Fire near Malay-le-Grand

48.18°N, 3.34°E · first detected on 13 July at 13:25

What the satellites measured

This fire was tracked from 13 July at 13:25 to 13 July at 14:19, through 12 satellite detections. The detected extent reaches 233 ha.

Detected extent
233 ha
Cumulative power
104 MW
Peak power, one pixel
12 MW
VIIRS and MODIS detections
12

These four figures cover the polar orbits alone, the ones that measure an area. The pass table below also counts geostationary detections, more frequent but too coarse for geometry, and its power column sums a whole pass where the peak above is that of a single pixel.

“Detected extent” is not “burned area”: it is the union of the ground footprints of the satellite pixels, and a pixel counts in full (375 m for VIIRS, 1 km for MODIS) even when only a forest edge is burning. Compared with press figures it is in practice one and a half to three times the area reported. Detections taken at the edge of the scan swath, too coarse to measure anything at all, are excluded. These figures come from thermal detection and are not an official assessment: only the emergency services and the competent authorities are authoritative.

Replay how the fire spread

The map is framed on this fire's footprint and loads only its detections. The timeline below covers the period in which satellites saw it, from the first to the last detection, with twelve hours before and twenty-four after; the ticks on the bar mark the emergency services' announcements that fall within it. The cursor opens on the most powerful pass, and playback replays the whole fire in about thirty seconds. “1 h” shows what is burning within an hour of the chosen moment : the map then follows the power curve below and empties when it falls. “24 h” stacks twenty-four hours : a fire stays visible between two satellite passes, which come two to four times a day. Both are true, but they say different things.

The detected extent

Outline of the burned area near Malay-le-Grand, drawn over satellite imagery
The outline is the union of the ground footprints of every satellite detection of this fire, from the first pass to the last. The background is the EOX cloudless Sentinel-2 mosaic, 2024 vintage: it shows the landscape BEFORE these fires, not the burn scar.

Before, after: the burn scar seen from space

Sentinel-2 satellite image of the same area near Malay-le-Grand after the fire, on 2 August 2026
Sentinel-2 satellite image of the area near Malay-le-Grand before the fire, on 18 June 2026
Before · 18 June 2026After · 2 August 2026

Sentinel-2, 10 m resolution. The dates are those of the least cloudy passes available: “after” is not the day after the fire went out, it is the first clear sky that followed. Contains modified Copernicus Sentinel-2 data (2026).

The spread, pass after pass

  1. Malay-le-Grand seen by Sentinel-2 on 10 July

    10 July

    before the fire

  2. Malay-le-Grand seen by Sentinel-2 on 13 July

    13 July

    during

  3. Malay-le-Grand seen by Sentinel-2 on 18 July

    18 July

    after

One image per usable Sentinel-2 pass, on the same framing throughout so that the comparison means something. The satellite comes back every two to five days and clouds rule out some of the passes: the gaps in the series are days without an image, not days without fire.

How the radiative power evolved

One point per satellite pass: the sum of the fire radiative power measured over the fire. This is the curve that says whether the fire eased off or picked up again, which no cumulative figure shows. The window covers 3 days; beyond that, clustering would merge two successive fires in the same place.

Fire dynamics

Loading history…

Satellite passes in detail

PassPower summed over the passDetectionsSensor
13 July at 14:1918 MW2N20
13 July at 13:2586 MW10N21

One other fire near Malay-le-Grand

Separate fires, apart in time or in space, not pieces of this one. A single municipality can have several over one summer, and a forest massif often covers more than a hundred square kilometres.

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