Eme Mcp

eme-mcp

[PyPI] [MCP Registry]

MCP server for EME — Earth-Moon-Earth, moonbounce. When the moon is up from your grid, when it is up from both ends of a schedule at once, what the path costs on 2m, 70cm and 23cm, and which days ahead are least degraded.

Part of the qso-graph project. No network, no authentication.

Why it needs nothing from the network

The moon's position is computed here, from the abridged ELP-2000/82 series as Meeus tabulates it (Astronomical Algorithms, chapter 47). That is around 250 lines of standard library and a coefficient table. It is also what WSJT-X does, and the norm for EME software.

That matters for more than tidiness. Moonrise and moonset are different for every grid square, so a service-backed answer means a request per location per query — and a planning tool that stalls, rate-limits, or goes dark when a remote service does.

JPL Horizons is still here — as the test oracle. Recorded Horizons responses are fixtures, so every CI run checks these numbers against NASA's rather than against themselves. Measured against Horizons for a Boise grid:

Thirty arcseconds, against a 432 MHz array that is degrees wide.

Install

uvx eme-mcp            # run it; nothing to install

Tools

What this does not yet do

Sky noise is not included. The full degradation figure an EME operator plans with combines the distance term with the galactic background behind the moon, from the Haslam 408 MHz all-sky map. That map is not yet carried and pinned, so eme_degradation and eme_calendar report the distance term and say so in every answer rather than returning a number that looks complete and is not. Tracked in qso-graph-devel#52.

Elevations are geometric: no atmospheric refraction, which lifts an object near the horizon by about half a degree.

The two path-loss figures

They answer different questions and are often confused, so both are returned:

• echo_db is the one to budget a station with — the radar equation, accounting for the moon reflecting about 6.5% of what reaches it. Near 252 dB on 2m, 262 on 70cm and 271 on 23cm at mean distance, which are the numbers EME operators know.
• round_trip_db is twice the free-space loss. It ignores the moon entirely.

Licence

GPL-3.0-or-later. See LICENSE.

The algorithms are from Jean Meeus, Astronomical Algorithms (2nd edition, Willmann-Bell, 1998), chapters 7, 11, 12, 22, 40 and 47 — cited in the source where each is used. The implementation is ours; the mathematics is his and is not claimed.