| Equal Day/Night | 12 hrs day, 12 hrs night | Equator (all year) | Equinoxes (all lat) |
The lowest latitude at which Midnight Sun occurs is approximately 66°N/S — the Arctic/Antarctic Circle — on the relevant solstice. In the Air Almanac, this is listed as approximately 66N for June and 66N for December polar night (when the question asks for lowest latitude where Sun never rises).
Twilight is the period before sunrise and after sunset when the Sun is below the sensible horizon but still illuminates the sky. It is defined by how far the centre of the Sun is below the sensible horizon.
Sun 0° to 6° below horizon
Enough light for most outdoor tasks
Used in EU-OPS day/night definition
Sun 6° to 12° below horizon
Horizon visible, stars visible for navigation
Used by mariners for star sights
Sun 12° to 18° below horizon
Sky not completely dark
Ends when full darkness begins
Civil Twilight definition (full):
• The period between sunset and End of Evening Civil Twilight (ECT)
• The period between Start of Morning Civil Twilight (MCT) and sunrise
• Related to the centre of the Sun being 6° below the sensible horizon
• A period when it is possible to carry out daylight tasks without artificial lighting
• Used in the EU-OPS definition of day flying / night flying
Air Almanac Abbreviations:
Despite popular belief, it is not immediately dark after sunset at the Equator. Civil twilight still exists. However, because at the Equator the Sun sets almost vertically (perpendicular to the horizon), the twilight period is short.
Between 60°N and 60°S, the minimum duration of civil twilight is 21 minutes. This occurs at the Equator at the equinoxes, when the Sun sets most steeply.
As latitude increases, the Sun's path makes a shallower angle with the horizon at sunset. This means it takes longer for the Sun to descend through the 6° zone, so twilight duration increases with latitude.
In polar and sub-polar regions, extraordinary effects can occur:
Permanent Twilight (////) — In high latitudes in summer, the Sun may remain within 6° of the horizon all night. It never rises (so no sunrise time listed) but never reaches true darkness — this is shown as "//// " in the Air Almanac, indicating permanent civil twilight through the night.
The Air Almanac tables assume a sea-level observer. An aircraft at altitude has a depressed sensible horizon (the dip increases with altitude).
🛩 At FL350, the depression of the horizon is approximately 3°.
⬆ Sunrise is earlier — you can see the Sun before it rises above the sea-level horizon.
⬇ Sunset is later — you can still see the Sun after it has set at sea level.
⏱ Duration of twilight is shorter — because the Sun must travel 6° below the depressed sensible horizon (not the geometric horizon), and with the horizon already depressed by ~3°, this 6° arc is covered faster.
The Air Almanac sunrise/sunset tables list LMT times for specific latitudes at 3-day intervals. To use them for an arbitrary position:
Step 1 — Interpolate for exact latitude between the two tabulated latitudes.
Step 2 — Interpolate for date between the two bracketing dates in the table.
Step 3 — Result is LMT of sunrise/sunset at your latitude.
Step 4 — Convert LMT → UTC using arc-to-time for your longitude (East: subtract; West: add).
Step 5 — If Standard Time is required, apply ST correction to UTC.