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Academy

Learn to observe. Then build the observatory.

Learning paths, from what an observation is to a commissioned site: instruments and siting, links and clocks, edge compute and field AI, Earth observation, site operations, the open protocol, and the standards that make data trusted. Every lesson runs on the same atlas, spectrum and methods as the rest of this site.

Choose a pathHow the academy works

Learning by building: a weather station assembles part by part in a training yard.

Foundations

Instruments

Connectivity

Edge and AI

Earth observation

Site operations

Protocol

Policy and standards

START

01 · Principles

Taught the way observatories are run.

Source before claim, method before tool, evidence before sign-off. The rules the long-lived observatories in the atlas kept are the rules every lesson keeps.

01From the record

Each path opens with the observatories that met its problem, and the lesson they left, cited from the atlas.

02Method, then tool

Every calculation ships with its formula and a worked example you check by hand before any software runs it.

03Real data

Exercises run on real elevation, real open networks and real standards, with their licences stated.

04Evidence, not badges

A module ends in an artefact someone else can check: a site plan, a link budget, a WIGOS record, a conformance run.

02 · Paths

From first principles to a commissioned site.

Start anywhere. Paths cross where the work does: a site plan needs power, timing and backhaul, and every path ends on the protocol.

FoundationConcepts and vocabulary, no prerequisites.

PractitionerPlan, configure and check real systems.

AdvancedDesign, integrate and operate at scale.

01 · Path

Foundations of observation.

Before the instrument, the idea: what an observation is, why it must be comparable, and how five thousand years of observatories learned to share units, hours and records.

For · Everyone: students, hosts, communities, new team members.

  1. What an observation isTell a measurement from an observation: value, unit, time, place, method and uncertainty. Foundation
  2. Five thousand years in six erasWalk the atlas from Stonehenge to Rubin and name what each era added. Foundation
  3. ComparabilityExplain why the Medici network and the Magnetic Union mattered: shared instruments, hours and units. Foundation
  4. Calibration and traceabilityFollow a reading back to a reference and say how far you can trust it. Practitioner
  5. Long recordsSee why an unbroken series from one site becomes an instrument in itself, and how records are lost. Practitioner
  6. From station to systemDescribe how separate stations become one observing system, and what holds a federation together. Practitioner
Open the atlas

03 · How it works

Open to read. An account keeps your work.

The academy sits on the open main site. Read any lesson without signing in; an account keeps your progress, plans and runs. Teams work a path together in the NXS Observatory app.

  • ReadEvery lesson is public, in English and French, with its sources.
  • TryInteractive explainers on real data: terrain, line of sight, link budgets, timing, satellite passes.
  • BuildExercises in the NXS Observatory app produce plans, manifests and conformance runs you keep.
  • ContributeLessons are versioned in the open. Propose a correction or a new module; contributors keep their rights.
  • TeachUniversities, colleges and training centres can use the material in their own courses; talk to us about teaching.

Stories

Learn from a place.

Each story walks through one place or one system with figures you can turn, cut and recompute. All stories

Horizon 2030: Overview What changes by 2030Six shifts will reshape how the Earth is observed before the decade ends: networks that sense, models that forecast, foundation models that read imagery,…System: End to end An observation grid, end to endAn observation is not a reading. It is a reading with a place, a time, a calibration and a path that anyone can follow back. An observing grid is the…Place: Dense city block The instrumented streetFour city blocks, read as an observing system: small cells on street poles, air-quality and heat sensors beside them, and an edge node that corrects, times…Place: Forest and wildfire Seeing smoke soonerA fire is cheapest to fight in its first hour. Ridge-top cameras, weather in the stand and satellite hot spots each see it at different times and scales;…Place: River basin and floods Rising water, counted in metresA flood map is a sentence about the future: this ground lies below that level. Gauges along the valley, a weather station and a terrain model turn the…Place: Orbit Orbits as infrastructureLow orbits are fast and crowded, high orbits slow and spacious. Every choice of altitude is a trade between delay, footprint and how long the satellite…

— · Begin

Every observatory starts with someone learning to look.

Start with the history, the spectrum or the protocol.

Start with the atlasExplore the spectrumRead the protocol
Academy

Learn to observe. Then build the observatory.

Learning paths, from what an observation is to a commissioned site: instruments and siting, links and clocks, edge compute and field AI, Earth observation, site operations, the open protocol, and the standards that make data trusted. Every lesson runs on the same atlas, spectrum and methods as the rest of this site.

01 · Principles

Taught the way observatories are run.

Source before claim, method before tool, evidence before sign-off. The rules the long-lived observatories in the atlas kept are the rules every lesson keeps.

01From the record

Each path opens with the observatories that met its problem, and the lesson they left, cited from the atlas.

02Method, then tool

Every calculation ships with its formula and a worked example you check by hand before any software runs it.

03Real data

Exercises run on real elevation, real open networks and real standards, with their licences stated.

04Evidence, not badges

A module ends in an artefact someone else can check: a site plan, a link budget, a WIGOS record, a conformance run.

02 · Paths

From first principles to a commissioned site.

Start anywhere. Paths cross where the work does: a site plan needs power, timing and backhaul, and every path ends on the protocol.

FoundationConcepts and vocabulary, no prerequisites.
PractitionerPlan, configure and check real systems.
AdvancedDesign, integrate and operate at scale.
03 · How it works

Open to read. An account keeps your work.

The academy sits on the open main site. Read any lesson without signing in; an account keeps your progress, plans and runs. Teams work a path together in the NXS Observatory app.

  • ReadEvery lesson is public, in English and French, with its sources.
  • TryInteractive explainers on real data: terrain, line of sight, link budgets, timing, satellite passes.
  • BuildExercises in the NXS Observatory app produce plans, manifests and conformance runs you keep.
  • ContributeLessons are versioned in the open. Propose a correction or a new module; contributors keep their rights.
  • TeachUniversities, colleges and training centres can use the material in their own courses; talk to us about teaching.
— · Begin

Every observatory starts with someone learning to look.

Start with the history, the spectrum or the protocol.