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The H₂ Sensing Compendium

Why hydrogen is uniquely hard to sense, every way people sense it anyway, and which hardware to trust in the field. Built by and for Hestia Energy's geologic hydrogen exploration team.

Thirty-plus deeply technical pages on how hydrogen is detected — each starting from the physical mechanism, carrying a figures-of-merit table, and ending with a field verdict for geologic H₂, all citing sources you can hand to anyone who asks. Every quantitative claim was checked against its live source in an adversarial verification pass. New readers should start with the Foundations ladder; specialists can jump straight to the sensor taxonomy.

Nobody should read this wiki cover to cover. Pick the path that matches what you came for:

The constraint everything else follows from

Section titled “The constraint everything else follows from”

Hydrogen gives a sensor very little to work with. It is a symmetric two-atom molecule with no permanent dipole, so it is invisible to the infrared methods (NDIR, TDLAS, FTIR) that make cheap CO₂ and methane sensors possible; its electronic transitions sit in the vacuum ultraviolet where air is opaque. What remains is a short list of physical handles — polarizability (Raman), outlier thermal conductivity and speed of sound, catalytic reactivity on palladium and platinum, Pd-hydride formation, and electrochemistry — and every sensor built for H₂ exploits one of them. The wiki is organized around that list. Begin with Why hydrogen is hard to sense.