Works matching IS 17439213 AND DT 2023 AND VI 18 AND IP S372
Results: 13
Spatio-temporal Characterization of Hot Chromospheric Fibrils.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 123, doi. 10.1017/S1743921323001199
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Study of the Impact of Coronal Rain on Kink Oscillations of Coronal Loops.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 119, doi. 10.1017/S1743921323000534
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Automatic detection of solar active regions from SOHO/MDI and SDO/HMI synoptic magnetograms.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 94, doi. 10.1017/S1743921323000509
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Long-term Evolution of Magnetic Field Proxies as Deduced from Archival Data.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 84, doi. 10.1017/S1743921323000467
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A new mechanism for the butterfly diagram of the solar cycle.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 91, doi. 10.1017/S1743921323000455
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Origin of extreme solar eruptive activity from the active region NOAA 12673 and the largest flare of solar cycle 24.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 62, doi. 10.1017/S1743921323000285
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Photospheric magnetic field variation during solar flares and their implication for the generation of sunquakes.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 88, doi. 10.1017/S1743921322005026
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Observational Signature of Tilt Quenching of Bipolar Magnetic Regions in the Sun.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 86, doi. 10.1017/S1743921322005002
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Automatic Algorithm for Tracking Bipolar Magnetic Regions.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 97, doi. 10.1017/S1743921322004975
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Image refinement and estimations of radiation formation heights with the Deep Solar ALMA Neural Network Estimator.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 150, doi. 10.1017/S1743921322004859
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How has the solar wind evolved to become what it is today?
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 103, doi. 10.1017/S1743921322004756
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Spectroscopic Detection of Alfvénic MHD Waves in the Sunspot Chromosphere.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 110, doi. 10.1017/S1743921322004744
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Solar Observations with ALMA: A New Frontier.
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- Proceedings of the International Astronomical Union, 2023, v. 18, n. S372, p. 28, doi. 10.1017/S1743921322004586
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