solar_correlation
Analyzes how solar flux (SFI) impacts HF propagation on a given band by grouping spot data into SFI brackets and displaying spot counts, average SNR, and reliability per bracket.
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).
Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| band | Yes | ADIF band ID (102-111) | |
| tx_grid | No | Optional TX grid to filter (omit for global) | |
| rx_grid | No | Optional RX grid to filter (omit for global) | |
| source | No | Dataset source (default: "wspr") | wspr |
Output Schema
| Name | Required | Description | Default |
|---|---|---|---|
| result | Yes |