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Free Real-Time Radiation Monitor & Solar Weather Dashboard_

Live NOAA SWPC Telemetry · Geomagnetic Storm Tracking · Ionizing Radiation Reporting

Kp Index
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Solar Wind
km/s
Solar Flux
SFU (F10.7)
Mag Field Bz
nT (southward = storm)
Solar Wind Particle Stream
DSCOVR / ACE Upstream Monitor — km/s
Sensor Network — World Map
12 Monitoring Stations Equirectangular projection
Global Sensor Network (μSv/h)
Kp Index — Last 24 Hours
Planetary Geomagnetic Activity QUIET
-24h Kp 0-3: Quiet   4: Active   5+: Storm Now
Space Weather Status
IONOSPHERE SPECTRAL DENSITY — DRIVEN BY LIVE Kp
Solar & Cosmic Telemetry
Deep Space Observation
ParameterValueDelta
Magnetometer Bz — 6 Hour Timeline
Interplanetary Magnetic Field — nT
-6h Bz negative (southward) → geomagnetic coupling Now
Anomaly Log
[--:--:--] Awaiting NOAA SWPC uplink...
Geomagnetic Load
MAGNETOSPHERE LOADING (Kp/9)
Kp 0 — Quiet Kp 5 — Storm Kp 9 — Extreme

Free Radiation Monitoring Dashboard — How It Works

This free radiation monitor provides real-time reporting on global ionizing radiation levels, solar weather conditions, and geomagnetic activity. All data is sourced directly from NOAA's Space Weather Prediction Center (SWPC), the world's authoritative source for space weather forecasting and solar event reporting. The dashboard updates automatically every two minutes, giving you continuous access to live space weather telemetry without any registration, API keys, or fees.

The Kp Index chart displays the last 24 hours of planetary geomagnetic activity, measured on a 0 to 9 scale. This index is essential for understanding when geomagnetic storms may affect GPS accuracy, radio communications, power grid stability, and aurora visibility. A Kp value of 5 or above indicates a geomagnetic storm. The color-coded bar chart makes it easy to spot storm periods at a glance, and the status badge provides an instant summary of current geomagnetic conditions — from quiet to extreme storm levels.

Solar Wind & Magnetometer Reporting

The solar wind particle stream visualization shows real-time data from the DSCOVR and ACE spacecraft positioned at the L1 Lagrange point, approximately 1.5 million kilometres upstream of Earth. Particle speed and density are mapped directly to the animation — faster solar wind creates faster-moving particles, and higher proton density increases particle brightness. When solar wind speeds exceed 500 km/s, the display shifts from cyan to yellow, and above 700 km/s it turns red, providing an immediate visual warning of elevated conditions.

The magnetometer Bz timeline tracks the north-south component of the interplanetary magnetic field over the past six hours. When Bz turns negative (southward), it enables magnetic reconnection with Earth's magnetosphere, allowing solar wind energy to couple more efficiently into our magnetic field. Extended periods of strongly negative Bz are the primary driver of geomagnetic storms, making this one of the most important parameters for space weather forecasting.

Worldwide Radiation Sensor Network

The global sensor network displays estimated ground-level radiation readings for 12 cities worldwide, including Tokyo, Berlin, New York, London, Sydney, Brussels, Reykjavik, Singapore, Moscow, and Cape Town. Two historically significant sites — Pripyat (near Chernobyl) and Fukushima — are included with elevated baseline values reflecting legacy contamination. Each sensor card includes a sparkline showing recent variation, and the interactive world map lets you visualise all station locations with hover-to-inspect functionality.

Ground-level radiation estimates are calculated using a physics-based model that combines known geological baselines per city with real-time cosmic ray modulation data. Higher geomagnetic latitude increases cosmic ray exposure due to weaker magnetic shielding, and elevated Kp index values modulate the cosmic ray intensity reaching Earth's surface. While these are modeled estimates rather than direct sensor readings, they use the same real NOAA data that drives professional space weather reporting systems.

Free Tool — No Signup Required

This radiation monitoring dashboard is completely free to use with no account creation, no ads, and no data collection. It runs entirely in your browser using client-side JavaScript and public NOAA APIs. Whether you are a space weather enthusiast, a radio amateur monitoring HF propagation conditions, a researcher tracking geomagnetic storm impacts, or simply curious about the radiation environment around you, this tool provides professional-grade reporting in an accessible, visually engaging format. It is one of over 50 free browser-based tools available at jasperbernaers.com — all built with the same commitment to real data, zero friction, and beautiful design.

FAQ — Global Radiation Flux: Ionizing Radiation & Solar Telemetry

Frequently Asked Questions — Radiation Monitoring Dashboard

What is μSv/h and what are safe levels?

Microsieverts per hour (μSv/h) measures the rate of ionizing radiation dose absorbed by the human body. Typical natural background radiation is 0.08 to 0.15 μSv/h, varying by altitude, geology, and proximity to radon sources. Anything above 0.50 μSv/h in a residential area triggers a monitoring network alert. For context, a chest X-ray delivers roughly 20 μSv in a single exposure.

How is Solar Flux (SFU) calculated?

The solar flux unit (sfu) measures the intensity of solar radio emissions at a frequency of 2800 MHz (10.7 cm wavelength). It is recorded daily by observatories worldwide and serves as a primary indicator of solar activity. Values typically range from 60 sfu during solar minimum to over 300 sfu during solar maximum. Higher solar flux correlates with increased UV radiation, geomagnetic storms, and HF radio propagation changes.

What causes elevated radiation readings?

Elevated readings can result from natural sources (radon gas from granite bedrock, cosmic rays at high altitude, thorium-rich soil) or artificial sources (proximity to nuclear facilities, medical isotope production, legacy contamination). Solar particle events (SPEs) during coronal mass ejections can temporarily raise cosmic radiation levels, especially at high latitudes and flight altitudes above 10,000 metres.

What is the Kp Index and why does it matter?

The Kp Index is a global geomagnetic activity index on a 0-9 scale. Values of Kp 5 or above indicate a geomagnetic storm, which can disrupt GPS satellites, HF radio communications, and power grids. Kp 7+ events are classified as severe storms. The Kp Index is derived from magnetometer data at 13 observatories between 44° and 60° geomagnetic latitude.

What monitoring networks provide this data?

Global radiation monitoring relies on networks such as the IAEA International Monitoring System (IMS), Europe's EURDEP (European Radiological Data Exchange Platform) with 5,500+ stations across 39 countries, the US RadNet system, and national networks like FANC (Belgium) and BfS (Germany). Solar data comes from NOAA SWPC, the Penticton Solar Observatory, and ESA's space weather programme.

How does altitude affect radiation exposure?

Cosmic radiation doubles approximately every 2,000 metres of altitude gain. At sea level, cosmic radiation contributes about 0.03 μSv/h. At commercial flight altitude (10-12 km), it reaches 3-8 μSv/h depending on latitude and solar activity. Airline crews are classified as radiation workers in the EU and receive annual dose monitoring.

What is the difference between alpha, beta, and gamma radiation?

Alpha particles (helium nuclei) are stopped by paper or skin but dangerous if inhaled. Beta particles (electrons) penetrate skin but are stopped by aluminium. Gamma rays (photons) penetrate most materials and require lead or concrete shielding. Most environmental monitors measure gamma radiation as it is the dominant external exposure pathway. Neutron radiation from cosmic rays is also significant at altitude.

What is a normal annual radiation dose?

The global average annual dose from all sources is approximately 2.4 mSv (millisieverts). This breaks down to roughly 1.2 mSv from radon inhalation, 0.5 mSv from external terrestrial radiation, 0.3 mSv from cosmic rays, and 0.3 mSv from food and water. Medical exposures (CT scans, X-rays) add an average of 0.6 mSv in developed countries. The recommended occupational limit is 20 mSv/year.

Is the data on this dashboard real-time?

Yes! Solar and cosmic telemetry data (solar flux, solar wind speed, Kp index, Bz magnetic field, proton density, storm scales, and alerts) are live data from NOAA's Space Weather Prediction Center (services.swpc.noaa.gov). The Kp bar chart shows real 3-hourly observations from the last 24 hours. Solar wind particles are animated at speeds matching real upstream measurements. Ground-level radiation estimates at specific cities are modeled from real cosmic ray data — actual ground sensor networks (EURDEP, RadNet) don't provide free CORS-enabled APIs for direct browser access. The baseline values per city use known geological and altitude factors.

Is this dashboard free to use?

Yes, completely free with no signup, no ads, and no data collection. Everything runs 100% in your browser. It is one of 50 free tools at jasperbernaers.com.