gLOWCOST Georgia State University

Global cosmic-ray muon detector network

A detector in every country on Earth.

That is where this network is going. Twenty-one stations in eleven countries report today, and we are still expanding — one detector everywhere, and dense clusters in the regions where sensitivity to space and terrestrial weather runs highest.

Detectors cheap enough for a classroom, precise enough that when a solar storm passes Earth every station sees the count fall together.

Natural Earth · detector sites, Aug 2026 Hover a marker
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THE PROBLEM

Space weather hits a hyper-connected world, and we mostly watch it from orbit.

Coronal mass ejections and solar energetic particle events disturb power grids, satellite communications and GPS. The instruments we rely on to see them coming are largely satellites — the very assets a severe storm degrades. Ground-based cosmic-ray monitoring is the resilient second layer, but conventional observatories are expensive and few, so most of the planet goes unwatched.

OUR ANSWER

Make the instrument cheap, and put it everywhere.

gLOWCOST — global LOW-COst cosmic-ray muon detector network for monitoring dynamic changes in Space and Terrestrial weather — takes detection technology from fundamental nuclear physics and rebuilds it as a few-hundred-dollar instrument: plastic scintillator, silicon photomultipliers, and an edge-computing node that returns data in near real time. Founded in 2023 at the COSMIC centre at Georgia State University.

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SCIENTIFIC MOTIVATION

Every muon count is a message from two places at once.

Cosmic rays arriving at Earth are modulated by the Sun's activity on the way in, then shatter high in the atmosphere, where the temperature and density of the air decide how many muons reach the ground. So a single continuous count responds both to what the Sun is doing and to what the stratosphere is doing — provided you have enough stations, at enough latitudes, to tell the two apart.

That is why coverage is the science. Station metadata carries the geomagnetic cutoff rigidity, because latitude on a map is not the quantity that governs what gets through.

Scintillator & SiPM detection Edge computing & IoT GEANT4 shower simulation Citizen-science infrastructure
A gLOWCOST cosmic muon detector: an aluminium frame with scintillator layers and a readout board.
The baseline detector — scintillator, SiPM readout, single-board computer

Research thrusts

Four thrusts, one instrument.

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The plan

From a proven detector to a planetary instrument.

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Find your way in

Support the network

One gift puts a permanent station in a country that has never had one.

By partnering internationally and working through citizen science, we make this technology accessible worldwide — empowering communities, expanding coverage, and advancing our understanding of the cosmos. Contributions go into hardware, students, and keeping the data open.

Contact us directly

Georgia State University · global cosmic-ray muon detector network

Cosmic rays are
passing through you
right now.

A school can count them. When the Sun throws a storm at Earth, or the stratosphere warms overhead, the count changes — and twenty-one detectors across eleven countries record it together.

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Where the detectors are.

Hover a marker · click to open its plot

WHAT gLOWCOST IS

Research instruments at classroom prices.

Space-weather monitoring has meant expensive instruments in a few fixed places. Our detectors are cheap enough for a school and networked so that a class in Atlanta and a class in Lund record the same cosmic event — science and student training in the same instrument.

Several gLOWCOST detectors on a bench during a validation test, wired to single-board computers.

The network

A worldwide network, watching the same sky together.

Low-cost, portable muon detectors on five continents, reporting continuously for near real-time monitoring of space weather and the upper atmosphere. Select any station below to open its daily plot.

Every station, by region.

Green: GSU hub, Atlanta · red: partner stations

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Daily network summary

The whole network, in two figures a day.

Regenerated every day from every reporting station. Use the station table above for one site in detail; these show the network as a whole.

Thirty days against space-weather indices Muon flux · Kp · Dst · GOES X-ray
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Each station's flux stacked over the same thirty-day window, with the geomagnetic and solar indices beneath — the quickest way to see whether a dip is planetary or local. Sample figure shown — today's file was not reachable from this preview.
All stations, uncorrected Raw daily traces · one panel per site
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Uncorrected counts as recorded, before pressure and temperature corrections — a daily health check on the array, and the fastest way to spot a station that has gone quiet. Sample figure shown — today's file was not reachable from this preview.

Open data

Freely available on request.

Detector data are available to everyone following a confirmed access request. Summary plots show hourly muon-flux percent change alongside ground-level pressure; per-site metadata includes the geomagnetic cutoff rigidity.

The download tool is in beta — select a station and a date range, and it returns the underlying series. If it is unavailable, email us and we will send the files directly.

Contacts

Summary-plot queries
Enosh Herath Mudiyanselage — eherathmudiyanselag1@gsu.edu
Data requests & urgent needs
Xiaochun He — xhe@gsu.edu

Take part

You do not need a detector to take part.

Every measurement this network makes is public the moment it is recorded. A class with nothing but a browser can run the same analysis as a class with an instrument on the roof — and appears on the same results poster at the end.

Students staffing the gLOWCOST table with a live detector and poster at a public STEM expo.

Four ways in.

Tier What your class does What you need Cost
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Coordinated observing

Everyone measures the same event, on the same days.

Oct 2026 – Apr 2027 · open now

SSW Watch

Each winter the stratosphere over the pole can warm by tens of degrees in days, buckling the polar vortex. Because muons are made high in the atmosphere, that upheaval should register in our counts — strongest at our northernmost station, weakest in Atlanta. Students predict the size of the effect before they look. A clear "we could not detect this, and here is why" is a full result.

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Standing · whenever the Sun decides

Forbush Watch

When a coronal mass ejection sweeps past Earth it carries some cosmic rays away with it, and every station sees the count drop together within hours. There is no schedule for this. We alert participating classes when one is on the way, and students watch a storm that left the Sun days earlier arrive in their own data.

An east–west oriented gLOWCOST detector arrangement used to study directional muon flux.
East–west asymmetry run

For teachers

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For partner institutions

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Sep
19
2026

Come and see one

Find us at the PDK Good Neighbor Day Airshow.

DeKalb-Peachtree Airport, Atlanta. Gates at 1:00 pm through the night show at 9:00 pm. A detector counting live at the STEM Expo, students from Frederick Douglass explaining what it does, and the altitude profile we recorded at cruising height on the way to a conference. Free entry.

News & publications

What's happening on the network.

A few of the stories behind the network, newest first. Please spread the word and help us build this grassroots effort — we encourage teachers and students everywhere to take part in this worldwide STEM outreach.

Updates

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Publications

Collaboration & team

The people behind gLOWCOST.

Led from the Department of Physics & Astronomy at Georgia State University and run as an open collaboration with partner institutions and schools across eleven countries.

Project leads

Partner institutions & schools

Select an institution for its location, key participants and what they work on.

Interested in joining or supporting gLOWCOST?

To join the collaboration, host a detector, or make a donation, contact Xiaochun He or any team member above.

Get in touch

SUPPORT gLOWCOST

Help us put a detector in every country.

Funding a global instrument built out of inexpensive parts is harder than it sounds: no single agency owns the problem it addresses. By partnering internationally and working through citizen science, we make this technology accessible worldwide — empowering communities, expanding coverage, and advancing our understanding of the cosmos.

Every contribution goes into hardware, students and open data. A single gift can put a permanent station in a country that has never had one.

Researchers and students with a gLOWCOST detector at Nara Women's University, Japan.
A new host site coming online — Nara Women's University, Japan

Where a contribution goes.

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Gift levels and the university's online giving link can be set here — send me the fund name and URL from GSU Advancement and I will wire the buttons to it.

What funding unlocks

Coverage is the science.

A muon detector on its own measures one place. A network measures the planet — and the value of each new station rises with every other station already reporting. Gaps in the map are gaps in the physics.

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Citizen science

Accessible technology, everywhere.

Low cost is not a compromise here — it is the mechanism. Instruments inexpensive enough for a school make a global network possible at all, and put the measurement in the hands of the communities that host it.

Supporters are named on the station they fund and on network publications using its data, and receive the annual results poster carrying the students' own analyses.

Eleven countries reporting. One hundred and eighty-four to go.

Individuals, foundations, companies and universities can all sponsor coverage. Tell us what you would like your contribution to do and we will show you exactly where it lands on the map.

Partner institution

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Institution site ↗
Daily detector plot

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Last 30 days · full time series Flux % change · scaled temperature · scaled pressure {{ plotFile }}