SolARED: Solar Active Region Emergence Dataset for Machine Learning Aided Predictions

IF 2.4 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Spiridon Kasapis, Eren Dogan, Irina N. Kitiashvili, Alexander G. Kosovichev, John T. Stefan, Jake D. Butler, Jonas Tirona, Sarang Patil, Mengjia Xu
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Abstract

The development of accurate forecasts of solar eruptive activity has become increasingly important for preventing potential impacts on space technologies and exploration. Therefore, it is crucial to detect Active Regions (ARs) before they start forming on the solar surface. This will enable the development of early-warning capabilities for upcoming space weather disturbances. For this reason, we prepared the Solar Active Region Emergence Dataset (SolARED). The dataset is derived from full-disk maps of the Doppler velocity, magnetic field, and continuum intensity, obtained by the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO). SolARED includes time series of remapped, tracked, and binned data that characterize the evolution of acoustic power of solar oscillations, unsigned magnetic flux, and continuum intensity for 50 large ARs before, during, and after their emergence on the solar surface, as well as surrounding areas observed on the solar disc between 2010 and 2023. The resulting ML-ready SolARED dataset is designed to support enhancements of predictive capabilities, enabling the development of operational forecasts for the emergence of active regions. The SolARED dataset is available at https://sun.njit.edu/sarportal/, through an interactive visualization web application.

Abstract Image

SolARED:用于机器学习辅助预测的太阳活动区涌现数据集
对太阳喷发活动进行准确预报对于防止对空间技术和探索的潜在影响已变得越来越重要。因此,在太阳表面活动区域(ARs)开始形成之前进行探测是至关重要的。这将有助于发展对即将到来的空间天气干扰的预警能力。为此,我们编制了太阳活动区涌现数据集(SolARED)。该数据集来源于太阳动力学观测台(SDO)上的日震和磁成像仪(HMI)获得的多普勒速度、磁场和连续强度的全盘图。SolARED包括重新映射、跟踪和分组数据的时间序列,这些数据表征了2010年至2023年间50个大型ARs在太阳表面出现之前、期间和之后的太阳振荡声功率、无符号磁通量和连续强度的演变,以及在太阳盘上观测到的周围区域。由此产生的ML-ready SolARED数据集旨在支持增强的预测能力,从而能够对活跃区域的出现进行业务预测。SolARED数据集可通过交互式可视化web应用程序在https://sun.njit.edu/sarportal/上获得。
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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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