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arXiv · 2608.13812

H-$\alpha$ Integral Carrington Synoptic Maps Produced by NSO/NISP

K. J. Shuman·L. Bertello·O. Burtseva·A. A. Pevtsov
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Abstract

Monitoring long-term chromospheric activity and large-scale solar structures like filaments and plages is critical for understanding solar magnetic cycles and predicting space-weather events. While photospheric magnetic fields are routinely mapped, a consistent, global reference for chromospheric structures has been absent from H-$\alpha$ observations. This technical report provides a comprehensive description of the methodology used to construct the NSF Global Oscillations Network Group (GONG) H-$\alpha$ Integral Carrington Synoptic Maps from full-disk observations. We outline the processing pipeline developed to transform these observations into 720 x 360 pixel maps binned by Carrington longitude and sine(latitude) and describe characteristics of the final data product.

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K. J. Shuman, L. Bertello, O. Burtseva, A. A. Pevtsov. 2026-08-13. H-$\alpha$ Integral Carrington Synoptic Maps Produced by NSO/NISP. https://arxiv.org/abs/2608.13812

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