How TresEclipses works

A high-level explanation: precise astronomy, real terrain and a score designed to compare observing locations.

1

Eclipse astronomy

We calculate the relative position of the Sun and Moon for each moment and location. That gives the local eclipse type, contacts, magnitude, obscuration and central-phase duration.

2

Terrain and horizon

We use digital elevation models to estimate which part of the sky is visible from the observing point and which terrain obstacles appear in each direction. Trees, buildings and other artificial structures are not included.

3

Path over the relief

We cross-check the Sun and Moon path against the horizon profile. This helps detect whether a mountain could block the Sun during maximum eclipse or before totality.

4

Visibility score

The result is summarized as a score from 0 to 100. It is a guide for comparing places, not a guarantee of weather, access or safety.

5

Visual simulation

The horizon view helps you understand how the Sun and Moon will move from that exact point and which moments deserve extra attention.

From map to horizon

Two views for better decisions

First you compare areas with the score map. Then you drop down to the horizon profile to see whether the Sun is actually clear at the important moments of the eclipse. On large screens you can view both side by side. On smaller screens you can switch between them with the two-arrow button at the top right.

Mobile view of the TresEclipses simulator score map
Visibility map
Mobile animation of the TresEclipses horizon simulation
Animated horizon
TresEclipses simulator showing the best viewpoints in an area with score and eclipse data

Viewpoints

Find the best viewpoints in each area

The simulator shows the ten viewpoints with the best score inside the area you are viewing. You can open each one to compare score, totality duration, obscuration and terrain visibility, and save the places you care about for eclipse day.

  • Score calculated with real astronomy and each viewpoint's terrain horizon
  • Compare how long totality or annularity lasts at each point
  • Save your favourites and keep them ready on eclipse day
Open simulator

What goes into the score

A guide for ranking options

The score does not decide for you. It reduces a complex situation to a clear signal so you can choose, compare and prepare alternatives.

Local type

Distinguishes whether the eclipse is total, annular, partial or outside the useful observing zone from that point.

Duration

Evaluates how long the central phase lasts when totality or annularity exists.

Coverage

Takes magnitude and obscuration into account: how much of the solar disk is covered by the Moon.

Real horizon

Cross-checks the Sun path with mountains and relief to estimate whether the key moments will be visible.

The final check is always practical

Before travelling, check the weather forecast, access, permissions, road safety and real conditions at the site. TresEclipses helps you choose better, but it does not replace on-the-ground planning.