Axine Labs
Free / commercial imagery

Infrastructure Thermal Inertia

Apparent thermal inertia from a day and night pair: dense material against loose fill.

Day and night thermal differencing, normalised by albedo. Dense material gives up heat more slowly than loose fill.

Infrastructure Thermal Inertia
In view

Apparent thermal inertia from a day and night pair: dense material cools slowly, loose fill cools fast.

WHAT IT FINDS

What it detects.

MaterialTypical settingWhat can confuse it
Apparent Thermal Inertia (ATI) AnomaliesCivil infrastructure corridors, foundation pads, runway subgrades, and shallow buried utilitiesSurface wind gusts altering convective heat transfer

METHOD

How it works.

Calibrated reflectance goes in, and every pixel is fitted against a public reference library.

01Step 1

Pairing a day and a night pass

The midday and pre-dawn acquisitions are placed on a common grid. Both must cover the same ground inside one diurnal cycle, which is the constraint that makes this hard to procure rather than hard to compute.

02Step 2

Broadband albedo

Optical bands are integrated into a broadband albedo, which sets how much solar energy the surface took in during the day.

03Step 3

Apparent thermal inertia

ATI = (1 - α) / (T_day - T_night). The word apparent is load-bearing: this is a proxy for heat capacity and conductivity, not a measurement of either.

04Step 4

Segmentation into high and low inertia

Dense material separates from loose fill. What causes the contrast is an interpretation the map cannot make for you.

SPECIFICATIONS

What you get, and what it runs on.

Values deliveredApparent thermal inertia, floating point, unitless
OutputApparent thermal inertia surface
TurnaroundSet by the day and night acquisition window, not by processing
Formats
Cloud-Optimized GeoTIFF (COG)Vector Thermal Contours (GeoJSON)Provenance record (both acquisition times in UTC, method version)

Conditions it needs

Sun angle limit:50°
Cloud cover limit:0%
Vegetation cover limit:20%

Method and checks are documented in Axine Applied Spectroscopy Technical Whitepaper · Series 5.

Read the paper

Scope

Both passes have to be cloud-free and calm. Wind at night masks the signal this depends on.