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Sympathetic Solar Eruption on 2024 February 9
DOI: 10.1088/1674-4527/ad9a33 Bibcode: 2025RAA....25a5006L

Feng, Li; Li, Shu-Yue; Zhang, Qing-Min +4 more

In this paper, we perform a follow-up investigation of the solar eruption originating from active region 13575 on 2024 February 9. The primary eruption of a hot channel generates an X3.4 class flare, a full-halo coronal mass ejection (CME), and an extreme-ultraviolet (EUV) wave. Interaction between the wave and a quiescent prominence (QP) leads to…

2025 Research in Astronomy and Astrophysics
SOHO 0
A Statistical Study of Magnetic Flux Emergence in Solar Active Regions Prior to Strongest Flares
DOI: 10.1088/1674-4527/ad2e4d Bibcode: 2024RAA....24d5014K

Abramenko, Valentina I.; Kutsenko, Alexander S.; Plotnikov, Andrei A.

Using the data on magnetic field maps and continuum intensity for Solar Cycles 23 and 24, we explored 100 active regions (ARs) that produced M5.0 or stronger flares. We focus on the presence/absence of the emergence of magnetic flux in these ARs 2–3 days before the strong flare onset. We found that 29 ARs in the sample emerged monotonically amidst…

2024 Research in Astronomy and Astrophysics
SOHO 1
Resolution Enhancement of SOHO/MDI Magnetograms
DOI: 10.1088/1674-4527/ad3b3b Bibcode: 2024RAA....24f5029Q

Qin, Ying; Yu, Xiao-Guang; Ji, Kai-Fan +1 more

Research on the solar magnetic field and its effects on solar dynamo mechanisms and space weather events has benefited from the continual improvements in instrument resolution and measurement frequency. The augmentation and assimilation of historical observational data timelines also play a significant role in understanding the patterns of solar m…

2024 Research in Astronomy and Astrophysics
Hinode SOHO 0
A Revised Graduated Cylindrical Shell Model and its Application to a Prominence Eruption
DOI: 10.1088/1674-4527/acee4d Bibcode: 2023RAA....23l5004Z

Zhang, Qing-Min; Hou, Zhen-Yong; Bai, Xian-Yong

In this paper, the well-known graduated cylindrical shell (GCS) model is slightly revised by introducing longitudinal and latitudinal deflections of prominences originating from active regions (ARs). Subsequently, it is applied to the three-dimensional (3D) reconstruction of an eruptive prominence in AR 13110, which produced an M1.7 class flare an…

2023 Research in Astronomy and Astrophysics
PROBA-2 SOHO 2
Super-resolution of Solar Magnetograms Using Deep Learning
DOI: 10.1088/1674-4527/ac78ce Bibcode: 2022RAA....22h5018D

Xu, Long; Zhao, Dong; Dou, Fengping +2 more

Currently, data-driven models of solar activity forecast are investigated extensively by using machine learning. For model training, it is highly demanded to establish a large database which may contain observations coming from different instruments with different spatio-temporal resolutions. In this paper, we employ deep learning models for super…

2022 Research in Astronomy and Astrophysics
SOHO 11
Analyzing Dominant 13.5 and 27 day Periods of Solar Terrestrial Interaction: A New Insight into Solar Cycle Activities
DOI: 10.1088/1674-4527/ac7129 Bibcode: 2022RAA....22h5005S

Saikia, Eeshankur; Syiemlieh, Rissnalin; Adhikary, Manashee +1 more

Our analysis presents an explanation of the Sun-Earth coupling mechanism during declining phase of a solar cycle, and how the dominant 13.5 and 27 day periods play roles in the coupling mechanism which led to intense terrestrial magnetic storms during this declining phase compared to the rising phase of a solar cycle. Moreover, it is observed that…

2022 Research in Astronomy and Astrophysics
SOHO 1
Ensemble Numerical Simulations of Realistic SEP Events and the Inspiration for Space Weather Awareness
DOI: 10.1088/1674-4527/ac3adb Bibcode: 2022RAA....22b5003D

Li, Gang; Wang, Xin; Luo, Bingxian +5 more

The solar energetic particle (SEP) event is a kind of hazardous space weather phenomena, so its quantitative forecast is of great importance from the aspect of space environmental situation awareness. We present here a set of SEP forecast tools, which consists of three components : (1) a simple polytropic solar wind model to estimate the backgroun…

2022 Research in Astronomy and Astrophysics
SOHO 0
How much has the Sun influenced Northern Hemisphere temperature trends? An ongoing debate
DOI: 10.1088/1674-4527/21/6/131 Bibcode: 2021RAA....21..131C

Henry, Gregory W.; Solheim, Jan-Erik; Scafetta, Nicola +20 more

In order to evaluate how much Total Solar Irradiance (TSI) has influenced Northern Hemisphere surface air temperature trends, it is important to have reliable estimates of both quantities. Sixteen different estimates of the changes in TSI since at least the 19th century were compiled from the literature. Half of these estimates are "low…

2021 Research in Astronomy and Astrophysics
SOHO 44
Class imbalance problem in short-term solar flare prediction
DOI: 10.1088/1674-4527/21/9/237 Bibcode: 2021RAA....21..237W

Wan, Jie; Fu, Jun-Feng; Liu, Jin-Fu +3 more

Using data-driven algorithms to accurately forecast solar flares requires reliable data sets. The solar flare dataset is composed of many non-flaring samples with a small percentage of flaring samples. This is called the class imbalance problem in data mining tasks. The prediction model is sensitive to most classes of the original data set during …

2021 Research in Astronomy and Astrophysics
SOHO 11
Predicting the CME arrival time based on the recommendation algorithm
DOI: 10.1088/1674-4527/21/8/190 Bibcode: 2021RAA....21..190S

Luo, Bingxian; Liu, Zhu; Li, Ming +9 more

CME is one of the important events in the sun-earth system as it can induce geomagnetic disturbance and an associated space environment effect. It is of special significance to predict whether CME will reach the Earth and when it will arrive. In this paper, we firstly built a new multiple association list for 215 different events with 18 character…

2021 Research in Astronomy and Astrophysics
Hinode SOHO 5