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.
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.