ARCAFF: Cutout classification dataset

Solar active regions (ARs) are dynamic and magnetically complex areas on the Sun's surface, often associated with phenomena such as solar flares and coronal mass ejections. Accurate identification and classification of these regions are essential for understanding solar magnetic activity and forecasting space weather events. Traditional AR classification methods have predominantly relied on manual observation and analysis, which, while effective, are time-consuming and subject to human bias. Existing datasets for AR classification have significant limitations that hinder their effectiveness for deep-learning applications. We present (Active Region Classification and Flare Forecasting: Cutout Classification Dataset), a new large-scale dataset of solar AR magnetograms and continuum cutouts specifically designed for machine-learning applications. ARCAFF:CCD The dataset combines co-temporal line-of-sight magnetograms and continuum intensity images from the SOHO/MDI and SDO/HMI instruments. Each cutout is linked to AR identifiers assigned by the National Oceanic and Atmospheric Administration (NOAA) and includes both Mount Wilson and McIntosh classifications. The pipeline performs calibration, alignment, and structured labelling of full-disc magnetograms using AR classification metadata from NOAA Solar Region Summary (SRS) reports. The dataset covers nearly three decades of observations spanning multiple solar cycles, comprising 33,045 AR cutouts and 72,297 quiet Sun cutouts. Each cutout is accompanied by comprehensive metadata and, to our knowledge, represents the most extensive and detailed publicly available resource of its kind. The dataset provides a comprehensive resource for developing and testing machine-learning models for solar AR classification and space weather forecasting. ARCAFF:CCD