摘要
在UNet神经网络结构的基础上,引入多头自注意力(Multi-head Self Attention,MHSA)神经网络层,构建了一套太阳光球层磁场预测模型。通过在SDO/HMI观测数据上进行训练,此模型具备在一定精度上预测太阳磁场的能力。模型的测试结果还表明,MHSA的引入显著提升了模型的预测能力。
We present a prediction model of solar photosphere magnetic field in this paper.It is based on the UNet neural network,combining with the Multi-head self attention layer.After being trained on the SDO/HMI observation data,this model has the ability to predict the photosphere magnetic field at a certain accuracy.Furthermore,the results also shows that the MHSA layer makes significant improvement to the model’s performance.
作者
马骁鹏
Ma Xiaopeng(Zhengzhou University of Industrial Technology,College of Information and Engineering,Zhengzhou 451100,China)
出处
《科学技术创新》
2022年第18期74-77,共4页
Scientific and Technological Innovation
基金
河南省自然科学基金青年基金项目,基于深度神经网络的太阳风多参数联合预测研究,212300410294
河南省高等学校重点科研项目计划,基于深度卷积神经网络的太阳光球层磁场演化模型,20B170008。
关键词
UNet
注意力机制
太阳光球层
磁场预测
UNet
Attention mechanism
Solar photosphere
Magnetic field prediction