Pith

open record

sign in

arxiv: 2508.06892 · v1 · pith:AYXSAC72 · submitted 2025-08-09 · astro-ph.SR · physics.space-ph

Large Model Driven Solar Activity AI Forecaster: A Scalable Dual Data-Model Framework

Reviewed by Pith T0 review T1 audit T2 compute T3 formal T4 kernel pith:AYXSAC72record.jsonopen to challenge →

classification astro-ph.SR physics.space-ph
keywords solarforecastingactivityhumanparadigmspaceweatheraccuracy
0
0 comments X
read the original abstract

Solar activity drives space weather, affecting Earth's magnetosphere and technological infrastructure, which makes accurate solar flare forecasting critical. Current space weather models under-utilize multi-modal solar data, lack iterative enhancement via expert knowledge, and rely heavily on human forecasters under the Observation-Orientation-Decision-Action (OODA) paradigm. Here we present the "Solar Activity AI Forecaster", a scalable dual data-model driven framework built on foundational models, integrating expert knowledge to autonomously replicate human forecasting tasks with quantifiable outputs. It is implemented in the OODA paradigm and comprises three modules: a Situational Perception Module that generates daily solar situation awareness maps by integrating multi-modal observations; In-Depth Analysis Tools that characterize key solar features (active regions, coronal holes, filaments); and a Flare Prediction Module that forecasts strong flares for the full solar disk and active regions. Executed within a few minutes, the model outperforms or matches human forecasters in generalization across multi-source data, forecast accuracy, and operational efficiency. This work establishes a new paradigm for AI-based space weather forecasting, demonstrating AI's potential to enhance forecast accuracy and efficiency, and paving the way for autonomous operational forecasting systems.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.