Showing 61 - 66 results of 66 for search '"solar flares"', query time: 0.04s Refine Results
  1. 61

    Mask-Pix2Pix Network for Overexposure Region Recovery of Solar Image by Dong Zhao, Long Xu, Linjie Chen, Yihua Yan, Ling-Yu Duan

    Published 2019-01-01
    “…For example, during solar flare, Atmospheric Imaging Assembly (AIA) of Solar Dynamics Observatory (SDO) often records overexposed images/videos, resulting loss of fine structures of solar flare. …”
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    Article
  2. 62

    Correlation of the Flux of Energetic Rays and Particles with the Solar Cycle by Ehsan Tavabi, Sima Zeighami, Ali Aleali

    Published 2022-10-01
    “…A solar flare is a sudden flash that occurs near the solar surface. …”
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    Article
  3. 63

    Forecasting >300 MeV SEP Events: Extending SPARX to High Energies by C. O. G. Waterfall, S. Dalla, M. S. Marsh, T. Laitinen, A. Hutchinson

    Published 2023-06-01
    “…Correlations between SEP peak flux and peak intensity of the associated solar flare are seen to be weak at high energies, but improved when events are grouped based on the field polarity during the event. …”
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    Article
  4. 64

    A Regional Ionospheric Storm Forecasting Method Using a Deep Learning Algorithm: LSTM by Panpan Ban, Lixin Guo, Zhenwei Zhao, Shuji Sun, Tong Xu, Zhengwen Xu, Fengjuan Sun

    Published 2023-03-01
    “…In constructing the model, a number of correlated factors were used as inputs, including the properties of coronal mass ejections, solar flare bursts, interplanetary conditions, and geomagnetic and ionospheric states, and the output was whether an ionospheric storm occurred locally in the next 24 hr. …”
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    Article
  5. 65

    Constraining Solar Wind Transport Model Parameters Using Bayesian Analysis by Mark A. Bishop, Sean Oughton, Tulasi N. Parashar, Yvette C. Perrott

    Published 2025-01-01
    “…Such Bayesian analysis is readily extended to more sophisticated solar wind models, space weather models, and might lead to improved predictions of, for example, solar flare and coronal mass ejection interactions with the Earth.…”
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  6. 66

    Super‐Intense Geomagnetic Storm on 10–11 May 2024: Possible Mechanisms and Impacts by S. Tulasi Ram, B. Veenadhari, A. P. Dimri, J. Bulusu, M. Bagiya, S. Gurubaran, N. Parihar, B. Remya, G. Seemala, Rajesh Singh, S. Sripathi, S. V. Singh, G. Vichare

    Published 2024-12-01
    “…Further, an HF radio blackout was found to occur in the 2–12 MHz frequency band due to strong D‐ and E‐region ionization resulting from a solar flare prior to this storm.…”
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    Article