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Kunike fire, 30 March 2026 Kunike, Kunike Barina

Out · last detection 6 Apr 2026, 14:05 UTC

The fire started on 30 March 2026 in Kunike, Sierra Leone, and satellites saw it burning for 8 days. Copernicus’s global GWIS system rebuilt a burnt perimeter of 3,921 hectares from heat detections, spread across 2 municipalities.

It is the 57th largest in Northern since 2016 (of 1112 with a page). Number 33 in Sierra Leone in 2026, of 305.

Compare with…
Burnt area
3,921ha
GWIS perimeter (Copernicus)
Duration
8days
30 Mar 2026 – 6 Apr 2026
Municipalities hit
2
chiefdoms
Started on
30 Mar
2026
Heat detections
80
in a single hotspot: 151 MW
Danger at start
5
Very low · FWI index
Average daily power
228MW
detected power per day, on average

Where it burned

HOTSPOTS BY DAY 30 Mar6 Apr
6 Apr 2026

How it evolved, day by day

30 Mar 2026 · 116 MW · 16 31 Mar 2026 · 360 MW · 17 1 Apr 2026 · 125 MW · 6 2 Apr 2026 · 686 MW · 12 3 Apr 2026 · 38 MW · 5 4 Apr 2026 · 218 MW · 8 5 Apr 2026 · 123 MW · 9 6 Apr 2026 · 155 MW · 7
30 Mar 1 Apr 2 Apr 3 Apr 5 Apr

Fire radiative power detected each day, in megawatts, and number of hotspots. The magenta bar marks the peak day.

The weather it burned in

35°high
37km/h · peak gust
29%lowest humidity

It had gone 5 days without rain (1 mm or more) when it started. Rain came after the fire: 1.3 mm on 10 Apr.

This area had burned before

66% of the perimeter overlaps earlier fires recorded since 2016: 1,790 ha in 2016, 649 ha in 2017, 321 ha in 2018, 18 ha in 2020, 820 ha in 2023. Part of it burned more than once, so the yearly figures add up to more than the 2,575 ha that had burned before.

How big is it?

10 km
It burned the equivalent of 2.5% of the area of London (39 km² against 1,583 km²).

London boundary: geoBoundaries · Office for National Statistics (Open Government Licence v3.0).

This compares size, not location: both shapes are at the same scale, north up, centred on each other.

What happened to each town

  1. Kunike where it started
    3,846 ha reached on 30 Mar
    4.8 %
  2. 100 ha reached on 30 Mar
    0.2 %

Burnt area inside each municipality, from crossing the GWIS perimeter with administrative boundaries. The distance is from the town centre to the nearest fire: staying a kilometre away does not mean it reached the houses.

The weather day by day

ECMWF ERA5 reanalysis at the fire location, the standard reference for past weather, and the Canadian Fire Weather Index (the same system Copernicus uses), computed by WorldFires from that data. Days after the fire run until the first rain.

Open-Meteo.com (CC BY 4.0) · Copernicus Climate Change Service (ERA5)

Day High Min. humidity Peak gust Rain Danger (FWI)
30 Mar 32.4 °C 46 % 30 km/h 3.9 mm Very low 5
31 Mar 32.6 °C 45 % 26 km/h 0.0 mm Moderate 12
1 Apr 33.4 °C 46 % 23 km/h 0.0 mm Moderate 14
2 Apr 34.8 °C 36 % 37 km/h 0.0 mm High 22
3 Apr 34.2 °C 32 % 35 km/h 0.0 mm High 24
4 Apr 33.9 °C 39 % 20 km/h 0.0 mm Moderate 21
5 Apr 35.2 °C 29 % 35 km/h 0.0 mm High 27
6 Apr 35.3 °C 36 % 36 km/h 0.0 mm High 28
7 Apr after 34.8 °C 35 % 33 km/h 0.0 mm High 28
8 Apr after 34.9 °C 33 % 35 km/h 0.0 mm High 30
9 Apr after 33.7 °C 46 % 31 km/h 0.2 mm High 24
10 Apr after 35.1 °C 44 % 20 km/h 1.3 mm Moderate 14

Before and after, from space

Drag the line to compare the same ground before the fire and after it.

Before · 23 Mar 2026
After · 13 Apr 2026

If the day is cloudy, change the date: each satellite passes once a day. In false colour the burnt ground looks brown or red.

The smoke

CAMS · Copernicus

On 8 April 2026 the air beside the fire reached 56 µg/m³ of PM2.5. That day averaged 40: 2.7 times the WHO daily guideline (15).

PM2.5 peak56 µg/m³
Days over the guideline13 days
PM10106 µg/m³
Optical depth1.06
28293031123456789
Good Fair Moderate Poor Very poor Extremely poor

Particles from the Copernicus CAMS model at the centre of the perimeter; these are not measurements in each town. The pale bar is the worst hour, the solid one the daily average.

Open-Meteo.com (CC BY 4.0) · Copernicus Atmosphere Monitoring Service (CAMS)

Detections table · 80Every satellite heat detection, one by one, with time, satellite, power and coordinates.
⬇ Download CSV Times in UTC. Each detection is a 375 m pixel: a large fire yields hundreds per pass.
Date and timeSatelliteFRP (MW)LatLon

Other fires nearby

All fires in Sierra Leone ›

Frequently asked questions

How long did the Kunike fire last?
GWIS (Copernicus) dates it between 30 March 2026 and 6 April 2026: 8 days between the first and last heat detection of the perimeter.
How much area did it burn?
The perimeter GWIS (Copernicus) rebuilt from heat detections is 3,921 hectares (39.2 km²). It is an estimate: official national figures may differ.
Which municipalities burned?
The fire entered 2 municipalities: Kunike (3,846 ha, 4.8 %); Kunike Barina (100 ha, 0.2 %).
What was the weather like?
During the fire the temperature reached 35.3 °C, humidity dropped to 29 % and gusts hit 37 km/h. The fire danger index (FWI) reached 28, class High.
Where does this data come from?
From the GWIS (Copernicus) burnt perimeter, NASA FIRMS VIIRS hotspots and the administrative boundaries of Sierra Leone (geoBoundaries). It is not an official report.

Where to verify it

A satellite detection is not an official report. Final figures and the fire’s status are published by each country’s emergency service.

Satellite cross-check

Does something look wrong on this page?

This page is built from satellite data and official records, and it sometimes gets things wrong: the wrong dates, the wrong town, two fires merged into one, or something that was not a wildfire at all. If you know this fire first-hand (you live nearby, saw it, fought it or reported on it), tell us what really happened and we will check it.

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How we know this
  • Perimeter: GWIS (Copernicus), rebuilt from heat detections rather than mapped on imagery; 2 polygons grouped in this page.
  • Dates from the perimeter: the VIIRS detections inside it did not change them. 80 Suomi-NPP VIIRS detections on those dates.
  • We have not matched this page with any official record.
  • Weather: Copernicus ERA5 reanalysis at the fire location, in cells of about 25 km.

How we build fire pages: methodology ›

Where this data comes from

The perimeter comes from the Copernicus Global Wildfire Information System (GWIS), which rebuilds it from MODIS and VIIRS heat detections and publishes it under CC BY 4.0. It is not measured on imagery as in Europe, so it is an estimate. Heat detections come from the VIIRS sensors aboard Suomi-NPP and NOAA-20, distributed by NASA FIRMS at 375 m resolution. Municipal boundaries come from geoBoundaries ADM3 (Creative Commons Attribution 4.0 (CC BY 4.0)). The area per municipality is computed by WorldFires by crossing the perimeter with those boundaries, so it may differ from each country’s official figure.