While analyzing the skip path of a a 5-watt QSO I made last week from the San Francisco to Argentina with Project TouCans, I stumbled across a set of NOAA resources that completely changed how I look at ionospheric conditions. From real-time aurora dashboards to animated MUF forecasts and electron flux data, these tools offer hams powerful insights into propagation—and some surprises along the way.
I made a grey line QSO from the campus of City College San Francisco to Argentina with our 5-watt Project TouCans rig last week. Last night, KO6BTY and I found ourselves deep in the rabbit hole of ionospheric conditions. What started as curiosity about the Kp index and whether aurora activity might have influenced the QSO's skip path, led us to discover some powerful NOAA resources. From aurora dashboards and global ionosphere forecasts to animated MUF predictions and GOES electron flux data, these tools give ham radio operators new ways to understand HF propagation, F2 layer behavior, and the science behind those long-distance QSOs.
You'll immediatley notice that the skip looks weird. It jumps out of the ocean a little less than half the distance to Argentina, and then dives back in. No, we're not experimenting with neutrino-driven ham radio. This version of the mapping code assumes that every QSO utilizes a single skip off the F2 layer. That's clearly not the case for this one.
The colored grid overlaid on the Earth indicates the critical frequqency—the maximum frequency radio wave that will be reflected directly back to the Earth instead of escaping into space—of the F2 layer at each location. There's a legend in the lower right hand corner of the map. If you'd like to see the numeric values plotted, that's shown below.
You can see in both images that there's a very steep change in the values as the path approaches Argentina. That change is what had KO6BTY and I wondering if the aurora was active that evening.
We don't have anything interesting to report yet, but in the course of our search, we cam upon the following sites:
Aurorasauras
I've written about this site before. It's the best historic, graphical aurora data I've found. The time zone is a little bit annoying in that I'm not sure what time zone it's set for. At present, I just change the time until the grey line is in about the correct place vs my map. Still though, the data is very easy to read, and they have data that goes back more than a few days. Also, the maps feature links to pictures from people photographed the aurora at that time, so that's kinda cool!
My QSO took place at 7:56 PST, 2:56 UTC at about grey line... whatevs :)
NOAA Aurora Dashboard
This site has great animations as well as predictions of wht the aurora will do on the current day. It also displays recent Kp data. It doesn't go back very far though.
Aurora Animations for the North and South Pole
This is the site that led us to look for more data which is how I stumbled upon the very cool
Whole Atmosphere Model-Ionosphere Plasmasphere Electrodynamics Forecast Sytem
It has forecasts for the maximum usable RF frequency, (MUF), for the next two days! The forecast data is also animated.
Forecast dashboard with animations for MUF
Electron Flux
We're not using the data from this one yet, but it shows the electron flux arriving at the Earth at the geostationary orbit of the GOES satellites.
Copasetic Flow GloTEC Maps
I almost forgot to mention that this site has an up-to-date map of the F2 layer including hmF2 and foF2. The map uses a Cesium viewer so you can zoom in, out and explore the data.
One more NOAA Resource
The last seven days of Kp index readings can be found here
Wrapping it all up for now...
My unexpected QSO from the U.S. to Argentina with just 5 watts reminded us how dynamic and unpredictable HF propagation can be. We saw F2 layer changes on our generated plots that use NOAA GloTEC data. We wanted to know more. That led us to the NOAA’s ionosphere forecasts, aurora dashboards, and MUF predictions, which gave us fresh insight into what might have shaped that path. While we’re still piecing together the story—aurora activity, electron flux, and F2 layer variability all in play—it’s clear that these NOAA tools are invaluable for hams chasing DX, experimenting with QRP, or just learning more about how the ionosphere really works.
72s and good luck with the F2 layer!
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