Solar Weather
Solar flares, CMEs, geomagnetic storms, and the solar cycle — with direct ham radio impact for every event.
Solar Flare Classification: A, B, C, M, X — What Each Class Means for Radio
Solar flares are ranked A through X on a logarithmic scale based on GOES X-ray flux. Learn what each class means for HF blackouts, D-layer absorption, and radio operations.
advancedSudden Ionospheric Disturbances (SIDs): Real-Time Flare Detection via Radio
A Sudden Ionospheric Disturbance is a flare fingerprint readable by any VLF receiver. Learn how SIDs work, how to detect them, and what they mean for HF propagation.
beginnerSpace Weather 101: A Ham Radio Operator's Guide to the Sun-Earth Connection
Space weather — solar flux, K-index, X-ray class, and solar wind — directly controls HF propagation. Learn the Sun-Earth pipeline every HF operator needs to understand.
beginnerNOAA Space Weather Scales: R, S, G Explained for Ham Radio
NOAA's R, S, and G space weather scales quantify radio blackouts, radiation storms, and geomagnetic storms. Learn what each level means for HF propagation.
intermediateSolar Wind: The Invisible Force That Shapes HF Radio Propagation
How solar wind speed, density, and Bz affect HF propagation and geomagnetic activity. Live Bz and solar wind data on DXRadar.
advancedSolar Proton Events and Polar Cap Absorption: When High-Latitude HF Dies
How solar proton events cause polar cap absorption on HF radio, the NOAA S-scale, which paths are affected, and how long the blackout lasts.
intermediateSolar Flare Effects on Ham Radio: Blackouts, D-Layer Absorption, and Recovery
How solar flares cause HF shortwave blackouts via D-layer absorption, which bands are hit hardest, and how to monitor X-ray flux on DXRadar.
beginnerSolar Cycle 25 Peak: What It Means for HF Band Conditions
Solar Cycle 25 has exceeded all NOAA/NASA predictions, driving exceptional HF conditions. Live SSN and SFI data, band-by-band effects, and what comes next.
intermediateA History of Solar Cycles: From Cycle 1 to Cycle 25 and What Comes Next
Solar cycle history from 1755 to today — key cycles for ham radio, the Maunder Minimum, and what Cycle 25's unexpected strength tells us about Cycle 26.
intermediateReading SDO and SOHO Solar Images: What Each Wavelength Shows
A guide to NASA's SDO AIA wavelengths and SOHO LASCO coronagraph imagery for ham radio operators monitoring solar activity and CMEs.
advancedHemispheric Power and Kp: Two Ways to Measure Geomagnetic Activity
Kp index and Hemispheric Power measure geomagnetic storms differently. Learn the physics behind both, their correlation, and which to use for HF operating decisions.
advancedDSCOVR and ACE at L1: How Spacecraft 1.5 Million km Away Predict Your Band Conditions
How DSCOVR and ACE at the L1 Lagrange point provide 15-60 minute advance warning of solar wind conditions that determine HF band quality.
intermediateCoronal Mass Ejections: How CMEs Cause Geomagnetic Storms and HF Blackouts
How Earth-directed CMEs trigger G-scale geomagnetic storms and HF disruption 1-3 days after ejection. Live storm data on DXRadar.
beginnerThe Carrington Event: What Would a Mega-Storm Mean for Amateur Radio Today?
The 1859 Carrington Event remains the most powerful solar storm on record. Here's what a repeat would do to HF radio, the power grid, and amateur radio's emergency role.
advancedBz and the IMF: The Space Weather Number That Predicts HF Disruption
What Bz and the interplanetary magnetic field mean for HF radio, how southward Bz drives geomagnetic storms, and live Bz data on DXRadar.