Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Abduallah, Yasser"'
Autor:
Abduallah, Yasser, Wang, Jason T. L.
Solar flares are explosions on the Sun. They happen when energy stored in magnetic fields around solar active regions (ARs) is suddenly released. In this paper, we present a transformer-based framework, named SolarFlareNet, for predicting whether an
Externí odkaz:
http://arxiv.org/abs/2405.16080
Autor:
Xu, Chunhui, Wang, Jason T. L., Wang, Haimin, Jiang, Haodi, Li, Qin, Abduallah, Yasser, Xu, Yan
Image super-resolution has been an important subject in image processing and recognition. Here, we present an attention-aided convolutional neural network (CNN) for solar image super-resolution. Our method, named SolarCNN, aims to enhance the quality
Externí odkaz:
http://arxiv.org/abs/2403.18302
Autor:
Abduallah, Yasser, Alobaid, Khalid A., Wang, Jason T. L., Wang, Haimin, Jordanova, Vania K., Yurchyshyn, Vasyl, Cavus, Huseyin, Jing, Ju
We propose a novel deep learning framework, named SYMHnet, which employs a graph neural network and a bidirectional long short-term memory network to cooperatively learn patterns from solar wind and interplanetary magnetic field parameters for short-
Externí odkaz:
http://arxiv.org/abs/2402.17196
Autor:
Alobaid, Khalid A., Abduallah, Yasser, Wang, Jason T. L., Wang, Haimin, Fan, Shen, Li, Jialiang, Cavus, Huseyin, Yurchyshyn, Vasyl
Publikováno v:
The Astrophysical Journal Letters, 958:L34, 2023
Coronal mass ejections (CMEs) are massive solar eruptions, which have a significant impact on Earth. In this paper, we propose a new method, called DeepCME, to estimate two properties of CMEs, namely, CME mass and kinetic energy. Being able to estima
Externí odkaz:
http://arxiv.org/abs/2312.01691
Autor:
Farooki, Hameedullah, Abduallah, Yasser, Noh, Sung Jun, Kim, Hyomin, Bizos, George, Shin, Youra, Wang, Jason T. L., Wang, Haimin
Interplanetary magnetic flux ropes (MFRs) are commonly observed structures in the solar wind, categorized as magnetic clouds (MCs) and small-scale MFRs (SMFRs) depending on whether they are associated with coronal mass ejections. We apply machine lea
Externí odkaz:
http://arxiv.org/abs/2311.09345
Autor:
Farooki, Hameedullah, Noh, Sung Jun, Lee, Jeongwoo, Wang, Haimin, Kim, Hyomin, Abduallah, Yasser, Wang, Jason T. L., Chen, Yu, Servidio, Sergio, Pecora, Francesco
Small-scale interplanetary magnetic flux ropes (SMFRs) are similar to ICMEs in magnetic structure, but are smaller and do not exhibit ICME plasma signatures. We present a computationally efficient and GPU-powered version of the single-spacecraft auto
Externí odkaz:
http://arxiv.org/abs/2311.06759
Autor:
Jiang, Haodi, Li, Qin, Hu, Zhihang, Liu, Nian, Abduallah, Yasser, Jing, Ju, Zhang, Genwei, Xu, Yan, Hsu, Wynne, Wang, Jason T. L., Wang, Haimin
Publikováno v:
Solar Physics, 2023
Solar activity is usually caused by the evolution of solar magnetic fields. Magnetic field parameters derived from photospheric vector magnetograms of solar active regions have been used to analyze and forecast eruptive events such as solar flares an
Externí odkaz:
http://arxiv.org/abs/2211.02278
Autor:
Abduallah, Yasser, Wang, Jason T. L., Bose, Prianka, Zhang, Genwei, Gerges, Firas, Wang, Haimin
The disturbance storm time (Dst) index is an important and useful measurement in space weather research. It has been used to characterize the size and intensity of a geomagnetic storm. A negative Dst value means that the Earth's magnetic field is wea
Externí odkaz:
http://arxiv.org/abs/2205.02447
Solar energetic particles (SEPs) are an essential source of space radiation, which are hazards for humans in space, spacecraft, and technology in general. In this paper we propose a deep learning method, specifically a bidirectional long short-term m
Externí odkaz:
http://arxiv.org/abs/2203.14393
Autor:
Abduallah, Yasser, Wang, Jason T. L., Shen, Yucong, Alobaid, Khalid A., Criscuoli, Serena, Wang, Haimin
The Earth's primary source of energy is the radiant energy generated by the Sun, which is referred to as solar irradiance, or total solar irradiance (TSI) when all of the radiation is measured. A minor change in the solar irradiance can have a signif
Externí odkaz:
http://arxiv.org/abs/2107.11042