期刊
SOLAR PHYSICS
卷 294, 期 3, 页码 -出版社
SPRINGER
DOI: 10.1007/s11207-019-1412-z
关键词
Sunspots; Statistics; Solar cycle; Observations
资金
- Portuguese FCT - Foundation for Science and Technology [SFRH/BGCT/113686/2015, SFRH/BSAB/143060/2018]
- FCT - Foundation for Science and Technology [UID/Multi/00611/2013]
- FEDER - European Regional Development Fund through COMPETE 2020 - Operational Programme Competitiveness and Internationalisation [POCI-01-0145-FEDER-006922]
- POCH
- Fundação para a Ciência e a Tecnologia [SFRH/BSAB/143060/2018] Funding Source: FCT
Using neural networks as a prediction method, we attempt to demonstrate that forecasting of the Sun's sunspot time series can be extended to the spatio-temporal case. We employ this machine-learning method to forecast not only in time but also in space (in this case, latitude) on a spatio-temporal dataset representing the solar sunspot diagram extending to a total of 142 years. The analysis shows that this approach seems to be able to reconstruct the overall qualitative aspects of the spatial-temporal series, namely the overall shape and amplitude of the latitude and time pattern of sunspots. This is, as far as we are aware, the first time that neural networks have been used to forecast the Sun's sunspot butterfly diagram, and although the results are limited in the quantitative prediction aspects, it points to the way to use the full spatio-temporal series as opposed to just the time series for machine-learning approaches to forecasting. Additionally, we use the method to predict that the upcoming Cycle 25 maximum sunspot number will be around R25=57 +/- 17. This implies a very weak cycle and, in fact, the weakest cycle on record.
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