What data sources does this server use?

The server indexes 175 million WSPR (Weak Signal Propagation Reporter) and RBN (Reverse Beacon Network) signatures to analyze HF band openings and propagation patterns. It correlates this with solar activity data to predict ionospheric conditions.

Who should use this MCP server?

Radio operators, propagation forecasters, and HF enthusiasts who need real-time band opening analysis and historical propagation trends. It's designed for both casual operators and research-level propagation studies.

How do I install and run it?

Install via `uvx ionis-mcp@1.2.7`. The server runs over stdio transport, so connect it to your MCP client and query propagation data directly from your chat interface.

Can I forecast band openings with this?

Yes—the server analyzes historical WSPR/RBN signatures and solar correlation patterns to provide band opening predictions. Accuracy depends on current solar conditions and historical data density for your target bands and paths.

What's the difference between WSPR and RBN data?

WSPR captures weak-signal propagation reports from operators worldwide; RBN aggregates automated beacon reception reports. Together they provide complementary views of propagation—WSPR shows actual QSOs, RBN shows beacon detectability.

MCP ServerSTDIOOfficialv1.2.7

Qso Graph Ionis MCP Server

Analyze HF radio propagation patterns using 175M WSPR/RBN signatures and solar data. Built for radio operators and propagation researchers who need band opening forecasts and ionospheric correlation insights.

io.github.qso-graph/ionis-mcp

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Hosted URL

Local install

Transport

STDIO

Auth

No auth required

What the Qso Graph Ionis MCP server does

How models use it and what it is built for.

Connect to Qso Graph Ionis

Local install — runs as a subprocess.

uvx ionis-mcp==1.2.7

Resources

Where to find authoritative docs and source for Qso Graph Ionis.

Source repository

Example prompts for Qso Graph Ionis

Paste any of these into Agent Studio after connecting Qso Graph Ionis.

Show band openings for 20m and 40m in the next 6 hours
Correlate solar activity with 10m band propagation over the past week
Query WSPR signatures for transatlantic paths on 80m
What does the RBN data reveal about current skip distance trends?

Qso Graph Ionis MCP server — FAQ

Common questions about connecting and running Qso Graph Ionis.

What data sources does this server use?
The server indexes 175 million WSPR (Weak Signal Propagation Reporter) and RBN (Reverse Beacon Network) signatures to analyze HF band openings and propagation patterns. It correlates this with solar activity data to predict ionospheric conditions.
Who should use this MCP server?
Radio operators, propagation forecasters, and HF enthusiasts who need real-time band opening analysis and historical propagation trends. It's designed for both casual operators and research-level propagation studies.
How do I install and run it?
Install via `uvx ionis-mcp@1.2.7`. The server runs over stdio transport, so connect it to your MCP client and query propagation data directly from your chat interface.
Can I forecast band openings with this?
Yes—the server analyzes historical WSPR/RBN signatures and solar correlation patterns to provide band opening predictions. Accuracy depends on current solar conditions and historical data density for your target bands and paths.
What's the difference between WSPR and RBN data?
WSPR captures weak-signal propagation reports from operators worldwide; RBN aggregates automated beacon reception reports. Together they provide complementary views of propagation—WSPR shows actual QSOs, RBN shows beacon detectability.

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