Adds the second ionospheric data source layer. Polls NOAA SWPC's free
public JSON services every 5 minutes for three products:
* Planetary K-index (1-min cadence) → geomagnetic_observations
* 10.7 cm solar flux (hourly) → solar_flux_observations
* GOES X-ray flux (1-min, 0.1-0.8nm long-wave band only) →
solar_xray_observations
All three products feed HF / Es scoring inputs that the propagation
engine will start using in a follow-up commit:
* Kp drives HF absorption and Es damping (memory notes Kp is inversely
correlated with tropo/Es stability).
* F10.7 is the SSN proxy for ITU-R P.533 HF MUF prediction.
* GOES X-ray long-wave flux is the short-wave fade (SWF) / D-layer
absorption proxy — a C-class flare starts attenuating HF within
seconds of the X-ray peak.
New context `Microwaveprop.SpaceWeather` exposes `upsert_*/1` and
`latest_*/0` per product; `SpaceWeatherFetchWorker` pulls all three
independently so one endpoint's outage doesn't block the others.
Fixtures captured from live SWPC endpoints on 2026-04-15 for the
parser tests.
Not yet wired into scoring — that's a separate commit.
First step toward physics-based HF / sporadic-E scoring. Polls GIRO's
DIDBase tabular endpoint every 10 minutes for two US ionosondes
(Millstone Hill MHJ45, Alpena AL945), parses the plain-text response
into observation rows, and upserts into a new ionosonde_observations
table keyed on (station_code, valid_time).
This gets foEs (E-layer sporadic critical frequency) into the database
as a direct measurement — the key input for predicting 144 MHz Es
openings via ITU-R P.534-6. foF2 + MUFD are the F2-layer inputs for
HF MUF predictions.
Not yet wired into scoring. Boulder/Wallops/Austin/Idaho/Point Arguello
are in the GIRO catalog but were silent when probed — add them back
if/when they come online.
Next steps: SWPC JSON (Kp, F10.7, sunspot), GOES X-ray flux, D-RAP text,
and the P.534-6 Es scoring factor that uses foEs at midpoint for the
144/440 band configs.
