Solar Correlation
solar_correlationAnalyze how solar flux (SFI) affects propagation on a chosen HF band by grouping signal reports into SFI brackets with spot counts, average SNR, and reliability.
Instructions
How does solar flux (SFI) affect propagation on a specific band?
Groups signatures by SFI bracket and shows spot counts, average SNR, and reliability for each bracket. Higher SFI generally helps HF bands above 30m (F-layer ionization) but hurts bands below 30m (D-layer absorption).
Tool call template
Replace each placeholder with a value matching the input schema. Only required parameters are included; add optional parameters as needed.
{
"id": 1,
"jsonrpc": "2.0",
"method": "tools/call",
"params": {
"arguments": {
"band": "<band>"
},
"name": "solar_correlation"
}
}Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| band | Yes | ADIF band ID (102-111) | |
| source | No | Dataset source (default: "wspr") | wspr |
| rx_grid | No | Optional RX grid to filter (omit for global) | |
| tx_grid | No | Optional TX grid to filter (omit for global) |
Output Schema
| Name | Required | Description | Default |
|---|---|---|---|
| result | Yes |