G estimate \(G_{\text{est}}=v_{\rm RMS}^2/(8\pi c^2)\), density-scaled mode, CST dial, DC/DE/DM, Auto-Scan 10× & CSV. Note: “Harmony Glow” now affects only the Open-Toroid canvas (color + brightness + orbiting arrows/dots). Page background never changes.
| # | Time (CST) | Body | Mode (min) | v-RMS (m/s) | Gest (m³·kg⁻¹·s⁻²) | Δ vs G₀ | Pass/Fail |
|---|
| Symbol | Meaning | Value |
|---|
Upload a geomagnetic CSV file with columns like UTC_time,CST_time,H,D,Z,F (1-minute or 1-second data). H,D,Z,F in nT or similar. |B| is computed as F or √(H²+D²+Z²) if F is missing.
UTC_time,CST_time,H,D,Z,F
2025-11-01T00:00:00Z,2025-10-31T18:00:00-06:00,12345.1,-44.2,48567.8,49876.3
2025-11-01T00:01:00Z,2025-10-31T18:01:00-06:00,12346.2,-44.0,48566.9,49877.0
2025-11-01T00:02:00Z,2025-10-31T18:02:00-06:00,12347.0,-43.9,48565.5,49878.1
2025-11-01T00:03:00Z,2025-10-31T18:03:00-06:00,12346.5,-44.1,48566.2,49877.5
2025-11-01T00:04:00Z,2025-10-31T18:04:00-06:00,12345.8,-44.3,48567.0,49876.9
The upload panel parses the file, plots |B|, and converts it into a neutral CST dataset. A derived v-RMS series is written into the “Pasted samples (m/s)” box; tick “Use pasted data” to let real data drive v-RMS.