Roentgen - Aditya-L1 solar flare nowcasters (Team Navya, ISRO BAH 2026 PS-15)

Dual independent temporal convolutional networks (TCNs) that nowcast solar flares from India's Aditya-L1 X-ray telemetry:

File Channel Input Heads
nowcast_soft.pt SoLEXS soft X-ray (2-22 keV) 6 causal features from the 1-min count rate detect (binary) + class (quiet/A/B/C/M/X)
nowcast_hard.pt HEL1OS hard X-ray (8-150 keV) 6 causal features detect + burst tier (quiet/H1/H2/H3)
nowcast_hard_calibrator.joblib - isotonic calibrator for the hard detect prob -
navya-v2/*.pt next-generation retrain 16 (soft) / 25 (hard) band-resolved physics features detect + 6-class
  • Strictly causal (trailing windows only), seq_len 120 min, 150k params each, CPU real-time (40 ms per inference).
  • The two channels share nothing upstream; fusion happens at the serving layer only (union alert).
  • Validated against the independent GOES catalogue (never a model input).

Serving code, feature pipeline, dashboard and docs: https://github.com/Aur1ety/Roentgen (branch minimal for the deployable snapshot). MODELS.md in this repo carries the full provenance/receipts summary.

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