The map shows thermal anomalies detected by satellites during the selected period. Detections are shown not only in Armenia but also in nearby regions of neighbouring countries. The data comes from NASA FIRMS and is updated on AirQuality.am every 30 minutes.
Brighter icons indicate more recent detections. The number on an icon is the count of grouped satellite detections. Select an icon for details.
| Detection time | Location | Source | Confidence | FRP |
|---|---|---|---|---|
| 30.08.2026, 04:01 |
دهستان گجلرات شرقی, West Azerbaijan Province, Iran 39.11042, 45.32948 |
VIIRS / NOAA-21 | nominal | 2.5 MW |
|
30.08.2026, 03:14
3 detections |
Monteavan, Armavir Province, Armenia 40.20530, 44.31101 |
VIIRS / NOAA-20, MODIS | nominal | 19.7 MW |
|
30.08.2026, 02:20
2 detections |
دهستان گجلرات غربی, West Azerbaijan Province, Iran 39.11703, 45.15048 |
VIIRS / NOAA-21 | nominal | 5.5 MW |
| 29.08.2026, 20:48 |
Shahumyan, Armavir Province, Armenia 40.20251, 44.29128 |
MODIS | nominal | 8.8 MW |
|
29.08.2026, 14:56
4 detections |
Syunik Province, Armenia 39.54150, 46.39723 |
VIIRS / NOAA-20, VIIRS / Suomi NPP | high | 24.4 MW |
|
29.08.2026, 14:56
6 detections |
Syunik Province, Armenia 39.45331, 46.30827 |
VIIRS / NOAA-20, VIIRS / Suomi NPP, VIIRS / NOAA-21 | nominal | 13.4 MW |
| 29.08.2026, 14:36 |
Vagharshapat, Armavir Province, Armenia 40.18370, 44.28732 |
VIIRS / Suomi NPP | nominal | 3 MW |
| 29.08.2026, 14:36 |
Masis, Ararat Province, Armenia 40.04773, 44.41767 |
VIIRS / Suomi NPP | low | 5.3 MW |
|
29.08.2026, 14:36
4 detections |
دهستان دیزمارشرقی, East Azerbaijan Province, Iran 38.81098, 46.59820 |
VIIRS / Suomi NPP, VIIRS / NOAA-21, VIIRS / NOAA-20 | nominal | 7.4 MW |
| 29.08.2026, 14:00 |
Armavir Province, Armenia 40.13742, 44.09399 |
VIIRS / NOAA-21 | nominal | 2.7 MW |
| 29.08.2026, 14:00 |
Iğdır, Turkey 39.95923, 44.00295 |
VIIRS / NOAA-21 | nominal | 4.6 MW |
| 29.08.2026, 13:15 |
Samukh District, Azerbaijan 40.70210, 46.45733 |
VIIRS / NOAA-20 | nominal | 2.9 MW |
Times are shown in the Yerevan time zone. Detections within 1 km are grouped; the latest detection, highest confidence and maximum FRP are shown. A group is not a separately confirmed fire.
Approximate English location names are obtained from © OpenStreetMap contributors.
The MODIS and VIIRS satellite instruments observe Earth in visible and infrared wavelengths. Infrared channels are especially important for fire detection: the algorithm uses them to identify pixels that are significantly hotter than the surrounding surface. These points are called active fires or thermal anomalies.
MODIS, the Moderate Resolution Imaging Spectroradiometer, was developed as one of the main instruments in NASA's long-term Earth observation programme. The first instrument reached orbit aboard Terra in December 1999, followed by a second aboard Aqua in May 2002. MODIS observes not only fires but also clouds, aerosols, vegetation, snow, ice and the oceans. Its active-fire data has a resolution of about 1 km.
VIIRS, the Visible Infrared Imaging Radiometer Suite, continued this observation record with better sensitivity to smaller fires: its active-fire product has a resolution of about 375 m. The first VIIRS instrument was launched aboard Suomi NPP in October 2011. Similar instruments followed on NOAA-20, launched in November 2017, and NOAA-21, launched in November 2022. Because several satellites pass over the same area at different times, one fire can be detected repeatedly.
FIRMS was developed by the University of Maryland with support from NASA and the UN Food and Agriculture Organization. Its purpose is to turn satellite observations into an accessible active-fire map quickly. FIRMS publishes processed observations in near real time, but not instantly: several hours may pass between an overpass and a point appearing on the map.
A point on the map is not an official confirmation of a fire. Industrial facilities, flares, hot surfaces or other heat sources can also produce a thermal anomaly. Clouds and smoke can sometimes prevent a satellite from detecting a fire.
Nearby detections are grouped, but a large or long-running fire may still form more than one group. Coordinates mark the average centre of a group's detections and do not show the exact fire boundary.