Hotspots: The Foundation of Clusters

1. Hotspots

A hotspot is a thermal anomaly, often a heat source, that can indicate a potential fire.

Hotspots come from multi-spectral satellite data processed with specific algorithms that highlight areas with an unusually high temperature.

Each hotspot event has an associated location accuracy based on the satellite instrument’s pixel resolution.

This is visualized in the interface by a circle around the center of the hotspot. The accuracy (also known as GSD) is a property of the sensor (and for GEO satellites, additionally, the offset of the pixel location from the optical axis of the instrument).

In other words, Hotspots are detected using data from satellites that can sense heat. Each hotspot has a location accuracy, determined by the satellite's level of detail. Further on this article, we'll explore how the location accuracy is displayed per type of Satellite.

Each hotspot has an own menu similar to Clusters containing related information, such as:

• Details: timely and practical overview of information on what triggered the detection:
  • Acquisition Time: Time when the satellite captured and stored the image.

• • Detection Time: Time when the thermal anomaly (hotspot) was processed*

• Weather at Acquisition Time: Weather conditions when the image is captured.
• Visible Images Available: Related visual imagery.
• Scientific Data: Information about the intensity of the heat source.
• LEO Satellite Passes: Low Earth Orbit satellite confirmations of the hotspot event.

2. Satellites Used for Hotspot Detection

Previously, it had been mentioned that the size of a hotspot is linked to its accuracy. This is directly related to the type of satellite used for detection.

We work with two types of satellites:

1. LEO satellites (Low Earth Orbit) orbit close to Earth's surface, typically at altitudes less than 1,000 km. Their proximity allows them to capture detailed observations with smaller ground footprints, making them effective for detecting small fires. However, they take longer to revisit the same location, usually several days.

2. GEO satellites (Geostationary Orbit) orbit at an altitude of 35,786 km above the equator, matching Earth's rotation. This makes them appear stationary over a fixed position. They can observe half of the Earth’s surface every 15-30 minutes but with much larger ground footprints, providing broader but less detailed coverage.

Comparison between LEO and GEO Satellites

3. Differentiating Hotspots

Even though the core of information can be found in Clusters, it's important to understand how the detections differ from one another. 

Simply put, hotspot detections can vary in 2 cases:

1. Color - A hotspots color is directly associated to its age. The newer it is, the brighter it will be displayed. In this logic, older detections will be displayed in a grey tone.
2. Size - Hotspots differentiate in size based on the type of satellite and resolution of the detecting instrument (also known as GSD). The rule is straightforward: smaller hotspots indicate greater accuracy.

      _{Image of a Cluster with several hotpots differing in size and colour.}

In the image below, you can find a correlation between size and age of hotspots.

Hotspots are displayed as circles. Bigger circles are displayed as GEO detections, whereas the smaller ones are represented by LEO detections. This is directly related to GSD (pixel resolution and level of detail a satellite can capture).