PM Sun Sight / Running Fix

Afternoon sun sight, then Sun-Run Fix — FairWinds advances your AM LOP by the boat track and crosses it with the PM LOP.

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When

Two Daily Schedule steps share this afternoon window:

Schedule step What to do
PM Sun Sight (required) Take the afternoon sun sight
Sun-Run Fix (required) Select AM + PM sights and compute the running fix

After the noon window → sunset. The engine accepts pairs from 30 minutes to 12 hours apart on the same day and refuses a pair whose LOPs cross under 5°; the Sun Worksheet grades the crossing angle, and anything under 15–20° will magnify small errors several times over. What makes a good pair depends on how high the sun goes:

Longer runs also mean a longer DR leg carrying error into the fix, which is the other reason to keep the pair tight.

In FairWinds (Guided)

1. Take the PM sight

  1. Sun tab → Sextant → shoot the sun → Save
  2. Confirm a PM badge on the new Sun Sights row

2. Compute the Sun-Run Fix

  1. Still on the Sun tab, check exactly two sights (your AM and PM)
  2. The Sun Worksheet shows Running Fix with Course / Speed / Elapsed / Run — the vector between the two positions stamped on the sights (see below). If Run reads 0.0 NM with hours between the sights, stop: both sights were stamped with the same static reference and the fix will be wrong
  3. Tap Compute Running Fix
  4. Optional: Plot Running Fix
  5. Tap Save to Log

Saved as a Sun run fix in Positions.

FairWinds does not advance a noon latitude line against a single PM LOP for this step. The product path is sun-run-sun: AM LOP advanced by the logged run, crossed with the PM LOP.

How the run is calculated

This is the classic sun-run-sun, done with the two positions stamped on the sights instead of a log reading:

  1. Each sight stores its UTC and the position shown under Reference from at the moment it was saved (its DR stamp).
  2. The AM LOP is reduced from the AM stamp and the PM LOP from the PM stamp (intercept and azimuth from each sight's own assumed position).
  3. The run is the vector from the AM stamp to the PM stamp — course and distance, exact, no rounding. The displayed speed is distance / elapsed.
  4. The AM LOP is moved by that vector and crossed with the PM LOP. That intersection is the fix.

FairWinds never reads the boat's course or speed for this. The run is entirely the difference between the two stamps, so what the reference dropdown was set to at each sight decides everything:

Reference at both sights Run used Result
GPS — current position (Guided default) True net displacement between the sight times Exact; course changes between sights do not matter
Auto — DR projected (a DR mark with course and speed) The DR mark's course × speed × elapsed Correct if the DR is; the fix corrects the DR. Lay a new DR mark at each course or speed change
Auto — Latest fix, a specific fix, DR mark or Start line Zero — both stamps identical AM line never advanced; fix off by about the real run
Two different static references The vector between those two marks Not your run; fix off by the difference

The stamps are fixed once saved; changing the dropdown or adding a DR afterwards does not rewrite older sights. Full table of what each option resolves to: Position reference, DR and the run.

Timing: Hs, UTC, Hc and Zn are all taken at the instant you press Mark, so the time you spend on the result card before Save does not affect the sight.

Why it matters

This is your main afternoon full fix when you are working the sun. It confirms the morning work and gives you a fresh position before sunset and evening twilight.

Expert mode

Auto Compute Running Fix is hidden. Reduce both sights externally, advance the AM line by your run, then Fixes tab → Enter Fix → Running Fix.


Required — afternoon position and DR reset for the evening.